Session 7 Understanding ore systems though precise geochronology, isotope tracing and microgeochemistry Close Close Chapter 7-1 7-1 Origin of titanomagnetite-ilmenite mineralization, Arsentyev gabbro-syenite massif, Transbaikalia, Russia Roza Badmatsyrenova, Dmitriy Orsoev Geological Institute SD RAS, Ulan-Ude, Russia Abstract. The study of endogenic titanomagnetite-ilmenite ores are of interest as they present a number of petrologic problems. One such problem is determining their genetic connection with alkalimafic and mafic complexes and associated phosphorus enrichment. The Arsentyev gabbro-syenite massif is representative of these systems and provides an ideal situation in which a detailed study allows further understanding of interrelated magmatic and ore-formation processes. It is shown that an oxide-ore liquid separated from a parental silicate melt during early stages of subalkaline mafic magma crystallization. Keywords. Liquid immiscibility, geochemistry, ore mineralization 1 Introduction Titanomagnetite-ilmenite ores sourced from various deposits are considered as a premier source of commercial iron and vanadium. Select deposits additionally contain significant titanium enrichment providing a mineral source for titanium production. Currently ores from large tonnage, high grade deposits are now mined from Bushveld (the South Africa Republic), Lac-Tio (Canada), Panzhihuan (China), Kachkanar (Russia). Ore occurrences are known in the Urals, Kareliya, East Sayan, Transbaikalia, and Far East. The Arsentyev gabbro-syenite massif with titanomagnetite-ilmenite mineralization is representative of this association. Understanding iron ore deposit genesis is problematic, with particular difficulties in rectifying magmatic titanomagnetite-ilmenite deposits formation, yet a comprehensive understanding is essential for exploration. Therefore, studies identifying genetic processes occupies a special place in the analysis of ore genesis in magmatic systems. In addition to fundamental understanding, the study of already known of ore complexes is necessary for development of prospecting criteria and interpretations of results, which may form the basis for rating production feasability of titanomagnetite-ilmenate ores. 2 and have the geochemical signature of alkaline basalts. Two intrusive phases, each of them being followed by formation of dike complexes, form the Arsentyev massif (Fig. 1b). The first phase consists of a stratified series pyroxenites, olivine and kersutite gabbros, gabbros, anorthosites and syenite. The second phase includes the rocks of the syenite series. The titanomagnetite-ilmenite mineralization is confined to the stratified gabbro-anorthosite series. This mineralization is subdivided into syngenetic and epigenetic by morphological features and degree of localization. The widespread syngenetic mineralization is represented by disseminated and net-textured ores while the restricted epigenetic mineralization is represented by massive ores. As a rule, disseminated ores are confined to apatite-free and apatite ore gabbros and pyroxenites with 10 to 25 vol.% ore minerals. Ore gabbros are advanced among most differentiated intrusive region, where they alternate with leucogabbro (up to anorthosite) and gabbro. The thickness of orebodies are highly variable but prevail as ventricular and vein ore. The massive ores are usually contained within area associated with disseminated and net-textured ores and are related to protomagmatic fracturing. The contact between ore bodies with host gabbroids are tectonic as a rule. Geological setting and structure The Arsentyev massif is located at the central part of the Monostoy ridge west of the Arsentyevka village (Fig. 1a). The massif outcrops over a 20 km2 area. The Arsentyev massif is defined by intrusions of syenite-pyroxenite-gabbro with a high titanium ultramafic-mafic association (Badmatsyrenova et al. 2004). These intrusions are related to rift-like structures of various ages Close 726 Roza Badmatsyrenova · Dmitriy Orsoev 3 Mineral composition and geochemistry The disseminated ores are divided into titanomagnetiteilmenie ore and apatite-titanomagnetite-ilmenite ore with apatite contents of 10-15 wt.%. Apatite-titanomagnetiteilmenite ores have a subordinate value. Magnetite and ilmenite are the main ore minerals. They are intimately associated, forming xenomorphic aggregates interstial to silicate minerals and always crystallizing after the silicates. The grains size varies from 0.04 to 3 mm. They also occur as small inclusions in pyroxene, kersutite and plagioclase but in insignificant amounts. The separate grains of magnetite and ilmenite display variable degrees of isomorphism depending on their quantitative ratio. Both “homogeneous” magnetite having roughly a pure iron composition and titaniferous magnetite with dissolution structures are observed. Ilmenite also has variable composition based on the concentration of Fe3 +. In addition to ore minerals and apatite, the ores contain varying amounts of olivine, pyroxene and plagioclase. Amphibole and biotite are also present. Sulphides and spinel are present but economically insignificant compared to the apatite-titanomagnetite-ilmenite ores. The apatite-bearing ores have significantly more sulphides and spinel compared to the massive and disseminated irontitanium ores. The mineral composition of massive ores is rather restricted. The ore is dominated (70-90 vol.%) by aggregates of magnetite, titanomagnetite and ilmenite. Magnetite is the dominant ore mineral with a half to a third as much ilmenite. The grains of ore minerals are larger, up to 5 mm, in massive ores compared with disseminated ore minerals. Separate, fine-grained pyrite, pyrrhotite, chalcopyrite, marcasite and pentlandite are present in the ores at insignificant amounts. The constant presence of apatite at insignificant amounts and increased contents of spinel (up 10-30%) are characteristic of the massive ores. Kersutite is also present. Titanomagnetite from the massive ore contains 6.48 wt.% TiO2 and is seen as thin intergrowths of magnetite, ilmenite, spinel and ulvöspinel(?). Trellised or reticulated titanomagnetite from ore gabbros contain appreciablly less TiO2 (0.18-0.91 wt.%). Finally, titanomagnetite from host gabbros contains only TiO2 (0.06-0.08 wt.%). The concentration of TiO2 in ilmenite forming lamellar inclusion in titanomagnetite found in disseminated ore is 48.68 wt.% while concentration of TiO2 in massive ore is 53.31 wt.%. Spinel in disseminated ores contain 0.1 to 0.3 wt.% TiO2, whereas spinel from massive ores forming tear-shaped structures of immiscibility in magnetite contains TiO2 up 4.94 wt.% and in ilmenite in massive ore contains 0.96 wt.% TiO2. Manganese concentration in ilmenite is 0.52 to 1.57 wt.%. Mn in magnetite is 0.07 to 0.19 wt.%. The magnesium contents in magnetite-bear- ing ore much more exceeds (up to 1.57 wt.%) contents in ore gabbro and gabbro (0.08 wt.%). Mg concentrates in lamella of ilmenite in massive ores are 7.94 wt.%. The aluminium in magnetite in massive ores contains up to 1.73 wt.%. The maximum contents Al in rocks are 0.11 wt.%. Ilmenite is aluminum-poor (0.06 wt.% Al2O3). Dissolution structures in massive ores are present with Al2O3 up to 5.55 wt.%. Aluminium in titanomagnetite is associated with spinel intergrowths. Amphibole (TiO2 up to 6 wt.%) is identified as an accessory mineral in ores. Large kersutite crystals are distinctly brown colour and pleochroic suggesting greater Fe and Ti content. Analyzed amphibole have the high contents Al2O3, Ti and alkalis in comparison with gabbro from other units. Biotite in massive ore is FeO deficient with proportionaly more MgO, TiO2, Na2O than in dissiminated ores. Clinopyroxene composition directly correlates to plagioclase composition. The most magnesian pyroxene (MgO 14.56 wt.%) is associated with the most basic plagioclase (An40). The pyroxene Mg# changes from 80 to 74 %. Fayalite olivine is enriched with increasing ore abundances. Nickel contents correlate with the olivine. Apatite is often the only mineral in mafic rocks that yield information about volatile composition. Fluorapatite is found in gabbros and ores of the Arsentyev massif. The fluorine contents in ores (1 to 2 wt.%) is noticeably less than in gabbro (2 to 3.5 wt.%). High fluorine and phosphorus concentrations in connection with increased alkalinity of the primary basalt magma facilitates volatile immiscibility and support ore cluster formation. REE concentrations in apatite from gabbro have typical for basalt distribution: the relative concentration of lanthanides increases from HREE to LREE, the degree of division is marginal (La/Yb = 21-36), and a negative Europium anomoly is evident. Conversely, apatite from ores does not have a negative Europium anomoly. The new data does not contradict immiscibility of titanomagnetiteilmenite ores and apatite formation. The geochemical data suggest an iron-bearing silicate melt of large anion trivalent iron complexes (Fe2O42 -) formed after oxidation by interaction with alkaline oxide components and water. The predominance of oxidic iron in magnetite points to an oxidizing environment. It is probable that the formation of anion complexes Fe2O42- instead of cation of bivalent iron facilitates initiation of immiscibility in the melt system resulting in an ore-forming and a silicate liquid. 4 Conclusions Microprobe analysis shows that magnetite, ilmenite, amphibole and biotite of the massive ores are significantly richer in TiO2, Al2O3, MgO and Na2O than the minerals Close Chapter 7-1 · Origin of titanomagnetite-ilmenite mineralization, Arsentyev gabbro-syenite massif, Transbaikalia, Russia of the disseminated ores. The massive ores are characterized by high V (1400 to 1600 ppm), Zn (200 to 500 ppm), and Cr (21 to 36 ppm) concentrations and low concentrations of Sr (60 to 210 ppm), Co (73 to 112 ppm) and P2O5 (0.06 to 0.21 ppm) compared to the disseminated ores that have very high concentrations of the main components (TiO2, Fe2O3 and FeO). Variations in ore compositions are illustrated on the ratio plots of petrogenic and trace elements. A later independent formation of the massive ores is indicated by significantly lower values of Cr/ V and Ni/Co ratios than in the disseminated ores if using these ratios as indicators of ore formation stages. Using classification based on chemical composition, the ores of the Arsentyev massif belong to the iron-titanium-vanadium type. The study of distribution of noble metals has shown that the ores have platinum enrichment: Pt contents of massive ores are up to 6.3 ppb and Ag contents up to 2.8 ppm while Pt contents of disseminated one are < 2 ppb and Ag 1 ppm. 727 Conditions favorable for phosphorus induced liquid immiscibility can be expected in silicate-salt melts (Krigman, Krot 1991), or immiscibility may be induced by another component, possibly ferrous iron complexes. For example, it is possible to form gabbroid complexes associated with apatite-ilmenite and titanomagnetite mineralization, which, in opinion of some researchers (McBirney, Nakamura 1974, Marakushev 1987), is connected to immiscibility decomposition of the parental melt into a salic and a femic melt, where the latter representing an ore magma with the contents P2O5 7 to 8%. Two genetic ore types in the Arsentyev massif are allocated: the first type, massive titanomagnetite-ilmenite ores, are of immiscibility genesis while the second type, ore gabbro, formed in result of crystallization differentiation of a basalt magma. Acknowledgements This work was supported by the Russian Foundation for Basic Research (grant No 05-05-97246), Russia President grant for leading science school No Sh-2284.2003.5, Russian Science Support Foundation. References Badmatsyrenova RA, Orsoev DA (2004) Computer simulation of titanomagnetite-ilmenite mineralization formation, Arsentyev massif, Transbaikalia, Russia. In: Proc. of the Interim IAGOD Conference, Vladivostok, Russia, 1-20 September, 2004, pp. 407-410 Krigman LD, Krot TV (1991) Stable phosphate-aluminosilicate liquation in magmetic melts Geokhimia. 11: 1548-1561 (in Russian) Marakushev AA (1987) Geology and mineralogy of the anorthosite associations. Vladivostok, p.17 (in Russian) McBirney A.K., Nakamura Y (1974) Ann. Report Director geophys. Lab. Washington, 348 pp Close Close Chapter 7-2 7-2 Direct dating of ore minerals: A feasibility study of the Pb-Pb isotope step-leaching technique K. Bassano, J. Hergt, R. Maas, J. Woodhead pmd*CRC, School of Earth Sciences, The University of Melbourne, Australia Abstract. Pb-Pb step-leaching (PbSL) is a digestion technique based on sequential acid treatment of a mineral resulting in the selective recovery of radiogenic and common Pb components from the crystal lattice, making single-phase Pb-Pb dating possible. Developed originally by R. Frei and colleagues at Bern, the technique was recently applied to Proterozoic garnets to test the reliability of PbSL as a dating tool in multiply deformed terranes (Tonelli 2002). This study builds on previous observations and tests the reliability of PbSL in directly dating ore minerals such as sulfides (chalcopyrite, pyrite, pyrrhotite/pentlandite) and oxides (magnetite), thereby obtaining the timing of mineralisation from a phase that is unambiguously linked to the ore-forming process. This is based on the often surprisingly high U contents (relative to what might be anticipated), yielding rather higher than expected initial U/Pb ratios in several types of low-Pb sulfides. The technique is applied to well-constrained samples from a number of predominately Australian mineral deposits covering a range of mineralization types. Keywords. Pb-Pb, step-leaching, ore minerals, direct dating 1 Introduction The mechanism of Pb isotope unmixing in step-leaching was examined by Frei et al. (1997) who proposed two main processes; the surface/crystallographic site dependent hydrolysis of metal cations, and the progressive remobilisation of radiogenic Pb from the leached gel-like structure. Different rates of these processes during progressive leaching results in an effective separation of common and radiogenic Pb, producing generally linear unmixing arrays with age significance in the 206Pb/204Pb vs 207Pb/204Pb diagram. Benefits of PbSL over bulk U-Pb and Pb-Pb techniques include the ability to: – detect sub-microscopic U-rich inclusions using the distinct variations in 208Pb/206Pb (i.e. time-integrated Th/U) between host mineral and inclusions such as zircon or monazite – date a wide range of minerals with low-U; minerals generally thought to be unfavourable for conventional U/Pb dating – obtain ‘single’-mineral isochron ages without the need for analysing associated minerals to produce isotopic dispersion on isochrons Although previous authors (eg Collerson et al. 2002) have obtained age estimates on (mixed) ore minerals using PbSL prior to this study, further investigation is re- quired into the circumstances in which this technique may/ may not be reliably applied. 2 Discussion In this study the technique has been applied to well-constrained samples from a number of Australian ore deposits, including the analysis of chalcopyrite and magnetite from Broken Hill (BHT), Mt Isa, Ernest Henry (IOCG) and Osborne (IOCG). Magnetite and pentlandite/pyrrhotite from the Merensky Reef in the Bushveld Complex have also been studied. Studies of chalcopyrite from Copper Blow (Broken Hill) yielded promising results. Lead isotope ratios obtained, particularly in the second leach step, indicate the presence of radiogenic Pb with 206Pb/204Pb ratios ranging up to ~57. As chalcopyrite at Copper Blow occurs with torbernite (U-rich), typical grains were interrogated using the SEM to confirm that the Pb compositions reflect those of the chalcopyrite and not inclusions. Results for magnetite from the same deposit display greater spread in the 206Pb/204Pb (~23 to 183). The age estimates obtained from these co-genetic minerals are the same (magnetite: 1094±89Ma; MSWD=250; chalcopyrite: 1071±210; MSWD=213), to within error, although the uncertainties are quite large. Unlike the 206Pb/204Pb and 207Pb/204Pb ratios of these samples, 208Pb/204Pb displays very little variation, retaining values typical of common lead (~37 to 38). This indicates that the mineralising fluid from which these phases grew carried U but not Th into the system. Both chalcopyrite and magnetite were also analysed from the Osborne deposit. The chalcopyrite displays radiogenic values (206Pb/204Pb ~20 to 48) that generate an age estimate of 1252±190Ma. Preliminary studies at Ernest Henry indicate the samples are also highly radiogenic. Chalcopyrite shows a large spread in 206Pb/204Pb (~18 to 257) generating an age estimate of 1590±17Ma (MSWD=1). The variation in 206Pb/204Pb ratios displayed by the associated magnetite is even greater (~214 to 965) although the scatter is considerable. These data yield a poorly constrained age of 1044±450Ma because, although the range in ratios is considerable, ‘gaps’ in the array contribute to the large errors obtained as the isochrons become dominated by one or two points. Further analyses of these samples with varied leaching protocols produced consistently scattered data sets. Close 730 K. Bassano · J. Hergt · R. Maas · J. Woodhead In order to determine if the technique is producing the ‘correct’ age estimates, three samples from the Merensky Reef in the Bushveld Complex, South Africa (two magnetites and one mixed pyrrhotite /pentlandite sulfide) where analysed. Samples from this orthomagmatic deposit were selected due to the generally widely excepted age of the Bushveld Complex ore system. The resulting leach steps from each of these samples displayed little or practically no spread in 206Pb/204Pb and 207Pb/204Pb. The majority of the age estimates generated from this data fall within error of the “known” age of the Merensky Reef, however the uncertainties are large, most likely due to the minor data spread. 3 Evaluation of the leaching process ICPMS trace element analyses of the study samples have been undertaken in order to examine possible causes for the apparently variable success of this technique. First, the U and Pb contents of bulk-separates will clearly influence how much radiogenic ingrowth can occur relative to the common Pb component, and hence how great the spread in the Pb isotope ratios may be during stepleaching. How this varies between particular ore deposit types is a central question of this study. Another important question is to determine the factors that control the retention or mobility of different elements (particularly Pb, but also how this behaves relative to other trace elements). The acid leaching mechanism cannot be the same as that determined in the step-leaching experiments of silicates (where Si-O bonds are broken during hydrolysis reactions). The assessment of trace element mobility is conducted via analysis of the leachates from different leach steps, and comparisons between these and data for bulkseparates. Finally, the extent to which variations in the initial Pb isotope composition within samples has influenced the scatter in isochrons will be explored. This involves the analysis of numerous separate aliquots of material to check for levels of heterogeneity in their Pb isotope compositions. Acknowledgements The authors would like to thank the many members of the pmd*CRC who have provided us with the well-constrained materials required for this study. References Collerson KD, Kamber BS, Schoenberg R (2002) Applications of accurate, high-precision Pb isotope ratio measurements by multicollector ICP-MS. Chem Geol 188: 65-83 Frei R, Villa IM, Nagler ThF, Kramers JD, Przybylowicz WJ, Prozesky VM, Hofmann BA, Kamber BS (1997) Single mineral dating by the Pb-Pb step leaching method: Assessing the mechanisms. Geochim Cosmochim Acta 61: 393-414 Tonelli M (2002) An evaluation of Pb step leaching geochronology as applied to high-grade metamorphic terranes. PhD Thesis, University of Melbourne (unpubl) Close Chapter 7-3 7-3 Rutiles in eclogite from the Sulu UHPM Terrane: A preliminary study Chen Zhenyu, Chen Yuchuan, Wang Denghong, Xu Jue, Zhou Jianxiong Institute of Mineral Resources, Chinese Academy of Geological Science, Beijing, 100037, China Abstract. In recent years more than 40 rutile-bearing eclogite ore bodies have been discovered among the thousands of eclogite bodies in the Sulu Utra-High Pressure Metamorphic (UHPM) terrene. Rock- and ore-cores obtained by the Chinese Continental Scientific Drilling (CCSD) Project revealed the presence of several hundred meters of rutile-bearing eclogites. This paper presents a preliminary petrographic, trace element, and Pb isotope study of rutile ores in eclogite. Rutiles occur as inclusions, intergranular infillings, remnant replacements, and hydrothermal infillings in the host rocks. The ore minerals define four stages of rutile mineralization and metamorphic evolution in the eclogites. Electron microprobe (EMP) trace element analysis of three rutile specimens show that different occurrences of eclogite also have different trace element compositions in rutile. These compositional differences may reflect different source rocks for the eclogites. Peak metamorphic temperatures were calculated using the Zr geothermometer in rutile. The Pb isotopic compositions of rutile obtained by step-fuse analysis of single grains of rutile did not fall on one growth line, but show similar variation between different samples. This implies that the Pb isotopic compositions of rutile may have been disturbed during its growth. This variation could be used to trace the growth history of the rutile, and further to trace the process of continental subduction- exhumation. Keywords. Rutile, eclogite, petrography, trace elements, Pb isotope, Sulu UHPM terrene 1 Introduction The Sulu ultra-high pressure metamorphic (UHPM) terrene is the product of the Triassic collision involving the north China and Yangtze cratons. There are thousands of eclogite bodies of different size and occurrence in the UHPM belt in the Sulu terrene, and more than 40 rutile-bearing eclogite ore bodies have been recently discovered. The total reserves of rutile ore amount to several million tons (Huang J P., et al. 2003). The main hole of the Chinese Continental Scientific Drilling (CCSD) project is located at Maobei, Donghai, in the southern part of the Sulu UHPM terrene (a simplified geological map is showed in Fig. 1). Drilling to 5100m at this locality has recently completed. Rock- and ore-cores obtained by the CCSD revealed rutile-bearing eclogites amounting to several hundred meters (Xu et al. 2004). The rutile deposit in the Sulu UHPM terrene is a typical eclogite-type rutile deposit. To assess the relationship between UHPM and the mineralization of rutile in eclogite, we have conducted a preliminary study on the rutile from the main hole of the CCSD. In this study we focus on the different rutile occurrences, petrography, trace element composition and Pb isotopic composition. 2 Petrography of rutile and titanium minerals in eclogite The rutile ore bodies mainly occur in massive eclogites, as strips and lenses. Rutile-bearing eclogites have at least three different occurrences: (1) xenoliths in ultra-mafic serpentines, e.g. in Xugou and Jiangzhuang; (2) lenses in marbles e.g. in Yanmachang and Banzhuang; (3) metamorphosed intrusive complex rocks in Donghai. The eclogites show variable mineral assemblages and chemical compositions, and indicate diverse origins for their protoliths (Zhang et al. 2004). The observation and documentation of both the rock- and ore-cores obtained by CCSD reveal that the major titanium mineral phases of economic interest are rutile and titano-magnetite. The most important ore-bearing rock types are normal rutile eclogite, quartz eclogite associated with phengite-rutile eclogite and kyanite-rutile eclogite. The modal content of rutile in eclogite is 2%~5% (vol.) and is as high as 8%~10% (vol.) (Xu et al. 2004). Detailed petrographic investigation reveals that rutile in eclogite mostly occurs in four types: (1) as inclusions in garnets, omphacites or zircons, which may have crystallized during prograde metamorphism (coesite or its pseudomorph can be found coexisting with rutile in the same garnet, omphacite or zircon host); (2) as intergranular infilling grains between garnets and omphacites. In Close 732 Chen Zhenyu · Chen Yuchuan · Wang Denghong · Xu Jue · Zhou Jianxiong this stage, metamorphism reached its peak conditions, and rutile crystallized simultaneously with eclogite-face minerals such as garnets and omphacites. This is the main crystallization stage of rutile; (3) as replacement remnant, at the amphibolite-face retrograde metamorphism stage. Garnets and omphacites are altered to hornblende and plagioclase. Rutlie is also partly altered to ilmenite or titanite; (4) as hydrothermal infilling forms. Rutile fills in the cleavages and cracks as veins, strings or megacrysts. This rutile occurrence may have crystallized at the greenschist-facies metamorphic stage. At this time, hydrothermal fluids extracted components of mineralization from wall rocks and deposited them in cleavages and cracks in the rocks. On the other hand, the early rutile phase is partly or totally altered to ilmenite or titanite. As for the above-mentioned four occurrences, the second one is the most abundant, and accounts for about 90% of the gross rutile ore reserves. Rutile and titano-magnetite that were altered to ilmenite and titanite during retrogressive metamorphism led to a drop in grade of the titanium mineralization. content of these elements, averaging 615ppm, 324ppm, 3457ppm and 3333ppm for Cr, Nb, Fe and V respectively. In the Nb-Cr diagram defined by Zack, et al. (2004b), protoliths of these three eclogites all plot in the “mafic rocks” field. Temperature calculated from Zr content in rutile showed that the peak temperature of metamorphism for these eclogites was 550~575o for Qinglongshan, 565~615 o for Banzhuang and ~716 o for Machang. These temperature values are comparable with those calculated by the cation-exchange geothermometer of host minerals. 4 3 Pb isotopic composition of rutile Trace elements in rutile Rutile has long been considered to be an important carrier of high field strength elements (HFSE; Zr, Nb, Mo, Sn, Sb, Hf, Ta, W). It also plays a key role in subduction zones by retaining HFSE in the restite/residuum during dehydration and melting reactions. Recent studies by Zack et al. (2002, 2004a, 2004b) show that the trace elements in rutile can give us more information than just the dominant control of HFSE in eclogite. For example, the Nb, Cr content in rutile can be used to distinguish different protoliths of rutile-bearing eclogites. Additionally, the Zr content in rutile is temperature dependent and can be used as a geothermometer in rutile. In this study, we used a JXA-8800R electron microprobe to determine the trace element composition of rutiles in eclogites from Machang, Qinglongshan and Banzhuang. The Machang and Qinglongshan samples occur in metamorphosed intrusive complex rocks, and the Banzhuang samples occur as lenses in marbles. Particular operating conditions were used to obtain low detection limit (20kV, 100nA and 100~300s counting time, which resulted in a detection limit of elements of interest in the 20~30ppm range). Analytical results (Table 1) show that rutiles in eclogite from Machang have the lowest content of Cr and Nb, averaging ~89ppm and mostly below the detection limit. However, these rutiles also have the highest Fe and V content, averaging 5390ppm and 3853ppm respectively. Rutiles in eclogite from Banzhuang show the highest Cr and Nb content, averaging ~1574ppm and ~385ppm respectively; but they also show the lowest Fe and V content, averaging 2602ppm and 2114ppm respectively. Rutiles in eclogite from Qinglongshan have moderate To obtain the U-Pb age of rutile in eclogite from the Sulu UHPM terrene, we selected three rutile specimens for UPb isotope analysis by the step-fuse method. Unfortunately, we could not obtain a correct age because of the very low content of radiogenic Pb isotopes in rutile. But, to our surprise, the Pb isotopic compositions (206Pb/204Pb, 207Pb/ 204Pb, 208Pb/204Pb) obtained from a series of step-fuse analyses of a single grain from its shell to its core can not be plotted on one growth line. This means that Pb isotopic ratios can not be attributed to in-situ Pb growth. Franz et al. (2001) found a similar phenomenon when they tried to determine the U-Pb age of a rutile specimen in an eclogite-facies quartz vein within a metabasalt in South Dabieshan. In their case, one 4-cm-long single crystal was divided into 3 small fragments, and each fragment was analyzed. The isotopic variability among these fragments was too large to be attributable to in situ Pb growth, and patterns on the 206Pb/204Pb-207Pb/204Pb and 206Pb/204Pb208Pb/204Pb are incompatible with secondary addition or removal of Pb (Franz et al. 2001) . The rutile in the quartz vein may have been crystallized in the retrograde fluid, so they considered the initial Pb composition of this specimen to be isotopically heterogeneous, which implies that the Pb in the fluid is isotoptically variable during rutile crystallization. In our case, the Pb isotopic compositions of these three specimens have shown abrupt variations at a certain middle step and at the final step of fuse analysis in a similar way. This implies that these three rutile specimens have similar Pb growth history. The two abrupt variations indicate that Pb isotopic compositions of rutile were disturbed twice during its crystallization. These disturbances may reflect the variation of geologic settings Close Chapter 7-3 · Rutiles in eclogite from the Sulu UHPM Terrane: A preliminary study during rutile growth, which can be used to infer continental subduction-exhumation processes. This suggests to us that the variation of Pb isotopic composition in rutile by step-fuse analysis may be used to trace the growth history of the rutile, and further to trace the process of continental subduction- exhumation. Although this is a preliminary discussion and needs further study and more evidence to support it, this approach has shown great potential in the study of the geodynamics of subduction zones. 5 Conclusions The rutile deposit in the Sulu terrene is genetically related to the UHPM. Rutile is mainly mineralized during eclogite-facies metamorphism. The alteration by retrogressive metamorphism leads to a drop in grade of the titanium mineralization. EMP was used to obtain trace element composition of different occurrences of rutile in eclogites. These analyses show variations in Nb, Cr, Fe and V content between each occurrence, which may be used to infer the protolith of these eclogites. Temperatures calculated from the Zr geothermometer in rutile are comparable with the results from other methods. This implies that the Zr geothermometer in rutile is a feasible and effective method for calculating peak metamorphic temperatures. Pb isotopic compositions obtained from step-fuse analysis of single grains of rutile may be potential tracers of rutile growth history. If so, this analytical technique could play an important role in furthering the understanding of continental subduction- exhumation processes. 733 Acknowledgements This study is supported by the Major State Basic Research Development Program (2003CB716501). We thank Parham Gardner for her critical reviews, which improved this paper significantly. References Franz L, Romer RL, Klemd R, Schmid R, Oberhansli R, Wagner T, Dong S (2001) Eclogite-facies quartz veins within metabasites of the Dabie Shan (eastern China): Pressuretemperature-time- deformation path, composition of the fluid phase and fluid flow during exhumation of high-pressure rocks. Contrib Mineral Petrol 141: 322-346 Huang JP, Ma DS, Liu C, Wang CL (2003) Character and origin of rutile deposit in eclogite in Xiaojiao, Xinyi, Jiangsu province. Geoscience 17: 435-443 Xu J, Chen YC, Wang DH, Yu JJ, Li CJ, Fu XJ, Chen ZY (2004) Titanium mineralization in the ultrahigh-pressure metamorphic rocks from Chinese Continental Scientific Drilling 100~2000m main hole. Acta Petrologica Sinica 20: 119-126 Yang JJ, Jahn BM. (2000) Deep subduction of mantle-derived garnet peridotites from the Su-Lu UHP metamorphic terrane in China. J. metamorphic Geol., 18: 167-180 Zack T, von Eynatten H, Kronz A (2004b) Rutile geochemistry and its potential use in quantitative provenance studies. Sediment Geol. 171: 37-58 Zack, T, Kronz, A, Foley S., River T (2002) Trace element abundances in rutiles from eclogites and associated garnet mica schists. Chem. Geol. 184: 97-122 Zack, T, Moraes, R, Kronz A (2004a) Temperature dependence of Zr in rutile: empirical calibration of a rutile thermometer. Contr. Min. Petrol. 148: 471- 488 Zhang ZM, Xu ZQ, Liu FL, Shen K, Yang JS, Li TF, Chen SZ (2004) Geochemistry of eclogites from the main hole (100~2050m) of the Chinese Continental Scientific Drilling Project. Acta Petrologica Sinica 20: 27-42 Close Close Chapter 7-4 7-4 A non-magmatic component in fluids of South American Fe oxide-Cu-Au deposits inferred from δ 37Cl, 87Sr/86Sri and Cl/Br M. Chiaradia1, D. Banks, R. Cliff School of Earth Sciences, University of Leeds, Leeds LS2 9JT, U.K. 1 Present address: Department of Mineralogy, University of Geneva, 1205-Geneva, Switzerland R. Marschik Department of Earth and Environmental Sciences, Ludwig-Maximilians University, 80333-München, Germany A. de Haller Department of Mineralogy, University of Geneva, 1205-Geneva, Switzerland Abstract. The magmatic versus basinal brine origin of the hypersaline fluids associated with iron oxide-copper-gold (IOCG) deposits is controversial. In this study we present and discuss the first stable chlorine and strontium isotope data, combined with Cl/Br ratios, of inclusion fluids of South American IOCG deposits. The isotopic and elemental signatures of South American IOCG deposits suggest either mixing of juvenile magmatic fluids with up to several tens wt.% of crustal brines or magmatic fluids leaching up to few wt.% of evaporite. Keywords. Iron oxide Cu-Au deposit, chlorine isotope, strontium isotope, fluid inclusion, Andes range between 3 and 7‰ (Magenheim et al. 1995) whereas crustal chlorine has δ37Cl values around 0‰ (Eggenkamp et al. 1995). In principle, therefore, chlorine isotopes are able to discriminate between heavy mantle- and light crust-derived chlorine. Additionally, since IOCG deposits constitute an end-member of a continuum with magnetite-apatite (Kiruna-type) deposits (Hitzman 2000), combined investigations of these two mineralization types increase our understanding of the origin of their hypersaline fluids resulting in improved exploration strategies. 2 1 Introduction Iron oxide-copper-gold (IOCG) deposits represent a hydrothermal mineralization style characterized by abundant magnetite and/or hematite, variable amounts of Cusulfides, pyrite, gold and REE, and intense and voluminous sodic ± calcic and potassic alteration (Hitzman et al. 1992). These deposits form at shallow to mid-crustal levels within cratonic or continental margin settings (Hitzman et al. 1992), and although they usually occur within magmatic rocks, they are not always clearly related to igneous activity. The most controversial aspect of IOCG deposits is the origin of their hypersaline fluids as either (i) fluids exsolved from magmas (e.g., Pollard 2002), or (ii) basinal brines heated by nearby intrusions (e.g., Barton and Johnson 1996). We report the first stable chlorine and strontium isotope data, as well as Cl/Br ratios, for inclusion fluids of four IOCG deposits and one magnetite-apatite deposit from South America. Chlorine is the dominant metal ligand in IOCG hypersaline fluids and behaves conservatively during fluid-rock interaction. Therefore, chlorine isotopic compositions, combined with strontium isotopes and Cl/Br ratios, may provide tighter constraints, compared to O and S stable isotope data, on the origin of IOGC fluids. The mean mantle δ37Cl value is 4.7‰ with a Ore deposits investigated, samples and techniques The investigated deposits belong to the Carajás Mineral Province (CMP), Brazil, and to the Peruvian and Chilean Andes (Fig. 1). The CMP consists of a Late Archean volcano-sedimentary sequence deposited upon high-grade tonalitic and trondhjemitic gneisses of the southern part of the Central Brazilian Shield. The region is subsequently intruded by 2.56-2.76 Ga alkaline and calc-alkaline granites and by 1.8-1.9 Ga anorogenic granites (Machado et al. 1991). Either a continental rift (Olszewski et al. 1986) or a subduction-related arc (Dardenne et al. 1988) geodynamic setting is suggested. Investigated CMP mineralization includes the Archean to Early Proterozoic Sossego and Gameleira deposits. The Cretaceous IOCG deposits of Candelaria (Chile), and Raul-Condestable (Peru) and the magnetite-apatite deposit of El Romeral (Chile) occur in the Andean Cordillera of Peru and Chile in extensional to transpressional arc settings (e.g. Sillitoe 2003). Geological, mineralogical, and stable isotope data (mostly O, S) indicate dominantly magmatic fluids formed Gameleira (Lindenmayer et al. 2001) and El Romeral, whereas mixed magmatic and non-magmatic fluids characterize Sossego (Marschik et al. 2003) Candelaria (Marschik and Fontboté 2001) and Raul-Condestable (de Haller et al. 2002). Close 736 M. Chiaradia · D. Banks · R. Cliff · R. Marschik · A. de Haller Selected fragments of quartz representing the primary ore stages at Raul-Condestable, Candelaria, Gameleira, and Sossego, apatite from El Romeral, as well as two calcites from the late ore stage at Sossego were sampled and crushed. The inclusion fluids were analyzed for stable chlorine and strontium isotope compositions by thermal ionization mass spectrometry (TIMS) and for Cl- and Brconcentrations by ion chromatography at the School of Earth Sciences (University of Leeds, U.K.). 3 Sources of chlorine and strontium in inclusion fluids Chlorine isotope compositions and Cl/Br ratios of hydrothermal fluids of South American IOCG and magnetiteapatite deposits plot along two distinct arrays (Figure 2), allowing discrimination between magmatic fluid-dominated deposits (Gameleira and El Romeral) and deposits with mixed magmatic and non-magmatic fluids (Sossego, Candelaria, Raul) consistent with previous geochemical studies. We interpret the two trends defined by fluids of the magmatic fluid-dominated (Gameleira, El Romeral) and mixed fluid (Candelaria, Raul-Condestable, Sossego) deposits as the result of mixing between a common mantle-derived magmatic fluid and two distinct crustal sources of chlorine both with near 0‰ δ37Cl values but with different Cl/Br values (Fig. 2). The trend defined by the magmatic fluids of Gameleira and El Romeral integrated with data from the magmatic fluids of the Capitan and SW-England plutons (Banks et al. 2000: Figure 2) is shifted to high Cl/Br values suggesting that chlorine is a mixture between mantle and halitederived chlorine, probably resulting from variable magmatic interaction with evaporites. A non-magmatic component at El Romeral is supported by the significantly more radiogenic strontium isotopic composition (87Sr/ 86Sr = 0.7065) of the fluid compared to that of the associi ated magmatic rocks (87Sr/86Sri ~ 0.703-0.704). The Sr isotope data addtionally suggest evaporite assimilation by high-temperature exsolved magmatic fluids rather than evaporite assimilation by the magma itself is responsible for the observed Cl and Sr isotope systematics of the inclusion fluid at El Romeral. We have calculated that assimilation of 2 to 9 wt.% halite by a mantle-derived magmatic fluid could cause the shift to the near 0‰ δ37Cl values and high Cl/Br ratios observed in the Gameleira, El Romeral and Capitan pluton fluids. The existence of evaporites in the host sequences of El Romeral (Chile) and Capitan pluton (Mexico) yields geological support to the above scenario. However, there is no evidence for evaporites in the CMP. As a result a fluid souce with ~0‰ δ37Cl and high Cl/Br ratios such as a hypersaline crustal brine may explain the data of Gameleira. The other IOCG deposits investigated (Sossego, Candelaria, Raul-Condestable) define a linear array in the Close Chapter 7-4 · A non-magmatic component in fluids of South American Fe oxide-Cu-Au deposits inferred from δ37Cl, 87Sr/86Sri and Cl/Br Cl/Br-δ37Cl space that may result from mixing of the mantle-derived magmatic-hydrothermal fluid with a crustal brine characterized by Cl/Br ratios significantly lower than evaporites but higher than seawater (Figure 2). The fact that all these IOCG deposits plot along a common mixing line (despite the large compositional field of crustal brines) is intriguing and appears to indicate that the mantle-derived magmatic fluid has interacted with a crustal brine characterized by virtually identical Cl/Br ratios despite the different ages and geographic locations of the deposits. The presence of a non-magmatic fluid component in these IOCG deposits is again supported by strontium isotope compositions of the inclusion fluids, which are significantly more radiogenic ( 87Sr/ 86Sr i = 0.7053-0.7056 at Candelaria and 0.7051-0.7062 at RaulCondestable) than those of the associated magmatic rocks (87Sr/86Sri = 0.7031 at Candelaria and 0.7042 at RaulCondestable). In addition, at Candelaria-Punta del Cobre chalcopyrite, secondary biotite, ore-related calcite and anhydrite also have 87Sr/86Sri (0.7043-0.7063) higher than the magmatic rocks (R. Marschik, unpublished data). Calculated chlorine contributions from the crustal brine range between 50 and 95% assuming δ 37 Cl mantle = 4.7‰ (Magenheim et al., 1995) and a δ37Clbrine = -0.4‰. However, due to the ten- to hundred-fold higher chlorine content of crustal brines compared to (non-boiled) magmatic fluids, these figures correspond to 4 and 30 wt.% crustal brine contribution. The above calculations are highly sensitive to assumptions about Cl and Br concentrations in brines and magmatic fluids, to the poorly constrained δ37Cl composition of the mantle-derived magmatic fluid and crustal brines, and to the relatively large analytical uncertainty of δ37Cl values (±0.2‰), yet they clearly indicate the presence of a measurable non-magmatic, crustal Cl (and Sr) component in fluids of IOCG deposits. 4 Conclusions Chlorine and strontium isotope data combined with Cl/ Br ratios indicate that ore fluids in the investigated IOCG and magnetite-apatite deposits result from variable mixing of mantle-derived magmatic-hydrothermal fluids with crustal brines or evaporites. The Gameleira IOCG deposit and the El Romeral magnetite-apatite deposit formed by magmatic-hydrothermal fluids leaching evaporites from the host sequence or by mixing with crustal brines characterized by high Cl/BR ratios. Fluids of these deposits preserve a pristine magmatic O and S isotope signatures, yet minimal interactions with evaporites (e.g., 2-9 wt.%) are sufficient to produce the observed evaporite-type Cl and Sr isotope signatures as well as Cl/Br ratios. In contrast, the IOCG deposits of Candelaria, RaulCondestable and Sossego formed by the mixing of magmatic-hydrothermal fluids with up to a few tens percent 737 of crustal brine (4-30 wt.%). The significant contribution of crustal brines in these deposits is suggested by Cl and Sr isotope data as well as by Cl/Br ratios. The results are consistent with mixed magmatic and non-magmatic hydrothermal fluid signatures inferred from other isotope systems (oxygen, sulfur). Chlorine isotope data combined with Cl/Br ratios and strontium isotope compositions suggest a measurable contribution of crustal brines and/ or evaporites to the ore fluids in IOCG and magnetiteapatite deposits of South America. This conclusion may help to refine strategies for IOCG deposit exploration in South America. Acknowledgements We thank Rolf Romer (GFZ, Potsdam) and Holly Stein, Aaron Zimmerman, and Parham Gardner (AIRIE Program, Colorado State University, U.S.A.) for their comments that helped to improve an earlier version of the manuscript. References Banks DA, Green R, Cliff RA, Yardley BWD (2000) Chlorine isotopes in fluid inclusions: determination of the origins of salinity in magmatic fluids. Geochim Cosmochim Acta 64: 1785-1789 Barton MD, Johnson DA (1996) Evaporitic-source model for igneousrelated Fe oxide-(REE-Cu-Au-U) mineralization. Geology 24:259-262 Dardenne MA, Ferreira Filho CF, Meirelles MR (1988) The role of shoshonitic and calc-alkaline suites in the tectonic evolution of the Carajás district, Brazil. J South Amer Earth Sci 1: 363-372 de Haller A, Zúñiga Alvarado J, Corfu F, Fontboté L (2002) The iron oxide-Cu-Au deposit of Raul-Condestable, Mala, Lima, Peru. In: Sociedad Geologica del Peru (ed) Conf Abst Vol XI Congr Peruano Geol, Lima: p. 80 Eastoe CJ, Long A, Land LS, Kyle JR (2001) Stable chlorine isotopes in halite and brine from the Gulf Coast Basin: brine genesis and evolution. Chem Geol 176: 343-360 Eggenkamp HGM, Kreulen R, van Groos FK (1995) Chlorine stable isotope fractionation in evaporites Geochim Cosmochim Acta 59: 5169-5175 Hitzman MW (2000) Iron oxide-Cu-Au deposits: what, where, when, and why? In: Porter TM (ed) Hydrothermal iron oxide-coppergold and related deposits: a global perspective, vol 1. PGC Publishing, Adelaide, Australia, p 9-25 Hitzman MW, Oreskes N, Einaudi MT (1992) Geological characteristics and tectonic setting of Proterozoic iron oxide (Cu-U-AuREE) deposits. Precamb Res 58: 241-287 Johnson LH, Burgess R, Turner G, Milledge HJ, Harris JW (2000) Noble gas and halogen geochemistry of mantle fluids: comparison of African and Canadian diamonds. Geochim Cosmochim Acta 64: 717-732 Lindenmayer ZG, Pimentel MM, Ronchi LH, Althoff FJ, Laux JH, Araújo JC, Fleck A, Bortowski DC, Nowatzki AC (2001) Geologia do depósito de Cu-Au do Gameleira, Serra dos Carajás, Pará. In: Jost H, Brod JA, Queiroz ET (eds) Caracterização de depósitos auriferous brasileiros. ADIMB-DNPM, Brasília, p. 79-139 Machado N, Lindenmayer Z, Krogh TE, Lindenmayer D (1991) U-Pb geochronology of Archean magmatism and basement reactivation in the Carajás area, Amazon shield, Brazil. Precambrian Res 49: 239-354 Close 738 M. Chiaradia · D. Banks · R. Cliff · R. Marschik · A. de Haller Magenheim AJ, Spivack AJ, Michael PJ, Gieskes JM (1995) Chlorine stable isotope composition of the oceanic crust: implications for Earth’s distribution of chlorine. Earth Planet Sci Lett 131: 427-432 Marschik R, Fontboté L (2001) The Candelaria-Punta del Cobre iron oxide Cu-Au(-Zn-Ag) deposits, Chile. Econ Geol 96: 1799-1826 Marschik R, Spangenberg JE, Leveille RA, de Almeida AJ (2003) The Sossego iron oxide-Cu-Au deposit, Carajás, Brazil. In: Eliopoulos D et al (eds) Mineral Exploration and Sustainable Development v 1. Millpress, Rotterdam, p. 331-334 Olszewski WJ, Wirth KR, Gibbs AK, Gaudette HE (1989) The age, origin and tectonics of the Grão-Pará Group and associated rocks, Serra dos Carajás, Brazil. Precambrian Res 42: 229-254 Pollard PJ (2002) Evidence of a magmatic fluid and metal source for Fe-oxide Cu-Au mineralisation. In: Porter TM (ed) Hydrothermal iron oxide copper-gold and related deposits – A global perspective v 1. PGC Publishing, Linden Park, Australia: 27-41 Sillitoe RH (2003) Iron oxide-copper-gold deposits: An Andean View. Mineral Deposita 38: 787-812 Close Chapter 7-5 7-5 Origin of hydrothermal ore-forming processes in the Dapingzhang polymetallic copper deposit in the Lanping- Simao Basin, Yunnan Province Dai Baozhang, Jiang Shaoyong State Key Laboratory for Mineral Deposits Research, Department of Earth Sciences, Nanjing University, Nanjing, 210093, China Liao Qilin Jiangsu Geological Survey Institute, Nanjing, 210018, China Abstract. The newly discovered Dapingzhang polymetallic copper deposit in the Lanping-Simao Basin is hosted in volcanic rocks. The orebodies include an upper stratiform and lentiform massive sulfide orebody, and a lower vein type and disseminated sulfide orebody. The Rb-Sr isotopes of quartz fluid-inclusions in the vein type orebody yield an isochron age of 118 ±12 Ma. Fluid-inclusion analysis shows that the ore-forming fluid is of low to middle salinity (2.0-8.0 wt%NaCl), and of low to middle temperature (90~200oC). The δ34S values of pyrite and chalcopyrite minerals in this deposit concentrate at about 0‰. Our modeling and water/rock ratio calculations using available hydrogen-oxygen isotope data suggests an evolved meteoric water origin for the ore-forming fluids, instead of mixture of seawater and magmatic fluids. The Pb isotope composition indicates radiogenic Pb sources, and suggests Pb from sedimentary rocks and mantle-derived volcanic rocks in the basin both contribute to this deposit. In conclusion, the Dapingzhang deposit shares many similar geochemical characteristics with vein type copper deposits in the Lanping-Simao Basin. These data support the conclusion that the Dapingzhang polymetallic copper deposit is a hydrothermal deposit formed during Yanshanian period, not a massive sulfide deposit of submarine-exhalative-sedimentary origin as proposed by previous researchers. Keywords. Isotope geochemistry, quartz fluid inclusion, Rb-Sr isochron age, Yanshanian period, hydrothermal deposit 1 Introduction 2 Rb-Sr isochron age Determining the age of mineralization is essential for understanding any deposit. In this study, mineralization was dated using Rb-Sr analysis of fluid inclusions. The Rb-Sr isotopic compositions of fluid inclusions in 8 selected quartz samples were analyzed. The data were then plotted using the ISOPLOT program with λ ( 87 Rb) 1.42x1011/a. The input error was 87Rb/86Sr = 0.5%. The 6 samples from the vein type and disseminated sulfide orebody yield an isochron age of 118 ±12Ma, MSWD = 0.46. Previous isotope dating (Zhong et al. 2000) shows that the age of the host rock is 500~530 Ma. The ages of a variety of intrusions in this area are between 300 Ma and 150 Ma, which indicate that the Dapingzhang deposit formed after these local intrusions. Two samples from the massive orebody evidently depart from the isochron and show higher 87Sr/86Sr values (Fig. 1). This could be caused by increased contribution from materials with higher 87Sr/86Sr values (e.g., sediments in the basin). This could be because the massive orebody is relatively shallower than the vein type deposits. The limited sample number in this case (2) prevents the possibility of obtaining an age for the massive orebody. Some The Dapingzhang polymetallic copper deposit is an important recent discovery in Lanping-Simao Basin. It is composed of an upper stratiform and lentiform massive sulfide orebody, and a lower vein type and dissiminated sulfide orebody. Previous researchers have identified it as a massive sulfide deposit with submarine- exhalativesedimentary origin (Li 2000; Li et al. 2000; Li and Zhuang 2000; Li and Zhang 2001; Zhong et al. 2000). In this paper, new results of fluid inclusion, sulfur isotope and mineralization age are taken into account. The data lead to a different perspective on ore-forming process, which is also consistent with previous data. The Dapingzahng deposit was formed by extensive interaction between meteoric water (or brine) and host rocks. This is similar to the oreforming process identified in the vein type deposits in Lanping-Simao Basin. Close 740 Dai Baozhang · Jiang Shaoyong · Liao Qilin direct dating methods such as Re-Os isotope analysis of metal sulfides (Jiang et al., 2000) should be adopted in further research. The reliable age of 120 Ma for the vein type and disseminated sulfide orebody indicates that this deposit mainly formed in Yanshanian period. concentrate at about 0‰, implying that sulfur in this deposit is mainly mantle-derived. Sulfur with such characteristics can either come directly from volcano exhalative, or can be leached from volcanic rocks. For the Dapingzhang deposit, the latter is more reasonable. 3 4.2 Hydrogen-oxygen isotopes Fluid inclusions In this study, quartz and calcite minerals from variety of samples were carefully selected for fluid inclusion analysis in order to acquire information about the composition of ore-forming fluids. The results show that the range of homogeneous temperatures is 90~200 o C (mainly from130oC to 160oC), and the salinity of the ore-forming fluid varies from 2.0 to 8.0 wt%NaCl. These results are relatively lower in temperature and salinity than previous data; however this could be due to the fact that these samples originate from shallower depths than those from previous studies. As shown in Figure 2, the ore-forming fluid of Dapingzhang deposit is similar to that of the vein type deposit series in Lanping-Simao Basin composed by Jinman, Shuixie and Bailongchang. On the other hand, temperature of ore-forming fluids in massive sulfide deposits mainly ranges from 200oC to 350 o C, which is much higher than that of the Dapingzhang deposit. 4 To determine the origin and evolution of the ore-forming fluid, available hydrogen and oxygen isotope data (Li and Zhuang 2000; Zhong et al. 2000) are compiled (δ18OH2O values of -2.5 to +2.9‰, and δD values of –84 to –59‰ for the ore-forming fluids) and further analyzed. The calculation of water/rock interaction is taken in this study with the δD and δ18OH2O values of meteoric water are 120‰ and -16‰ (Liu et al., 2000) and the δD and δ18OH2O values of volcanic rocks are -65‰ and 8‰ (Shen 1997). Figure 4 shows that the available hydrogen and oxygen data are consistent with the two evolution curves at 150oC Isotope research 4.1 Sulfur isotopes Chalcopyrites and pyrites from variety of samples were selected in this study for sulfur isotope analysis. Both the results in this study and previous studies (Li et al. 2000; Zhong et al. 2000) indicate that δ34S values of all sulfides Close Chapter 7-5 · Origin of hydrothermal ore-forming processes in the Dapingzhang polymetallic copper deposit in the Lanping- Simao Basin, Yunnan Province 741 2. The ore-forming fluid is similar to that of the vein type deposit series, with low to middle salinity and low to middle temperature. Hydrogen-oxygen isotope data indicate an evolved meteoric water origin for the fluid. 3. Sulfur and lead isotope data imply that the host volcanic rocks are the main source for sulfur and oreforming metals. 4. It is most likely that mineralization of the Dapingzhang deposit is similar to that of the vein type deposit series in Lanping-Simao Basin. The Dapingzhang polymetallic copper deposit is a hydrothermal deposit. References and 250oC, respectively. Thus, it is most likely that the oreforming fluid is extensively evolved meteoric water. 4.3 Lead isotopes Available lead isotope data are plotted onto the Zartman Pb isotope diagram. Lead in this deposit is relatively rich in radiogenic Pb. Fig. 5 shows that host-rock samples lay on the orogen curve, while orebody samples lie between the orogen curve and the mantle curve, implying some contribution from a magmatic source. It is likely that host rocks supply most of the ore-forming metal to both the vein type deposit series and the Dapingzhang copper polymetallic deposit. 5 Conclusions Combining the new results in this study and the available data of previous researchers, we acquire some essential perspectives on the Dapingzhang copper polymetallic deposit: 1. The fluid-inclusion Rb-Sr isotopes of quartz in the vein-type orebody yield an isochron age of 118 ±12 Ma. This indicates that the orebody was formed in late Yanshanian period. Jiang S, Yang J, Zhao K (2000) Re-Os isotope tracer and dating methods in ore deposits research. Journal of Nanjing University (Natural Sciences) 36(6): 669~677 Li F (2000) Volcanic-exhalative-sedimentary ore- forming model of Dapingzhang Cu-polymetal deposit, western Yunnan. Bulletin of Mineralogy, Petrology and Geochemistry 19(4): 296~297 Li F, Zhang F (2001) Volcanic-exhalative- sedimentary genesis of Dapingzhang Cu-polymetal deposit, western Yunnan. Geology and Prospecting 37(4): 5~8 Li F, Zhuang F (2000) Fluid inclusion characteristics and its metallogenic significance of the Dapingzhang Cu-polymetal deposit in Simao, western Yunnan. Geotectonica et Metallogenia 24(3): 237~243 Li F, Zhuang F, Yang H (2000) Fluid inclusions analysis of Dapingzhang Cu-polymetal deposit, western Yunnan. Acta Petrologica Sinica 16(4): 581~586 Liu J-J, Li C-Y, Pan J-Y (2000) Isotopic Geochemistry of copper deposits in sandstone and shale of Lanping-Simao basin, western Yunnan. Mineral Deposits 19(3): 223~234 Ohmoto H, Skinner BJ (1983) The Kuroko and related volcaogenic massive sulfide deposit. Economic Geology (Monograph) (5): 604 Shen W (1997) Textbook on isotopic geology. Atomic energy publishing house, Beijing. Wu N (2003) Geochemistry of the vein-type copper deposits in Lanping-Simao Basin, Yunnan Province, China. Paper for master’s degree of Department of Earth Sciences, Nanjing University Wu N (2003) Lead and sulfur isotope geochemistry and the ore sources of the vein-type copper deposits in Lanping-Simao Basin, Yunnan Province. Acta Petrologica Sinica 19(4): 799~807 Zhong H, Hu R-Z, Ye Z-J (1999) Isotopic chronology of the spiliteceratophyre formation in Dapingzhang, Yunnan Province and its geologic significance. Science in China (D) 29(5): 407~412 Zhong H, Hu R-Z, Ye Z-J (2000) Sulfur, lead, hydrogen and oxygen isotopic geochemistry of the Dapingzhang copper- polymetallic deposit, Yunnan Province. Geochemica 29(2): 136~142 Close Close Chapter 7-6 7-6 Stable isotope geochemistry of the gold-sulfide mineralized zone of the Kottapalle block of the Ramagiri greenstone belt, Dharwar Craton, South India M. Deb, K. Bheemalingeswara Department of Geology, University of Delhi, Delhi 110007, India Abstract. The Neo-Archean Ramagiri-Penakacherla belt is located in the eastern Dharwar craton of South India. It hosts auriferous quartz bodies in altered mafic and felsic volcanic rocks, intimately interlayered and co-folded with carbon phyllites. The sequence is metamorphosed to low greenschist facies. Pervasive quartz-carbonate alteration is a conspicuous feature in the gold-sulfide mineralized zone of the Kottapalle block of this greenstone belt. The carbonate compositions spread along the dolomite-ankerite or calcite-ankerite join. The host volcanics are of tholeiitic basalt, andesitic and dacitic compositions representing a probable island-arc setting. The majority of carbonaceous samples fall in the range of – 20 and – 28 per mil δ13Corg (PDB), suggesting a biogenic derivation of the reduced carbon and a sedimentary origin of the strata. Carbonate δ13C (PDB) have median values of -2.4 per mil and mean of – 4.0 per mil. δ34S (CDT) values of pyrite and pyrrhotite cluster around +2 per mil. Primary fluid inclusions, rich in CO 2 with subordinate CH 4 , as observed in preliminary microthermometric studies, demonstrate the pervasive presence of a CO2-rich hydrothermal fluid responsible for the extensive carbonation of the auriferous host rocks. Absence of any sedimentary carbonate strata in the sequence, and the stable-isotope data support the role of mantle-derived fluids in producing the quartz-carbonate alteration. The δ13C values of carbonates indicate that the hydrothermal fluid did not have any significant interaction with the reduced carbon in the ore zone. The sulphur isotope data points to the mantle-source of sulphur in the ore-bearing hydrotherms. Keywords. Shear gold, quartz-carbonate alteration, Dharwar craton, stable-isotope geochemistry 1 Introduction The Ramagiri-Penakacherla belt is one of a series of auriferous greenstone belts in the eastern Dharwar craton of South India. This belt, considered to be of Neo-Archean age (2746+ 64 Ma; Zachariah et al. 1995) is located in the Anantapur district of Andhra Pradesh. The belt forms a Y-shaped outcrop of prominently mafic volcanic rocks, which are surrounded on all sides by the Peninsular Gneiss. The litho-units present in the area (Ghosh et al. 1970) are: – Dolerite dyke – Ultrabasic rocks – Pyroclastics – – – – – – – – Light and dark phyllites Greenstones with chert layers Quartz-chlorite schists Quartzite Banded Iron Formation Hornblende schist Metagabbro Granitic rocks, massive and banded The light grey phyllite consists essentially of carbonate and chlorite, with minor amounts of sericite and quartz. The dark grey phyllite on the other hand has chlorite as the dominant phase over carbonates. Auriferous quartz bodies of different types and generations occur in this part of the sequence (shown in italics above) in the form of reefs, pods and veinlets along the pervasive foliation. In the Kottapalle block of the Ramagiri ore zone (Fig. 1) the altered volcanics are intimately interlayered and cofolded with carbon phyllite. In the auriferous zone these rocks contain sulfide minerals such as, pyrite, chalcopyrite, pyrrhotite, sphalerite and minor arsenopyrite..The metamorphic mineral assemblage indicates that the grade of metamorphism has attained low green schist facies. Pervasive quartz-carbonate alteration is a conspicuous geological feature noted in the gold-sulfide mineralized zone in the Kottapalle block. It has affected both the felsic and mafic volcanic units of the greenstone belt. The carbonates co-exist as grains, bands and patches with the carbonaceous matter in the carbon phyllites. Thus, carbon, either as graphitic carbon or as carbonate is invariably associated with the Au-sulfide mineralization. This first stable isotope study in this belt was conducted to ascertain the source of carbon and sulfur in the ore-host rock association. This work would also provide useful insight into the oregenetic process and environment of ore emplacement. Towards this end, three bore holes drilled by the Geological Survey of India in the Kottapalle block (cf. Fig. 1) were logged and sampled systematically and subjected to XRD, XRF, CHNS (elemental), EPMA analyses and stable isotope mass spectrometry. Close 744 M. Deb · K. Bheemalingeswara 2 Results 2.1 Petrology and geochemistry Based on discriminant diagrams, using their major and trace element abundances, the mafic and felsic volcanics in the host sequences were found to be of tholeiitic basalt, andesite and dacite compositions. In tectonic discriminant diagrams, the Kottapalle metabasalts plot in the IAB field, suggesting the possibility of subductionrelated volcanism in an island arc setting in the Archean Dharwar craton (cf. Zachariah et al. 1997). The volcanic rocks have been so severely altered and metamorphosed that the two main protoliths, tholeiitic basalt and dacite, can hardly be distinguished petrographically. Both the volcanics have turned into fine grained chlorite-sericite schists, the only distinction being the fine grained quartzofeldspathic matrix in the felsic compositions. These schists have been described as light and dark phyllites in field parlance. Carbonate grains in three samples of metabasalt and felsic volcanics were investigated through XRD, CL and EPMA (JEOL JXA 8600 superprobe) analyses. All carbonate grains analysed contain manganese as a minor component, with MnO content ranging from nil to 0.9 wt.%. Their compositional characteristics, in terms of the three major components, CaO, MgO and FeO, are presented in Figure 2. Coarse quartz-carbonate veins and lenses occur in contact with finely schistose carbonaceous and carbonate interlayerings in sericite-quartz schists (RG49/11). Compositions of carbonates in them showed the predominance of ankerite over dolomite molecule along the dolomite-ankerite join. Coarse brownish carbonates in lenses and bands in another section (RG47/1) within sericitechlorite-quartz schist showed a trend of increasing dolomitic and calcitic molecules. This section showed excellent microstructural relationships, with the schistosity transected by tightly folded late quartz veinlets. In yet another section (RG47/18) brownish pre- to syntectonic carbonate-quartz-sulfide lenses show compositions along the calcite-ankerite join. In this section, two types of carbonates are observed. The late carbonates, identified under CL, are clearly more calcitic. They are located along the grain boundaries of earlier carbonate grains. Fe-rich carbonates, as noted in this study, are typically related to gold mineralization in greenstone belts the world over. Total carbon content of 48 analyzed samples from the ore zone rocks ranged from 7.3 to 0.27 wt.%, with a mean of 3.11 wt.% (std. dev. 1sigma = 1.67%). Corg content mea- Close Chapter 7-6 · Stable isotope geochemistry of the gold-sulfide mineralized zone of the Kottapalle block of the Ramagiri greenstone belt, Dharwar craton 745 δ18O (SMOW) per mil of 21 carbonates from Kottapalle ore zone (Fig. 4) show spread of δ13C values from 0 to 9.2 per mil with a mean of – 4.0 and a median of – 2.4 per mil. δ18O values range from 26.0 to 12.5 per mil. One pure calcite from a late veinlet had an unusual composition of -9.2 per mil δ13C and -11.2 δ18O. While only one sample showed sea water-derived carbonate δ13C value near zero, the majority clustered between – 1.5 and – 2.7 per mil. A few values were spread between – 3.9 and - 6.2 per mil while 2 samples gave values around – 9 per mil. Limited sulfur isotope analyses of 8 monomineralic pyrite and 1 pyrrhotite separates gave a range of δ34S (CDT) between +2.8 and -1.7 per mil, with the majority clustering around +2 per mil (Fig. 5). 3 sured in 15 samples ranged from 5.8 wt.% to nil, while Ccarb, estimated as the difference between Ctotal and Corg in 15 samples, ranged between 5.9 wt.% to nil. 2.2 Stable isotope composition Twenty one analyses of δ13Corg in three carbonaceous samples (Fig. 3) ranged between – 14.2 and – 32.4 per mil (PDB), with the majority of samples falling in the range of – 20 and – 28 per mil. These values suggest a biogenic source for the carbon, and thus, a sedimentary origin for the carbonaceous strata. Values heavier than – 20 per mil probably reflect partial equilibration with co-existing carbonates or thermal maturation to heavier values by liberation of CH4. δ13CCarb-graphite of 11.6 and 13.8 per mil in co-existing carbonate and reduced carbon suggest an equilibration temperature of about 300 to 225oC (cf. Oberthür et al. 1996). A plot of δ13C (PDB) per mil against Discussion and conclusion For shear- or fault-controlled Archean epigenetic goldquartz deposits, controversy prevails regarding the source of the ore components and fluids. There are two end-member genetic hypotheses - one metamorphic and the other magmatic - which continue to compete. Since most deposits of this type show pervasive carbonate alteration and sulfide association, determination of the source of carbon and sulfur in the ore zone can lend significant support to either of the two hypotheses. Extensive quartz-carbonate alteration of the host volcanics, absence of any sedimentary carbonate strata in the sequence and presence of primary fluid inclusions rich in CO2 with subordinate CH4, as observed in preliminary microthermometric studies, demonstrate the pervasive presence of a CO2-rich hydrothermal fluid. This type of fluid is necessary for carbonation of the auriferous host rocks in the Kottapalle block of the Ramagiri greenstone belt. The variation in the composition of the carbonates, noted above, may be attributed to episodic fluctuations in the temperature and composition of the fluids in the structural conduits (cf. Mumin et al. 1996). The median δ13C of -2.4 per mil composition of the carbonates is too negative to have been derived from metamorphically remobilized CO2 from sea water-derived carbonate. This median value of ore zone carbonates and their spread upto -6.2 per mil conforms closely to the range Close 746 M. Deb · K. Bheemalingeswara of -2.0 to -6.0 recorded by Groves et al. (1988) for faultcontrolled regional carbonation involving CO2 of magmatic or mantle origin. The median value is also close to the -3.1 ± 1.3 per mil δ13C value of undoubted magmatically-derived carbonates found in association with molybdenite mineralization in a granodiorite intrusion in Canada (Burrows et al. 1986). Direct involvement of mantle fluids in the ore-bearing hydrotherm is envisaged instead of reworking of mantle-derived carbonates into metamorphic fluids, as an alternative process of ore formation. This is supported by the limited variation in the δ13C values of carbonates and the near-zero (+2 per mil) mantle signature in the associated sulfides. Absence of strongly negative (> -10 per mil) δ13C values in the carbonates also imply that the hydrothermal fluid did not have any significant interaction with reduced carbon. Acknowledgements This study was made possible by the kind permission granted by the Deputy Director General (Southern Region), Geological Survey of India for the logging and collection of bore hole samples. The help received in the field from senior geologist, K.N.Reddy is gratefully acknowledged. The EPMA, CL, XRD and Mass spectrometry were carried out during a revisit of the first author (MD) to the Geochemisches Institut, Göttingen, Germany with an Alexander von Humboldt Foundation fellowship. He is grateful to Prof. J.Hoefs for extending all laboratory fa- cilities at Göttingen. Thanks are also due to Dr. Andreas Hoppe, Director, Landesamt fur Bodenforschung, Wiesbaden, for help in generating the XRF data. This study was supported by a research grant (ESS/CA/A5-11/95) from the Department of Science & Technology, Govt. of India, to the first author. References Burrows DR, Wood PC, Spooner ETC (1986) Carbon isotope evidence for a magmatic origin for Archean gold-quartz vein ore deposits. Nature 321 851-854 Ghosh DB, Sastry BBK, Rao AJ, Rahim AA (1970) Ore environment and ore genesis in Ramagiri Gold Field, Andhra Pradesh, India. Econ. Geol. 65 801-814 Groves DI, Golding SD, Rock NMS, Barley ME, McNaughton NJ (1988) Archean carbon reservoirs and their relevance to the fluid source for gold deposits. Nature 331: 254-257 Mumin AH, Fleet ME, Longstaffe FJ (1996) Evolution of hydrothermal fluids in the Ashanti gold belt, Ghana: stable isotope geochemistry of carbonates, graphite and quartz. Econ. Geol. 91: 135-148 Oberthür T, Schmidt Mumm A, Vetter U, Simon K, Amanor, JA (1996) Gold mineralization in the Ashanti belt of Ghana: genetic constraints of the stable isotope geochemistry. Econ. Geol. 91: 289-301 Zachariah JK, Hanson GN, Rajamani V (1995) Postcrystallisation disturbance in the neodymium and lead isotope systems of metabasalts from the Ramagiri schist belt, southern India. Geochimica et Cosmochimica Acta 59: 3189-3203 Zachariah JK, Rajamani V, Hanson, GN (1997) Petrogenesis and source characteristics of metatholeiites from the Archean Ramagiri schist belt, eastern part of Dharwar craton, India. Contrib. Mineral. Petrol. 129: pp. 87-104 Close Chapter 7-7 7-7 Isotope systematics of ore-bearing granites and host rocks of the Orlovka-Spokoinoe mining district, eastern Transbaikalia, Russia A. Dolgopolova, R. Seltmann, C. Stanley Natural History Museum, Dept. Mineralogy, CERCAMS, Cromwell Road, London SW7 5BD, UK D. Weiss Imperial College, London, Prince Consort Road, London SW7 2BP, UK B. Kober Institute of Environmental Geochemistry, Im Neuenheimer Feld 234, D-69120 Heidelberg, Germany W. Siebel Dept. of Earth Sciences, Eberhard-Karls-University, Wilhelmstr. 56, D-72074 Tübingen, Germany Abstract. Pb, Rb and Sr isotope data are reported for the Khangilay, Orlovka and Spokoinoe granite massifs and their host rocks in the Orlovka-Spokoinoe mining district, Eastern Transbaikalia, Russia. Pb isotope analyses indicate a common Pb source for all three granite massifs reflecting a homogenous source melt from which all magmatic members evolved. Pb isotope systematics identify two possible scenarios for the source of Li-F granites: 1) a crust-mantle source where a mixture of MORB and continental-derived material were brought together in an orogenic environment; and 2) a type II enriched mantle source where subducted continental material could have been strongly implicated in volcanic suites. New Rb-Sr isotope age data yield a 143.8±4.2 Ma age for barren granites of the Orlovka and Khangilay massifs. mantle interaction in the development of granitoid magmatism, the genetic relationship between the three massifs and similarities and differences among them may be identified. Rb-Sr isotopes provide additional insights into the age of granites from the Orlovka-Spokoinoe mining site. Keywords. Pb Rb Sr isotope systematics, ore-bearing granite, Eastern Transbaikalia 1 Introduction The rare-metal granite-related Orlovka tantalum deposit and the Spokoinoe tungsten vein quartz-greisen deposit are located in Eastern Transbaikalia 140 km and 148 km SE of Chita, respectively. Both deposits are hosted by the Khangilay granite pluton and are believed to be its satellites (Fig. 1) (Badanina et al. 2004; Beskin et al. 1994; Kovalenko et al. 1999; Syritso et al. 2001). In recent years, the evolution of rare-metal granites, their formational stages, and their relation to intraplate magmatism have been studied. Specifically, Rb-Sr and Sm-Nd isotopic systems were used to reveal the source(s) of rare-metal granite melts from the study area, and the results indicate that sources were likely to be either crustal, mantle or combined crustal-mantle (Kostitsyn 2001; Kovalenko et al. 1999, 2002, 2003; Yarmolyuk et al. 2001, 2003). Our study uses Pb isotopes for the granites of the Orlovka, Spokoinoe, and Khangilay massifs and their host rocks with the goal to study the evolutionary trends and features of the Khangilay pluton and the Orlovka and Spokoinoe deposits (barren versus mineralized granites, ores, host rocks). By examining fluid-rock and crust- Close 748 A. Dolgopolova · R. Seltmann · C. Stanley · D. Weiss · B. Kober · W. Siebel 2 Geological setting The Orlovka-Spokoinoe mining district belongs to the Central Asian Orogenic Belt (CAOB) (Jahn et al. 2000) or Transbaikal-Mongolian orogenic collage where multiple oroclinally bent magmatic arcs separated by accretionary complexes and ophiolitic sutures are located between the major cratons. Rare-metal Li-F enriched granites and pegmatites are widespread as products of continental crustal growth and associated intraplate magmatism. The Khangilay pluton is located in the central portion of the Paleozoic Aginskaya microplate, which is made up of predominantly sandstone and shales (Beskin et al. 1994; Syritso et al. 2001). The granitoids of the pluton cut Proterozoic to Carboniferous shales and volcanics, a Triassic terrigenous and volcano-sedimentary sequence, and gabbro-diorite, granodiorite, and lamprophyre bodies (Kovalenko et al. 1999). The microplate was intruded by granite plutons, the largest of which is 24 km by 22 km in dimension at a depth of 500-2500 m based on gravimetric data. It is exposed at the surface as three separate granitic (Khangilay, Spokoinoe and Orlovka) massifs. The Khangilay granite massif is composed of biotite granite and biotite-muscovite granites. The Orlovka satellite is a highly differentiated Ta-(Nb-Sn-) bearing intrusion of lithionite-amazonite-albite granite. The Spokoinoe body is a muscovite-albite granite with W (Sn, Be) mineralization. To assess magma–host-rock interactions of the Khangilay-Orlovka intrusions within the regional geochemical framework, greisenized Spokoinoe granites and a representative suite of host rocks (volcanics, hornfelses, metasediments, gabbro-diorite) were included in the study. 3 Results and discussion The mixing diagram (Fig. 2) shows a strong relationship between the barren parental granites of the Khangilay pluton and the ore-bearing granites of the Orlovka and Spokoinoe massifs. They all plot within a single linear array. Despite a wide range of Pb isotope compositions within each granite body, they do not differ significantly among all three granite massifs (Dolgopolova et al. 2004). It hints at fractionation from a homogenous (or homogenized) source melt with uniform initial 206Pb/204Pb and 207Pb/204Pb ratios. The overall data trend demonstrates a simple mixing of the uniform Pb composition with different radiogenic components in the rocks and a strong relation of the barren parental rocks to the ore-bearing rocks. Lead isotope signatures of the host rocks are more scattered than those of the granite rocks and are off the granite’s mixing line. The Orlovka ore-bearing amazonite granites, with the highest Pb concentration, were used to identify the initial Pb isotopic signature subsequently transferred to the ore-bearing rocks. The high Pb concentrations, up to 190 ppm, found in ore-bearing amazonite granites minimize the effects of fluid-wall rock interaction and associated perturbation to Pb systematics. The amazonite granites are characterized by the lowest rate of radiogenic Pb accumulation because of their very low 238U/204Pb (µaverage = 1.3). The calculated initial values for these “least sensitive” ore-bearing granites are very similar and their averages are: 206Pb/204Pb = 18.41 ± 0.02; 207Pb/204Pb = 15.56 ± 0.006; and 208Pb/204Pb = 38.3 ± 0.03 (Dolgopolova et al. 2004). Pb isotope compositions were also determined in two separate grains of K-feldspar from the ore-bearing amazonite granite of the Orlovka Ta-Nb deposit. Pb isotope analyses and U-Pb isotope dilution measurements were carried out for blue-green cores and white feldspar rims. Differences between core and rim Pb isotopic compositions are negligible within the limits of statistical significance. The averages of measured initial Pb isotope compositions of feldspars are shown in Table 1. The average values of initial Pb isotope composition of ore-bearing granites were calculated previously to assess sources of the granitic magmas and were in the range of: 206Pb/204Pb = 18.49 ± 0.05; 207Pb/204Pb = 15.57 ± 0.01 and 208Pb/204Pb = 38.23 ± 0.06 (Dolgopolova et al. 2004). Our new data on Pb isotope compositions of K-feldspar (Table 1) show very good agreement with the calculated Close Chapter 7-7 · Isotope systematics of ore-bearing granites and host rocks of the Orlovka-Spokoinoe mining district, eastern Transbaikalia, Russia 749 0.0012 (Fig. 4). The data for barren biotite-muscovite granites are in excellent agreement with published data of the Orlovka-Spokoinoe granites, where the determined age of granites was 142.9 ± 1.8 Ma at initial 87Sr/86Sr of 0.706 ± 5 (Kovalenko et al. 1999). 5 initial Pb isotopic composition of the Orlovka granite pluton. Pb isotope systematics show the presence of a mantle signature transferred during the formation of the studied granites (Figure 3). A mantle-derived component is in a transitional field between mid-ocean ridge basalt (MORB) and type II enriched mantle (EM II) (Zartman and Doe 1981) but closer to the latter. There is a mixture of different epochs presented on Figure 3. The mantle arrays indicate present-day mantle Pb isotopes while granite data reflects “frozen” Jurassic Pb isotope compositions. If the mantle arrays are traced back to a Jurassic age with less radiogenic EM II and MORB sources than the plotted arrays, they would slightly shift to the lower left part of the plot and indicate EM II input. Therefore, Pb isotopic data suggest two possible sources contributed to the formation of the studied granites: 1) a crust-mantle source where a mixture of MORB and upper crustal-derived material were brought together in an orogenic environment; and 2) type II enriched mantle source where subducted continental material could have been strongly implicated in several island-arc volcanic suites and the corresponding isotopic signatures, thus reflecting a strong similarity of EM II with upper continental crust or continentally derived sediment. 4 New Rb-Sr age data Seven samples of barren and ore-bearing granites of Khangilay and Orlovka massifs were analyzed for Rb and Sr isotope compositions. Analyses of four samples from the barren granites yield a whole rock isochron age of 143.8 ± 4.2 Ma with an initial 87Sr/86Sr ratio of 0.7065 ± Regional evidence for the proposed model Evidence from Sr, Nd and O isotope investigations (Kovalenko et al. 1999, 2002, 2003; Yarmolyuk et al. 2003) is consistent with our lead isotope data reaffirming the two possible common sources for granitic magmas of the Orlovka-Spokoinoe mining district. However, there is no unequivocal data implicating either a mixed upper crustmantle source or a type II enriched mantle source. Regional studies of Transbaikalian granitoids incorporating geochemical, geophysical and geodynamic data indicate both crustal and mantle inputs triggering granitic melt generation of all petrochemical series (Jahn et al. 2000; Kovalenko et al. 1996; Litvinovsky et al. 2002). The isotopic heterogeneity of these granites was predetermined by the isotopic heterogeneity of their sources (Kovalenko et al. 1996). Blocks of consolidated preRiphean crust were overthrust during the accretionary collision of the foldbelts onto the younger crustal complexes of within-block oceanic basins contributing to an anomalous crustal thickness. The Riphean-aged crust in Caledonian structures most likely reflects the same average composition of a mixed source (basites + pelites) of the granitoid magmas; the source formed at 450-500 Ma. The isotopic evolution of this source resulted in εNd(T) ~ 0 of the mixed source by 100-200 Ma. Some of the young (~120 Ma) granites show evidence of assimilation of preRiphean crust (Kovalenko et al. 1996). Some metaluminous and peralkaline syenite-granite suites and closely associated comendites of Transbaikalia constrain A-type granitoid magma generation emplaced at ca. 280 Ma as a result of fractional crystallization of syenite magmas. Alkali-rich silicic magma formed at an estimated depth of 50-60 km far exceeding the normal crust thickness. The Sr-Nd isotope data advocate the main role of mantle-de- Close 750 A. Dolgopolova · R. Seltmann · C. Stanley · D. Weiss · B. Kober · W. Siebel rived material in the source region from which the alkali-rich syenitic and granitic magmas were produced (Litvinovsky et al. 2002). Also, widespread Transbaikalian alkali monzodiorite-syenite series are explained by fractional crystallization from tephritic magma intrusions at ca. 130 Ma. In contrast to calc-alkaline granite batholiths generated during continental crustal growths, subalkaline granites of Transbaikalia are often accompanied by basalt-trachyte-pantellerite-alkaline granite associations marking rift structures of intraplate “hotspots” (Kovalenko et al. 1996). The related Li-F and alkaline granites represent A-type granites with high heat production. Sr, Nd and O isotope investigations of late Oligocene–Holocene volcanics from the adjacent area of the Southern Baikal region (Yarmolyuk et al., 2003) show that the isotopic signature of the magma source is a mixture of moderately depleted mantle and enriched mantle reservoirs of types I and II enriched mantle (EM I and EM II). EM II source has been reported to be one of the mantle sources contributing to the formation of Early Mesozoic rocks of the Mongolia-Transbaikalia magmatic area and has been listed among mantle sources for the CAOB as a whole (Kovalenko et al. 2002). The published data on Sr and Nd isotopes for the Orlovka massif with the values of initial 87Sr/86Sr of 0.706 ± 0.005 and εNd = 0.1 (Kovalenko et al. 1999) also favor EM II mantle input. Data hints at the possibility that an EM II source controlled intraplate activity in Eastern Transbaikalia during late Mesozoic times including formation of the Orlovka and Spokoinoe deposits. 6 Conclusions Pb isotope data of crustal rocks and ore deposits of the Orlovka-Spokoinoe mining district complement the existing Nd and Rb-Sr data for this region. Our results indicate that the three granite massifs have uniform Pb isotope compositions and show a strong genetic relationship between the barren biotite-muscovite granites of Khangilay and the Spokoinoe and Orlovka ore-bearing granites suggesting a common source for the three massifs. Pb isotope data also confirm that the Khangilay pluton can be considered as the parental intrusion for its hosted mineralized apical intrusions. Pb isotope systematics outline two possible scenarios for the source of granitic melts: a mixed upper crust-mantle source, and a type II enriched mantle source. New Rb-Sr isotope data confirms the age of 143.8±4.2 Ma for biotite and biotite-muscovite granites of the Khangilay and Orlovka massifs. Acknowledgements The authors would like to thank Russian colleagues who participated in the INTAS 97-0721 project for inspiring discussions, assistance in field sampling and analytical support. Continuous assistance of the EMMA laboratory at the Natural History Museum London and of Barry Coles (Imperial College London) with the analytical part of the project is acknowledged. This is a contribution to the IGCP Project #473 “GIS Metallogeny of Central Asia”. Close Chapter 7-8 7-8 Syn-metamorphic dates for tourmaline formation around Mount Isa, north-west Queensland, Australia Robert J. Duncan, Andy R. Wilde pmd*CRC, School of Geoscience, Monash University, Melbourne, VIC 3800, Australia Roland Mass, Katherine Bassano pmd*CRC, School of Earth Sciences, Melbourne University, Melbourne, VIC 3010, Australia Abstract. Pb stepwise leaching of tourmaline from the Palaeoproterozoic Western Fold Belt of the Mount Isa Inlier yield dates of 1559±17 Ma, 1577±52 Ma and 1480±90 Ma. Structural, petrological and textural data suggest that 1559±17 Ma is the best estimate for peak metamorphism in the area. Estimates of Pb closure temperature and comparison with peak metamorphic temperatures indicate that this age represents tourmaline crystallisation. These dates represent syn-metamorphic fluid flow and indicate metal mobility during the Isan Orogeny. A result of this event is regional-scale silicification that has the same relative timing as extensive silica deposition in the rocks that now host the Cu orebodies at Mount Isa. Keywords. Mount Isa, metamorphism, tourmaline, hydrothermal fluid flow, Pb stepwise leaching 1 Introduction To further constrain the timing of the Isan Orogeny in the Western Fold Belt of the Mount Isa Inlier we applied the Pb step-leaching (PbSL) technique to tourmaline. PbSL involves sequential acid leaching of low-U minerals to generate Pb-Pb isochrons for old (>400 Ma) rocks (Frei and Kamber 1995). The tourmaline samples dated here can be demonstrated to have formed under, or close to, peak metamorphic conditions using structural, petrographical and geochemical evidence. As tourmaline is generally considered metasomatic in origin, this work not only allows an improved understanding of the timing of peak metamorphism, but also new insights into the nature of fluid flow associated with compressional deformation. The timing and nature of this hydrothermal event has potential implications for the Cu mineralisation at Mount Isa. 2 Previous work The polydeformed mid- to late Proterozoic Mount Isa Inlier in north-west Queensland was tectonically active between 1900 and 1500 Ma (Blake and Stewart 1992). The most intense period of deformation is considered to be largely synchronous with peak high temperature-low pressure metamorphism that resulted from crustal shortening during the Isan Orogeny from 1590 to 1500 Ma (Connors and Page 1995; O’Dea et al. 1997). Previous attempts to date peak metamorphism have focused on U-Pb analysis of zircon and monazite (Connors and Page 1995; Hand and Rubatto 2002), but their relationship to metamorphic reactions and structural features is ambiguous (e.g. Roberts and Finger 1997). Published Ar-Ar biotite dates (Perkins et al. 1999) are likely to represent cooling ages past the closure temperature. Table 1 summarises the current age estimates of peak metamorphism on single mineral phases. 3 Tourmaline occurrence, petrography and geochemistry Tourmaline-rich lithologies are abundant in areas around Mount Isa. Tourmaline is especially prevalent in the Eastern Creek Volcanics (ECV) west of the Mount Isa fault. In this area it occurs in quartz-K feldspar-mica-apatite pegmatites around the contact of the Sybella Batholith and apparently stratabound, but not stratiform, tourmalinites (representative of extensive silicification). Minor tourmaline occurrences have been identified in the ECV to the east of Mount Isa. The three samples selected for dating are from within a 25 km radius of Mount Isa and are in close proximity to small mineral occurrences (Fig. 1). Tourmaline has been identified as an accessory phase in the silica dolomite alteration halo to the Cu orebodies at Mount Isa (Mathias and Clark 1975). The silicification at the mine is considered to have occurred prior to Cu mineralisation, synchronous with D2 or D3 deformation (Swager 1985; Wilde et al. this volume) during the peak of deformation. The orebody tourmaline is dravitic in Close 752 Robert J. Duncan · Andy R. Wilde · Roland Mass · Katherine Bassano composition and is concentrated in the Paroo Fault in the footwall of the Cu orebodies (W. Perkins and J. Knights pers. comm. 2004). Tourmaline from close to the King Cu deposit is stratabound, but not stratiform within quartzite and psammopelitic units of the Myally subgroup. Tourmaline growth overprints the S2 fabric, defined by biotite and sillimanite, and is deformed by D3 NNW-trending shear zones and NNW gently plunging meso-scale folds (Fig. 2a). The sample consists of zoned glomerocrysts and coarsegrained strained quartz, along with minor amounts of titanite, sphalerite and Fe-Ti oxides. Adjacent to the Eldorado U deposit (hosted by the ECV) is a quartz-tourmaline-K feldspar-mica pegmatite. The pegmatite is parallel to the S2 fabric and is boudinaged by D3 structures. Tourmaline in the pegmatite selvages defines a steeply plunging mineral lineation (L2) and pseudomorphs cordierite poikiloblasts in the wall rock (Fig. 2b). Primary fluid inclusions within tourmaline from this sample contain up to 436 ppm U (Duncan and Wilde 2004). At Anderson’s Lode (a small U deposit hosted by the ECV) a quartz-fibrous tourmaline vein is deformed by D3 shearing. Host rock tourmaline is overprinted by a biotite-chlorite metamorphic matrix (Fig. 2c). These relationships suggest that tourmaline crystallisation was early to syn-metamorphic and pre-D3 in timing. Paragenetically associated with the quartz-tourmaline vein are minor amounts of pyrite and chalcopyrite. Electron-microprobe analyses demonstrate the transitional Fe-Mg composition of all the tourmaline samples. Tourmaline from Anderson’s Lode is schorlitic, whilst samples from Eldorado and King are dravitic. Trace element analysis by laser ablation ICP-MS reveals that the tourmalines are relatively enriched in light rare earth elements with variable Eu and Ce anomalies, indicative of crystallisation from a metamorphic fluid (cf. Jiang et al. 2004). 4 Pb stepwise leaching PbSL was carried out at the University of Melbourne. The main advantage of PbSL over bulk U-Pb dating is the ability to chemically separate Pb from U-rich and U-poor domains within the samples, thus generating Pb isotopic dispersion from a single mineral separate. 208Pb/206Pb systematics can be used to recognise, and discard if necessary, results from leach steps dominated by unequilibrated impurities with distinct Th/U ratios, such as zircon and monazite. Tourmaline concentrates (200 to 400 µm) were produced by conventional dense medium separation and purified by hand-picking. After removal of surficial Pb contamination with distilled water, samples weighing 80 to 100 mg were sequentially leached with 1.5 N HCl-2N HBr mix, 1N and 8N Close Chapter 7-8 · Syn-metamorphic dates for tourmaline formation around Mount Isa, north-west Queensland, Australia HBr, 7N and 15N HNO3 and 48% HF on a hot plate at ~100oC for periods of five minutes to 120 hours. Pb from each leach step was extracted using a single pass over 0.1 ml columns of EICHROMTM Sr resin following the method of Thériault and Davies (1999). Pb isotopic ratios were determined by multi-collector ICP-MS (Woodhead 2002). 753 Pb-Pb isochrons parameters and ages were calculated using ISOPLOT (Ludwig 2003). External 2sigma m (±0.03%) or internal (2sigmam) errors (whichever is greater) and error correlations derived from these uncertainties were used as input errors for the isochron calculations. No blank corrections were applied. Tourmaline from Anderson’s Lode yielded five leach steps, with a range in 206Pb/204Pb of 17.2 to 72.9. A regression of all five leach steps identifies some scatter (MSWD 77), but a relatively precise Pb-Pb isochron age of 1559±17 Ma (Fig. 3a). Seven leach steps derived from the tourmaline at Eldorado gave a range in 206Pb/204Pb from 19.9 to 67.2, regression of all the data indicates a excessive amount of scatter (MSWD >6000). Inspection of the 208Pb/206Pb data shows that three leach steps are affected by Pb from Thrich micro-inclusions. Omission of these points results in a four-point age of 1577±52 Ma (MSWD 46; Fig. 3b). The five leach spectra of the tourmaline from King yield the narrowest range in 206Pb/204Pb (16.4 to 35.3). After the removal of one step with anomalously high 208Pb/ 206 Pb (i.e., Pb derived from Th-rich inclusions), this short data array produce an imprecise age of 1488±90 Ma (MSWD 16; Fig. 3c). 5 Interpretation of ages Estimates of Pb closure temperatures in tourmaline for compositions similar to these samples were calculated according to the method outlined by Dahl (1997) and range from 580 oC to 630 oC. The Anderson’s Lode area is characterised by low to mid-greenschist facies rocks, so the 1557 Ma date reflects tourmaline formation. Around Eldorado peak metamorphic temperatures are estimated at 540oC to 640oC (Rubenach 1992) and at King temperatures of ~600oC are likely to have been encountered during peak metamorphism (Connors 1992). At these two locations the ages and associated large errors may represent a period of elevated heat flow, when the ambient geothermal gradient was above the Pb closure temperature and Pb could diffuse easily. The may explain the range of U-Pb zircon dates (Table 1; 1565 to 1480 Ma from one sample in Connors and Page (1995)). Comparing age data derived from Pb-Pb dating of tourmalines with other metamorphic dates it is clear that between ~1575 and ~1530 Ma the Western Fold Belt around Mount Isa was undergoing high-temperature/low-pressure peak metamorphism. This metamorphic window reflects the prolonged duration of tectonic shortening during the Isan Orogeny. It appears that regional tourmalinisation resulted from prolonged hydrothermal activity related to this compressional deformation. The best estimate of peak metamorphism is now ca. 1557±17 Ma. The occurrence of tourmaline with small Cu and U deposits and paragenetic relationships with minor Close 754 Robert J. Duncan · Andy R. Wilde · Roland Mass · Katherine Bassano sulphides suggests that during hydrothermal fluid movement driven by metamorphism, metals of economic interest were mobile. The regional spatial and temporal association of tourmalinisation with silicification indicates that the silica-rich halo around the Cu orebodies may have formed at a similar time. Acknowledgements The PbSL routines are based largely on unpublished experiments by M Tonelli, J Hergt and J Woodhead (Univ. of Melbourne). The work reported is part the pmd*CRC with support from Xstrata Copper. Thanks to R. Romer for reviewing this abstract. References Blake DH, Stewart AJ (1992) Stratigraphic and tectonic framework, Mount Isa Inlier. In: Stewart AJ, Blake DH (eds) Detailed studies of the Mount Isa Inlier. Aust Geol Surv Organ Bull 243: pp 1-11 Connors KA (1992) Tectonothermal evolution of the Mount Novit Ranges, Mount Isa Inlier, Australia. PhD Thesis, Monash University Connors KA, Page RW (1995) Relationships between magmatism, metamorphism and deformation in the western Mount Isa Inlier, Australia. Precambr Res 71: 131-153 Dahl PS (1997) A crystal-chemical basis for Pb retention and fissiontrack annealing systematics in U-bearing minerals, with implication for geochronology. Earth Planet Sci Lett 150: 277-290 Duncan RJ, Wilde AR (2004) Tourmaline at Mount Isa, Australia: a tracer of metal-rich hydrothermal fluid flow. In: Muhling J et al. (eds) SEG 2004: Predictive Mineral Discovery Under Cover, Perth, Western Australia; Extended Abstracts, Centre for Global Metallogeny, The University of Western Australia Publication 33: 413 Frei R, Kamber BS (1995) Single mineral Pb-Pb dating. Earth Planet Sci Lett 129: 261-268 Hand M, Rubatto D (2002) The scale of the thermal problem in the Mt. Isa Inlier. In: Preiss VP (ed) Geoscience 2002: Expanding Horizons. Abstracts of the 16th Australian Geological Convention, Adelaide, SA, Australia 67: 173 Jiang SY, Yu JM, Lu JJ (2004) Trace and rare-earth element geochemistry in tourmaline and cassiterite from the Yunlong tin deposit, Yunnan, China: implications for migmatic-hydrothermal fluid evolution and ore genesis. Chem Geol 209: 193-213 Ludwig KR (2003) User’s Manual for Isoplot 3.00: A geochronological toolkit for Microsoft Excel. Berkeley Geochronology Center Spec Publ 4, California, p 70 Mathias BV, Clark GJ (1975) Mount Isa copper and silver-lead-zinc ore bodies; Isa and Hilton mines. In: Knight CL (ed) Economic Geology of Australia and Papua New Guinea. Aust Inst Mining Metall, pp 351-371 O’Dea MG, Lister GS, MacCready T, Betts PG, Oliver NHS, Pound KS, Huang W, Valenta RK (1997) Geodynamic evolution of the Proterozoic Mount Isa terrain. In: Burg JP, Ford M (eds) Orogeny through time. Geol Soc Spec Publ 121: 99-122 Perkins C, Heinrich CA, Wyborn LAI (1999) 40Ar/39Ar geochronology of copper mineralization and regional alteration, Mount Isa, Australia Econ Geol 94: 23-36 Roberts MP, Finger F (1997) Do U-Pb zircon ages from granulites reflect peak metamorphic conditions? Geology 25: 319-322 Rubenach MJ (1992) Proterozoic low-pressure/high-temperature metamorphism and an anticlockwise P-T-t path for the Hazeldene area, Mount Isa Inlier, Queensland, Australia. J Meta Geol 10: 333-346 Swager CP (1985) Syndeformational carbonate-replacement model for the copper mineralization at Mount Isa, Northwest Queensland; a microstructural study. Econ Geol 80: 107-125 Thériault RJ, Davies WJ (1999) Rapid extraction of Sr and Pb by ionspecific chromatography for thermal ionisation mass spectrometry analysis. In Radiogenic age and isotopic studies, report 12, Geol Surv Can Current Research 1999-F: 9-12 Wilde AR, Gregory MJ, Duncan RJ, Gessner K, Kühn M, Jones P (2005) Geochemical process model for the Mt Isa Cu-Co-Ag deposits, this volume Woodhead JD (2002) A simple method for obtaining highly accurate Pb isotope data by MC-ICP-MS. J Anal Atom Spec 17: 1-6 Close Chapter 7-9 7-9 Potassic alteration and veining and the age of copper emplacement at Mount Isa, Australia Melissa J. Gregory, Andy R. Wilde, Bruce F. Schaefer, Reid R. Keays pmd*CRC, School of Geoscience, Monash University, Melbourne, VIC 3800, Australia Abstract. Preliminary 187Re/188Os dating of whole rocks and sulphide separates from the Mount Isa copper orebody has generated an isochron age of 1367 ± 80 Ma (MSWD = 49; n = 6). This age is approximately 150 myr younger than published biotite 40Ar/39Ar ages previously assumed to date the copper-forming event at ca. 1523 Ma. These older ages are from rocks in which biotite is likely to be metamorphic rather than hydrothermal in origin. Unambiguous potassic alteration related to copper formation is characterised by biotite replacement of metabasalt (brownstones) and potassium feldspar replacement of meta-tuffs. Previous 40Ar/39Ar dating of biotite from brownstone yields 1352 Ma to 1385 Ma ages, while 87Rb/ 86 Sr dating of potassium feldspar altered tuffs gives 1323 Ma. Muscovite from the Buck Quartz Fault, considered a conduit for copper mineralising fluids, yields an 40Ar/39Ar age of 1324 Ma. We suggest that these ages more accurately reflect the age of copper emplacement, whereas the older 40Ar/39Ar ages more likely relate to cooling from peak metamorphism. Keywords. Mount Isa, Re-Os, potassic alteration 1 Introduction The Mount Isa copper deposit contains over 13 million tonnes of copper at 3.3 wt.%, and is hosted within the Proterozoic Urquhart Shale (Perkins 1990). Textural evidence suggests that chalcopyrite-pyrrhotite mineralisation occurred late in the tectonic history of the Mount Isa Inlier (Perkins 1984; Swager 1985; Valenta 1994; Waring 1990). The absolute age of copper mineralisation, however, is poorly defined. In this paper we discuss the available radiometric data and their significance. Most published data are from potassic phases, such as biotite, muscovite and potassium feldspar so it is necessary to review evidence for the relationship of such phases to copper deposition. 2 Metamorphic biotite 2.1 Eastern Creek Volcanics The Eastern Creek Volcanics below and to the east of the Mount Isa copper deposit have undergone lower greenschist facies metamorphism. Stable assemblages in the metabasalts include chlorite, albite, actinolite, epidote, calcite, titanomagnetite, magnetite, sphene and biotite. Biotite and chlorite define a metamorphic foliation in some areas. 2.2 Urquhart Shale Biotite is a common phase in metasedimentary rocks of the Mount Isa Group, including the Urquhart Shale. It defines the peak metamorphic foliation, and ranges in composition from Fe-rich to more magnesian phlogopite, depending on the host rock composition. Biotite is rare in the intense silica-dolomite alteration associated with economic copper mineralisation, but distinctive biotite-magnetite-stilpnomelane bearing rocks occur in close proximity to Pb-Zn ore (Fig. 1). Swager et al. (1987) interpret these zones to be the result of the interaction of the copper mineralising fluid with pre-existing iron-rich metasomatic rocks in the Urquhart Shale. Conversely, Waring (1990) suggests that these zones were the result of greenschist facies metamorphism. He notes that the biotite-magnetite-stilpnomelane assemblage is cut by dolomite veins considered to be contemporaneous with copper emplacement. 3 Absolute age of metamorphism The absolute age of the peak (maximum temperature and pressure) of regional metamorphism is poorly constrained. Biotite from the Eastern Creek Volcanics 14.5 km east of the mine, gave 40Ar/39Ar ages of 1534 ± 4 Ma and 1524 ±3 to 1554 ± 2 Ma (Perkins et al. 1999). These ages were interpreted to reflect hydrothermal activity at the end of regional metamorphism at 1534 Ma. This date is consistent with the SHRIMP U-Pb zircon ages of 1532 ± 7 Ma by Connors and Page (1995) and the whole rock 87Rb/86Sr ages of 1544 ± 12 Ma from Page and Bell (1986). U/Pb monazite dating by Hand and Rubatto (2002) suggests that peak metamorphism is older at ca. 1575 Ma. This older age is supported by new metamorphic tourmaline dates of 1559 ± 17 Ma and 1577 ± 52 Ma using PbPb step leaching (Duncan et al. this volume). 4 Potassic alteration 4.1 Urquhart Shale There are over 60 potassium-rich layers within the Urquhart Shale throughout the Mount Isa mine sequence (Croxford 1964). These layers are typically less than 5 cm Close 756 Melissa J. Gregory · Andy R. Wilde · Bruce F. Schaefer · Reid R. Keays thick, and characterised by an unusual pale gray colour. Croxford (1964) interpreted these layers as tuffs, based on the rare presence of glass shards. The tuffs consist of microcline (after adularia), quartz, rutile, hematite, sericite and carbonate. Perkins (1997), however, found that only the tuffs in the mine area were potassium-rich, suggesting a hydrothermal origin for potassium. 4.2 Eastern Creek Volcanics Detailed logging of drillcore at the northern end of the Mount Isa copper deposit (mine section 38,000 mN) has defined a zone of potassium-rich alteration within the Eastern Creek Volcanics, below copper mineralisation in the Urquhart Shale (Fig. 1). This zone, which is dominated by biotite, has previously been called brownstone and has been reported in many deep drillholes that have inter- sected the Eastern Creek Volcanics below the Mount Isa copper deposit (e.g. Hannan et al. 1993). This biotite-rich alteration parallels the Paroo Fault (Fig. 1) and is thicker (up to 70m) where copper mineralisation overlies the fault. In thin section, the biotite-dominated rocks have a groundmass of chlorite, albite and ilmenite that is overprinted by a fine network of biotite veinlets. Undeformed biotite also pseudomorphs weakly foliated chlorite. 4.3 Potassium feldspar veining Away from biotite-rich zones, potassium-rich veins are observed in the metabasalts of the Eastern Creek Volcanics. These veins are dominated by potassium feldspar, calcite, quartz and chalcopyrite and are commonly 2 to 5 mm thick. Typically the veins are zoned with potassium feldspar lining the metabasalt contact and calcite with lesser quartz in the core. Chalcopyrite is intergrown with the potassium feldspar. The vein boundaries are sharp and cross cut the peak metamorphic foliation found within the metabasalts. 5 Absolute age of ore formation Preliminary 187Re/188Os isotopic analyses of whole rocks and sulphide separates from the Mount Isa copper orebody define an imprecise isochron age of 1367 ± 80 Ma (Fig. 2). 87Rb/86Sr dating of potassic altered tuff horizons from the mine area define isochron ages from 1341 ± 21 Ma to 1474 ± 202 Ma (Farquharson and Richards 1975; Page Close Chapter 7-9 · Potassic alteration and veining and the age of copper emplacement at Mount Isa, Australia 1981). A significantly more precise age is achieved by combining the two data sets (as all samples are from the same lithology and area) to give an age of 1323 ± 12 Ma (Gregory et al. 2004). A radiogenic initial ratio of 0.7418 ± 0.0061 suggests isotopic resetting may have occurred at this time (Farquharson and Richards 1975; Gregory et al. 2004; Page 1981). Perkins et al. (1999) reported numerous 40Ar/39Ar dates for biotite and muscovite from the Urquhart Shale and the Eastern Creek Volcanics (Table 1). Biotite and phlogopite from stilpnomelane-magnetite zones gave 40Ar/39Ar ages of 1523 ± 3 Ma and 1516 ± 3 Ma, from which 1523 Ma was interpreted as the most likely date of copper ore deposition (Perkins et al. 1999). Perkins et al. (1999) also dated biotite separates from brownstones within the Eastern Creek Volcanics adjacent to the copper deposit. 40Ar/39Ar dating of these separates gave distinct plateau ages at 1352 ± 3 Ma and 1385 ± 3 Ma, which was interpreted as the age of late stage fluid flow. Muscovite from the Buck Quartz Fault, interpreted to be the inflow zone for the copper bearing fluids (Waring 1990), gave an 40Ar/39Ar age of 1324 ± 2 Ma, also interpreted as due to minor late stage fluid flow (Perkins et al. 1999). 6 Discussion and conclusions Biotite and phlogopite are virtually absent from intensely altered and mineralised rocks which form the Mount Isa copper deposit but there is a close spatial relationship between biotite-rich alteration below the Paroo Fault and copper mineralisation above the fault. The biotite overprints the metamorphic foliation and the spatial relationships and timing supports the idea of hydrothermal fluid 757 flow along the fault, as suggested by Hannan et al. (1993) and Heinrich et al. (1995). Chalcopyrite-bearing potassium feldspar veins overprint the metamorphic foliation and therefore have the same relative timing as the biotite-rich alteration and the copper ore. The presence of both biotite-rich alteration below the Paroo Fault and potassium feldspar-rich veins demonstrates the presence of a potassium and copper-rich fluid. This fluid post-dates regional metamorphism and is spatially associated with the Mount Isa copper deposit. A number of isotopic dating techniques suggest that the peak of metamorphism at Mount Isa occurred prior to 1532 Ma and possibly prior to 1575 Ma. Emplacement of the Mount Isa copper deposit, based on numerous studies, clearly postdates the metamorphic peak. The absolute age of copper emplacement however, and particularly the gap between the conclusion of metamorphism and ore formation has been poorly defined. Our re-evaluation of published 40Ar/39Ar and 87Rb/86Sr data on potassic hydrothermal alteration, together with our preliminary 187Re/188Os dating of sulphide ore suggest that copper mineralisation was emplaced between 1300 Ma and 1400 Ma, at least 130 million years after the metamorphic peak. An alternative interpretation may be that the terrain remained above the closure temperature for these systems for several hundred million years after the peak of metamorphism. We suggest that the ca. 1523 Ma age of Perkins et al. (1999), previously assumed to be the date of copper ore formation, instead dates cooling from the metamorphic peak. The maximum temperature of ore formation is suggested to be between 300 and 350°C (Heinrich et al. 1989; Heinrich et al. 1995), and may not have exceeded the Ar closure temperature range of the metamorphic biotite. Therefore, there is significantly more evidence to support a ca. 1350 Ma age for copper mineralisation compared with the previously accepted ca. 1523 Ma age. This has implications for the genetic models proposed for the formation of the Mount Isa copper deposit. Acknowledgements Work reported here was conducted as part of the pmd*CRC with support from Xstrata Copper. References Connors KA, Page RW (1995) Relationships between magmatism, metamorphism and deformation in the western Mount Isa Inlier, Australia. Precambr Res 71:131-153 Croxford NJW (1964) Origin and significance of volcanic potashrich rocks from Mount Isa. Inst. Min. & Met. Tr. 74:33-43 Duncan RJ, Wilde AR, Maas R, Bassano K (2005) Syn-metamorphic dates for tourmaline formation around Mount Isa, North-west Queensland, Australia, this volume Close 758 Melissa J. Gregory · Andy R. Wilde · Bruce F. Schaefer · Reid R. Keays Farquharson RB, Richards JR (1975) Isotopic remobilization in the Mount Isa tuff beds. Chem Geol 16:73-88 Gregory MJ, Wilde AR, Keays RR, Schaefer BF (2004) Preliminary ReOs dating of the Mount Isa copper ores, Northwest Queensland. Barnicoat AC, Korsch RJ (eds) Predictive Mineral Discovery Cooperative Research Centre – Extended Abstracts, Geoscience Australia Record 2004/09, pp 79 Hand M, Rubatto D (2002) The scale of the thermal problem in the Mt Isa Inlier. In: Preiss VP (ed) Geoscience 2002: Expanding Horizons, 16th Australian Geological Convention, Adelaide, South Australia, pp 173 Hannan KW, Golding SD, Herbert HK, Krouse HR (1993) Contrasting alteration assemblages in metabasites from Mount Isa, Queensland; implications for copper ore genesis. Econ Geol 88:1135-1175 Heinrich CA, Andrew AS, Wilkins RWT, Patterson DJ (1989) A fluid inclusion and stable isotope study of synmetamorphic copper ore formation at Mount Isa, Australia. Econ Geol 84:529-550 Heinrich CA, Bain JHC, Mernagh TP, Wyborn LAI, Andrew AS, Waring CL (1995) Fluid and mass transfer during metabasalt alteration and copper mineralization at Mount Isa, Australia. Econ Geol 90:705-730 Page RW (1981) Depositional ages of the stratiform base metal deposits at Mount Isa and McArthur River, Australia, based on U-Pb zircon dating of concordant tuff horizons. Econ Geol 76:648-658 Page RW, Bell TH (1986) Isotopic and structural responses of granite to successive deformation and metamorphism. Journal of Geology 94:365-379 Perkins C, Heinrich CA, Wyborn LAI (1999) 40Ar/39Ar geochronology of copper mineralization and regional alteration, Mount Isa, Australia. Econ Geol 94:23-36 Perkins WG (1984) Mount Isa silica dolomite and copper orebodies; the result of a syntectonic hydrothermal alteration system. Econ Geol 79:601-637 Perkins WG (1990) Mount Isa copper orebodies. In: Hughes FE (ed) Geology of the mineral deposits of Australia and Papua New Guinea. Aust Inst Mining Metall, pp 935-941 Perkins WG (1997) Mount Isa lead-zinc orebodies; replacement lodes in a zoned syndeformational copper-lead-zinc system? Ore Geol Rev 12:61-111 Swager CP (1985) Syndeformational carbonate-replacement model for the copper mineralization at Mount Isa, Northwest Queensland; a microstructural study. Econ Geol 80:107-125 Swager CP, Perkins WG, Knights JG (1987) Stratabound phyllosilicate zones associated with syntectonic copper orebodies at Mt. Isa, Queensland. Aust J Earth Sci 34:463-476 Valenta R (1994) Syntectonic discordant copper mineralization in the Hilton Mine, Mount Isa. Econ Geol 89:1031-1052 Waring CL (1990) The Genesis of the Mount Isa Copper Orebodies. PhD, Monash University Close Chapter 7-10 7-10 Contact metamorphism at the manganese deposits of the Noda-Tamagawa Mine, northeast Japan: Insight from oxygen isotope data of manganese minerals Ken-ichiro Hayashi Doctoral Program in Earth Evolution Sciences, Graduate School of Life and Environmental Sciences, University of Tsukuba, Tsukuba 305-8572, Japan Abstract. Manganese ores of the Noda-Tamagawa mine are metamorphosed equivalents of bedded-type sedimentary manganese deposits. The ore lenses are typically zoned with a central pyrochroite-hausmannite zone, outer tephroite zone, and outermost rhodonite zone closest to the wall rock chert. The δ18O (VSMOW) values of 65 tephroite, 32 rhodonite and eight quartz samples from the manganese ores and chert are in the ranges of 9.9–20.0‰, 11.7– 20.3‰ and 23.0–23.9‰, respectively. The overall order of 18O-enrichment corresponds to the order of equilibrium fractionation among these minerals. However, the temperatures calculated from quartz-rhodonite and rhodonite-tephroite pairs from neighboring ore zones do not give temperatures consistent with those estimated from the mineral assemblages in the wall rocks. These data suggest that equilibrium was not established among neighboring mineral pairs, H2O, and CO2 during metamorphism. The fluid/rock ratios during metamorphism were very low (<< 1). Keywords. Manganese deposit, oxygen isotope, contact metamorphism, metamorphic fluid 1 Introduction Manganese ores of the Noda-Tamagawa mine are highly metamorphosed and folded. This metamorphism makes it difficult to obtain information on the primary features of the deposits, such as the original mineralogy, chemical composition, and environment of deposition. Despite these difficulties, the deposit is interpreted to be the metamorphosed equivalent of bedded-type sedimentary manganese deposits. The main objective of this study is to elucidate the origin and metamorphic history of the manganese ores at Noda-Tamagawa using the δ18O relationships among various metamorphic Mn-bearing silicate minerals. These data constrain the temperatures of metamorphism, fluid/rock ratios, and composition of the metamorphic fluids. 2 Geology of the Noda-Tamagawa mine The manganese deposits of the Noda-Tamagawa mine are situated in the northeastern part of a roof pendant of the granodiorite body. The roof pendant is ca. 8 km (N-S) x 12 km (E-W) in area, and is comprised of the Jurassic Formation. In the vicinity of the Noda-Tamagawa mine, these rocks have been hornfelsed due to the thermal meta- morphism by the granodiorite. Sillimanite, andalusite, and cordierite are present in some pelitic hornfels near the manganese ore bodies. As a result of the thermal metamorphism, a distinct zoning of manganese minerals developed in each ore lens, on a scale of 2 to 5 m. Pyrochroite (Mn(OH) 2) and hausmannite (Mn3O4) typically occupy the central part of the ore lens (0 to 1 m in thickness), surrounded by a tephroite (Mn2SiO4) ore, and an outer rhodonite (MnSiO3) ore. The major Mn-bearing minerals in the NodaTamagawa mine can be represented in the MnO-SiO2Al2O3 system. The principal zoning sequence in the ore lenses of the Noda-Tamagawa mine corresponds to a trend of decreasing MnO content (and increasing SiO2 content) toward the wall rocks. Bulk chemical compositions of the manganese ores change along the MnO-SiO2 join from near the MnO apex for pyrochroite-hausmannite ore in the central part of the bed to rhodonite near the wall rock. 3 Oxygen isotope study Mineral grains were hand picked from thick sections of ~0.5 mm under a binocular microscope. Since most ore samples of this study are monomineralic in nature, the purities of mineral separates were better than 95 %. Extraction of oxygen from quartz, rhodonite and tephroite was carried out using a CO2-laser and BrF5 by a fluorination method similar to that described by Hayashi et al. (2001). The reproducibility of the δ18O values was better than ±0.2 ‰. 4 Results and discussion The δ18O values of quartz samples from 3 localities of the mine have a narrow range from 23.0 to 23.9 ‰. Quartz from thin quartz layers in rhodonite ore has essentially the same δ18O value as quartz in the wall rock chert. Thirtytwo samples of rhodonite from rhodonite ore have δ18O values that range from 11.7 to 20.3 ‰; 65 samples of tephroite from tephroite ore and have values from 9.9 to 20.1 ‰. The order of 18O enrichment is generally quartz > rhodonite > tephroite, which corresponds to the ex- Close 760 Ken-ichiro Hayashi pected order of enrichment for isotopic equilibrium between minerals. Reversals in the order of 18O enrichment (i.e., nonequilibrium relationships) was observed for some rhodonite and tephroite pairs that were collected from zones separated by a distance of less than 1 m. The δ18O values for the series of samples from ore stope L13S78 do not show a symmetrical pattern from the wall rocks toward the center of the ore lens. In general, the δ18O values of both rhodonite and tephroite are higher in the footwall of the ore zone than those in the hanging wall. Because the manganese ores in the Noda-Tamagawa mine are generally monomineralic on a hand specimen scale, truly coexisting mineral pairs are difficult to obtain. However, if the Mn-silicates and oxides were both formed from MnCO3 and SiO2 (i.e., the most probable primary mineral assemblage of the Mn ores before metamorphism) in conditions accompanying a large amount of metamorphic fluid, isotopic equilibrium may be expected among minerals in samples up to a few meters apart. Isotopic equilibrium temperatures were calculated for mineral pairs in the neighboring zones within individual ore lenses (Fig. 1). Except for one very high temperature, three quartz-rhodonite and four rhodonite-tephroite pairs give temperatures between 545°C and 145°C. These temperatures are much lower than the estimated metamorphic temperatures and suggest that the minerals did not equilibrate at peak temperature. The presence of sillimanite, although it is rare in the pelitic hornfelses near the manganese ore bodies suggests that the peak metamorphic temperature was near the stability limits for andalusite and sillimanite (ca. 600°C at P= 2kb). The δ18O values for H2O and CO2 in equilibrium with quartz, rhodonite and tephroite at the calculated temperatures are variable, 7.6 to 18.4 ‰ for H2O and 16.7 to 33.6 ‰ for CO2. These data suggest that the equilibrium was not established among neighboring mineral pairs, H2O, and CO2 during the metamorphism. At high fluid/rock ratios, isotopic equilibrium between the neighboring (but non-coexisting) minerals would be expected. Therefore, our data suggest that the fluid/rock ratios during metamorphism were very low (<< 1) or that fluids with different isotopic compositions were present. A comparison of δ18O values between the manganese silicate minerals of this study and calc-silicate minerals from skarn deposits provides constraints on the nature of metamorphism and the origin of the isotopic composition of the Mn-minerals. As the skarn minerals were probably equilibrated with magmatic or meteoric water (e.g. El Rhazi and Hayashi 2002), the relatively narrow range of δ18O values of the skarn minerals was probably controlled by the δ18O values of skarn-forming water. In contrast, the wide range of δ18O values for the manganese minerals in this study suggests that their isotopic compositions mainly reflect the precursor minerals. The contribution of 18O-depleted fluids during metamorphism was not important. References El Rhazi M, Hayashi K (2002) Mineralogy, geochemistry, and age constraints on the Beni Bou Ifrour skarn type magnetite deposit, northeastern Morocco. Resource Geology 52: 25-39 Hayashi K, Maruyama T, Satoh H (2001) Precipitation of gold in a low-sulfidation epithermal gold deposit: insights from a submillimeter-scale oxygen isotope analysis of vein quarts. Economic Geology, 96: 211-216 Close Chapter 7-11 7-11 Isotopic geochemistry of Mesozoic igneous rocks and mineralization of Shanmen silver deposit in Yi-Su Basin, Jilin Province Huang Wenbin Institute of Mineral Resources, Chinese Academy of Geological Sciences, Beijing 100037, and Chinese Geological Library, Beijing 100083, China Shen Haoche JIlin University, Changchun Jilin, 130021, China Fen Lin Research Institute, China Water Northeastern Investigation Design and Research Co. Ltd., Changchun, 130021, China Abstract. The present study focuses on isotopic geochemistry of the Mesozoic igneous rocks and the Shanmen silver deposit in Yi-Su basin. Petrochemistry, isotopic geochemistry and isotopic geochronology are used to explore the relationship between regional magmatic activity and the formation of the ore deposit. In this study, we explore the isotopic geochemistry in the deposit and the surrounding igneous rocks by studying Rb, Sr, Pb, S, H and D isotopes. This helps us to discern the source of the economic minerals and the metallogenetic mechanism responsible for the formation of the Shanmen silver deposit. Keywords. Igneous rock, isotopic geochemistry, silver deposit, source of ore material 1 Introduction The Yi-Su basin is located in the fold zone of the TianShanXinan orogenic belt, where two deep parallel faults known as the Yi-Su fracture zones, are oriented 45~50°E and extend to the base of the lithosphere. The strata from the Paleozoic group to the Cenozoic group lie along the side of the basin. Metamorphosed igneous rocks that have experienced alteration and compressional deformation, outcrop around the outer edge of the basin. Many economic deposits have been discovered in this region, including iron, copper, gold, silver, and coal, fluorite deposits. These deposits are controlled by fractures and show an intimate relationship with Mesozoic igneous rocks. The Shanmen silver deposit is located in the Yi-Su basin. In this paper, we present a detailed study of isotopic geochemistry of the Mesozoic igneous rocks and the sliver ore in order to determine the relationship between magmatic activity and mineralization. 2 Isotopic geochemistry and formation of igneous rocks 2.1 Petrochemistry A variety of igneous rocks from the Herynian to Himalayan can be found in the Yi-Su basin.Neutral and acidic magmatic rocks comprise about 70% of the igneous rocks. The petrochemical composition of neutral and acidic igneous rocks shows that the younger rocks are relatively richer in Si and alkali elements. As rocks get older, Na2O content, and especially K2O content gradually rise. With the evolution of magma from neutral to the acidic-alkali, the petrochemical composition of the rocks shows a range in SiO2 content from 51.0% to 78.9%. Alkalinity ranges from Na2O>K2O to K2O<Na2O. Initial 87Sr/86Sr ratios vary from 0.74 to 0.70. These geochemical characteristics indicate that the netural and acidic magma was derived from the deep earth. 2.2 Genesis of igneous rocks 2.2.1 Mantle–derived (M-Type) igneous rocks Mantle-derived igneous rocks occur sparsely in this region, with the exception of large scaleHimalayan alkali basalts which are found along the Yi-Su deep fault. The 87Sr/86Sr ratio determined for olivine inclusions in basalt is 0.738. Because the geologic age of these basalts is relatively young, the 87Rb content is fairly low. The half-life of 87Rb is 48.8 b.y.. We suggest that the 0.738 may represent the initial 87Sr/86Sr ratio in the basalt. This indicates that the basaltic magma was derived from the upper mantle. 2.2.2 Mantle-crust mixed (MC-type) igneous rocks The rocks derived from both mantle and crustal materials are controlled by a basement rift, which lies in the topographically lower region of the basin. Most of the neutral-acidic and acidic igneous rocks occur in this locality. The initial 87Sr/86Sr ratio in these rocks ranges from 0.705 to 0.710. The δ18O value in the quartz varies from 7.8‰ to 8.5‰. The Rb/Sr ratio ranges from 0.6 to 0.4. SiO2 content varies form 57% to 72%, whereas Na2O>K2O, Al2O3/Na2O+CaO+K2O = 1, and f ’ (ω%) varies from 0.1 Close 762 Huang Wenbin · Shen Haoche · Fen Lin to 0.4. These characteristics can be used to identify igneous rocks derived from both crustal and mantle material in the relative deeper earth. 2.2.3 Crustal-derived (C-Type) igneous rocks Crustal-derived igneous rocks are mainly located in the folded region of the basin, and are controlled by regional fracture zones and folds. In this locality, the crust is thick. The initial 87Sr/86Sr ratio of these igneous rocks ranges from 0.716 to 0.720. The δ18O value in the quartz is l0‰, and the Rb/Sr ratio is high. The rocks are rich in Si and K, and poor in Ca. SiO2 content varies from 74% to 98% K2O>Na2O, f’ (ω%) varies from 0.4~0.7. These characteristics can be used to identify rocks derived from crustal materials. 3 Isotopic and geochemical features of the silver deposit 3.1 Regional geology The Shanmen silver deposit is located along the western margin in the Jihei fold system of the TianShan-Xinan orogenic belts. The main strata are the Cambrian-Ordovician Baoan group and the Middle Ordovician Huangyingtun group. The latter has undergone silicification, sericitization and carbonatization. Igneous rocks outcrop in the uplifted area, which intrudes along deep fractures, mainly consisting of monzogranite, biotite granite, and quartz diorite (Fig. 1). The Indosin Kaodaozi diorite, Wuolong hornblende pyroxenite and Yanshanian granites display a close relationship with the silver deposit. The Kandaozi pluton, which controls the distribution of the main ore body, is located near the upper section of the silver deposit, and overlaps the Huangyintun group. The Wuolong pluton, which forms the base of the ore body, lies on the eastern edge of the Kaodaozi pluton. It has a skewed contact with the main fracture, and forms the wall rock for the deposit. The silver deposit is 10 km long, 1~2 km wide, and is distinctly controlled by NE-NNE factures. These fractures divide the deposit into 5 ore blocks from south to north: the Zhangjiatun block, the Longwang block, the Wuolon block, the Gudong block and the Yingpan block. The Wuolong block contains the majority of the ore reserves, which occur in marbles and meta-siltstones from the middle-upper Huangyingtun group. The ore minerals are mainly silver (50%), galena, sphalerite, secondly pyrite and chalcopyrite. 3.2 Petrography and petrochemistry of the mine region The Kaodaozi pluton is the host rock for the main ore body. It consists mainly of diorite, with lesser quartz diorite and quartz monzonite. The petrochemical composition is as follows: K2O/Na2O<1, Al/K+Na+2Ca<1, [Fe2O3+FeO+1/ 2(MgO+Ca)] is 11.65, (Si+Na+K)/Fe2++Fe3++Mg) is 6.03, (Cao+Na2O+K2O/(Al2O3+CaO+Na2O) is 1.70, and the coefficient of consolidation is 24.37. The main accessory minerals are titanite, apatite and barringerite. The geochemistry of the rock is as follows: the 207Pb/ 204Pb ratios vary from 15.56 to 15.64, the 206Pb/204Pb ratios from 18.32 to 18.35, the 208Pb/204Pb ratios from 38.24 to 38.47, respectively. The initial 87Sr/86Sr ratio is 0.70544. The δEu values range from 0.92 to 1.02. The LRee/HRee is 5.93. Therefore, we suggest the Kaodaozi diorite is likely derived from the mantle-crust melting. Whole rock UTh-Pb dating, measured by MS, produces an age of 193.3 Ma. Pb-Pb dating of zircon in the quartz diorite produces an age of 187.8 Ma. The Wuolong pluton forms the base of the ore body, and is the wall rock for the deposit. It consists mainly of adamellite, with lesser granite and moyite. The petrochemical composition is as follows: K2O/Na2O>1, Al/ K+Na+2Ca>1, SiO2 content is 73.4%. The main accessory minerals are zircon, apatite and magnetite. The geochemistry of the rock is as follows: the 207Pb/ 204Pb ratios vary from 15.58 to 15.61, the 206Pb/204Pb ratios from 18.56 to 18.61, the 208Pb/204Pb ratios from 38.71 to 38.85, respectively. The initial 87Sr/86Sr ratio is 0.7158. The δEu value is 0.45. Therefore, we suggest the Wuolong pluton is likely derived from mantle-crust melting. U-Th-Pb dating for zircon, measured by MS, produces an age of 150Ma. Whole rock K-Ar dating produces an age of 158 Ma. Close Chapter 7-11 · Isotopic geochemistry of Mesozoic igneous rocks and mineralization of Shanmen silver deposit in Yi-Su Basin, Jilin Province 3.3 Isotopic and geochemical evidence of genesis of the Shanmen silver deposit A histogram is plotted for the 22 ore samples. The results show that the 208Pb/204Pb ratio shows normal distribution with a single population except one. This indicates that Pb isotopes come from a distinct parental material, and that the source of mineralization is separate. The model age, computed by a Doe single-stage model using Pb isotopes, is a negative age. This reveals that Pb isotopic values within the ore zone are similar to isotopic values expected from Pb derived from the upper mantle The model age computed by the Stacey two-stage formula is 180 Ma. This model age, which represents the age of the formation of the silver deposit, is close to the age of formation of Kaodaozi and Wuolong plutons. Moreover, the Pb isotopic composition in the ore is the same as the Pb isotopic composition of the two plutons, but differs from the stratum of Hangyintong group. Therefore, the source of Pb isotopes in the ore has an intimate relationship with magmatic activity. The Pb isotopic composition in galena ore may be compared with Pb isotopic composition in the rocks which 763 come from the modern mantle or the crust, in order to discern the source of minerals for the younger deposits (Y. W. Cheng, 1983). Fig. 2, Fig. 3 illustrate that Pb isotopic composition of the galena is between the Pb composition of the tholeiite found at mid-oceanic ridges (representing the upper mantle), and the Pb composition of island-arc magmas found along the western coast of the Pacific Ocean. The results reveal that the mineral material is derived from the deep earth, and formed from a magma composed of mixed upper mantle and crust. We compare the Pb isotopic composition in the galena in the Shanmen deposit with the Phanerozoic metal deposits in China. The Pb isotopic composition in the metal deposits, which are related to the Mesozoic lava or granodiorite in China is as follows (Cheng 1984): the Pb composition is steady, The 207Pb/204Pb ratios vary from 15.3 to 15.6, and the 206Pb/204Pb ratios >17.5. In the Shanmen silver deposit, the 206Pb/204Pb ratios vary from 18.017 to 18.149, whereas the 207Pb/204Pb ratios vary from 15.418 to 15.525. Therefore, we suggest the minaeralization may be related to the intrusion of the granodiorite. We measured the δ34S values in galena, sphalerite and pyrite in the ore bodies, wall rocks, and local strata. (Table 1). The δ34S data is as follows: the variation of the δ34S values is narrow, the δ34S values are low in the ore bodies and the wall rocks, This is similar to the δ34S values in meteorites. The δ34S values are negative in the stratum. The average δ34S values in pyrite are -1.37‰. This is within the range of δ34S values in meteorites. These results indicate that the mineral material is derived from the deep earth. The δ34S values from different ore bodies show a normal distribution. Most of them cluster around -2.0‰. The δ34S values in the ore minerals are as follows: δ34S (FeS) > δ34S(ZnS) > δ34S(PbS). This agrees with the equilibrium conditions for sulfur isotopes in hydrothermal systems. Therefore, these minerals are paragenetic. Thermometry of sphalerite galena shows that the metallogenic temperature was between 160 to 300oC. Close 764 Huang Wenbin · Shen Haoche · Fen Lin The δ18OH2O values in quartz show that mineralized fluids consisted of magmatic water in the early stages, and meteoric waters mixed with magmatic waters during the later stages. The δD values range from -92% to 106%. Thereby, we suggest the silver deposit was formed in the same hydrothermal system. 4 Conclusions The genesis of the igneous rocks in the study region falls into two groups: crustal-derived igneous rocks, and mantle-crustal mixed igneous rocks. These two groups of igneous rocks have distinct differences in petrochemistry, mineral assemblage, and geologic environment of formation. On the basis of detailed study of geology and isotopic geochemistry of Rb, Sr, Pb, S, H, and O in both ore and wall rock, we suggest the silver deposit is a mesothermal ore deposit, and the mineral material is derived form the mixed upper mantle and crust. The metallogenesis of Shanmen silver deposit has an intimate relationship with magamatic activity. The origin of mineral material and mineralizing fluids is complex. Magmatic activity is the metallogenetic mechanism of formation for this silver deposit. References Amstrong BL, Hales WH (1977) Rb-Sr and K-Ar geochemistry of Mesozoic grantic rock and their isotopic composition. Ball, Geol. Soc. Am 88 Cheng YW, Zhu BQ (1984) The feature of isotopic composition of ore lead and genesis. Geochemica 3: 35-45 Hu X, Xu C, Niu S (1990) Evolution of the early Paleozoic continental margin in northern margin of the North China Platform. Beijing: Peking University Publishing House, 6-34 Li L, Zheng YF, Zhou JB (2001) Dynamic model for isotope Pb evolution in the Continental Crust of China. Acta Petrologica Sinica 1:63-67 Liang YH, Zheng, XS, Zhang S (1996) The discussion on the relation between the magmatite and the silver deposit and exploration of the mechanism of the formation of the silver deposit in Sipin. Songliao Journal (Nature Science Edition) 1: 41-45 Liu, JQ (1987) Geochronology Study of Cenozoicin Lava in North East China. Acta Petrologica Sinica 4: 21-31 Taylor SR, Mclennan SM (1985) The continental crust: Its composition and evolution. Oxford: Blackwell, 67-96. Wang FK (1994) Analysis on metallogenetic conditions of the Shanmen Silver Deposit in Sipin, Jilin Povice. Jilin Geology 3: 9-16 Wang FK (1997) A new understanding of the Mesozoic intrusive rock genesis and relationship with metallogeny in the Shanmen Silver Deposit, Sipin Area. Jilin Geology 3: 9-26 Close Chapter 7-12 7-12 Platinum group elements as useful genetic tracers for the origin of polymetallic Ni-Mo-PGE-Au sulfide ores in Lower Cambrian black shales, Yangtze Platform, South China S.-Y. Jiang, Y.-Q. Chen, H.-F. Ling, J.-H. Yang, H.-Z. Feng State Key Laboratory for Mineral Deposits Research, Department of Earth Sciences, Nanjing University, Nanjing, China Abstract. The polymetallic Ni-Mo-PGE-Au sulfide ores occur in the Lowermost Cambrian Niutitang Formation of a thick black shale sequence in Yangtze Platform of South China. The origin for this special type of sulfide ore has been hotly debated. Three genetic models have been proposed: (1) extraterrestrial impact origin (Fan et al. 1984); (2) submarine hydrothermal exhalative origin (Coveney et al., 1992; Lott et al. 1999; Steiner et al. 2001); (3) seawater scavenging origin (Mao et al. 2002). In this paper, we discuss the origin for this special type of sulfide ore based on platinum group element geochemistry. We suggest that the chondrite-normalized PGE patterns of the sulfide ores show some distinctive difference from the seawater pattern and may indicate a submarine hydrothermal input for the metal enrichments in the sulfide ore. We defined a new parameter, namely Pt anomaly (Pt/Pt*), and found that the Pt anomaly in the polymetallic Ni-Mo-PGE-Au sulfide ores is similar to those ancient and modern sea-floor massive sulfide deposits. Other platinum group element pairs, such as Pt/Pd, Ir/Pd, and Au/Pd ratios of the Ni-Mo sulfide ores also share some similarity with those of ancient and modern submarine massive sulfide deposits. In conclusion, we support the submarine hydrothermal exhalative origin for the sulfide ores, and suggest that this is a new type of sediment-hosted submarine hydrothermal exhalative sulfide deposits. Keywords. PGE, sulfide ore, black shale, Lower Cambrian, South China 1 Introduction The polymetallic Ni-Mo-PGE-Au sulfide ores occur in the Lowermost Cambrian Niutitang Formation of a thick black shale sequence on the Yangtze Platform of South China, which extend over 1600 kilometers length along a NE trending belt. Although this type of polymetallic Ni-MoPGE-Au mineralization has been known for more than 30 years, its origin has long been debated (Fan et al. 1984; Coveney et al. 1992; Horan et al. 1994; Lott et al. 1999; Steiner et al. 2001; Mao et al. 2002; Coveney 2003; Lehmann et al. 2003). Our study in recent years suggest that the occurrence of PGE and other metal anomalies and mineralizations in black shales may belong to a special class of sedimentary-exhalative sulfide deposits that can potentially provide economically significant PGE and other metal resources in the future. 2 Geological setting In South China, the polymetallic enrichment bed in the Lowermost Cambrian Niutitang Formation accounts for extreme enrichments of a large spectrum of metals, such as Mo, Ni, Se, Re, Os, As, Hg, Sb, Ag, Au, Pt, and Pd, with up to 106 to 109 fold enrichment relative to seawater values. Although this belt extends over 1600 km, economically minable ores occur mostly within the provinces of Guizhou and Hunan, with the most famous deposits being Huangjiawan near Zuuyi (Guizhou province) and Dayong near Zhangjiajie (Hunan province). Steiner et al. (2001) suggested that the linear trend of the Ni-Mo sulfide ore occurrence in South China may relate to structural controls by a major deep fault zone in the transitional area between the Neoproterozoic back arc basin and the platform. Lott et al. (1999) found footwall hydrothermal quartz-sulfide stockworks for the sulfide deposit, which may represent submarine hydrothermal venting systems. Mao et al. (2002) reported a Re-Os age for the Ni-Mo sulfide ores of 541 ± 16 Ma. Chen et al. (2003) also obtained a similar age using the Pb-Pb dating technique for the host black shales (531 ± 24 Ma). The major ore minerals are vaesite, bravoite, jordisite, and MOCs; and minor ore minerals include arsenopyrite, chalcopyrite, covellite, sphalerite, millerite, polydymite, gersdorffite, sulvanite, pentlandite, tennantite, tiemannite, violarite, and native gold. Gangue components consist of organic debris, siliceous rock, carbonate, clay, and phosphorite. 3 Platinum group element geochemistry The Platinum group element and their chondrite-normalized patterns are very useful indicators for the origin of ore deposits including those within black shales and submarine hydrothermal exhalative massive sulfide deposits (e.g., Coveney et al. 1992; Pasava 1993; Pan and Xie 2001; Pasava et al. 2004). 3.1 The Ir anomaly The polymetallic Ni-Mo-PGE-Au sulfide ores in South China were first reported by Fan et al. (1973) and were regarded as an entirely new type of sulfide ore, which contains up to several percent of Ni, Mo, As, together with substantial amounts of PGE and Au. In 1984, Fan et al. (1984) found high Ir values for these polymetallic Ni-Mo- Close 766 S.-Y. Jiang · Y.-Q. Chen · H.-F. Ling · J.-H. Yang · H.-Z. Feng PGE-Au sulfide ores, and consequently they suggested a meteorite impact model for the origin of these ores. However, this model was doubted and discarded by Conveney et al. (1992) who found that the Ir contents are actually relatively low (<0.02-2 ppb, average 1.7 ppb) compared with other PGEs (up to 700 ppb Pt and 1255 ppb Pd). Hence, Conveney et al. (1992) concluded that an extraterrestrial source seems unlikely for the Chinese polymetallic Ni-Mo-PGE-Au sulfide ores. 3.2 The Pt anomaly (Pt/Pt*) Jiang et al. (2003) proposed a new PGE parameter of Pt anomaly (Pt/Pt*), which can be used as a sensitive genetic tracer. By analogy with the Eu anomaly in chondrite-normalized REE patterns, a Pt anomaly can be defined using the following equation: where the PtN, RhN, and PdN are the chondrite-normalized values of the samples. The Pt/Pt* values are generally larger than 1 (positive Pt anamaly) for most crustal sources. In contrast, the mantle-derived sources display negative Pt anomaly with Pt/Pt* close to or less than 1. We found that the Pt/Pt* values for the host rocks of phosphorites, siliceous shales, and black shales in South China are significantly larger than 1, but the Pt/Pt* values for the Ni-Mo sulfide ores are close to 1, overlapping the values for Kuroko VMS-type sulfide ores. This similarity may imply a similar submarine hydrothermal origin for the Chinese Ni-Mo sulfide ores. This hypothesis supports other studies that favor a hydrothermal origin for the Chinese polymetallic Ni-MoPGE-Au sulfide ores (Murowchick et al. 1994; Li and Gao 1996; Lott et al. 1999; Steiner et al. 2001). (0.1-3.3) and the ancient massive sulfide ores (0.4-1.0), although the range in these deposits seems to be smaller. The Fe-Mn crusts, which scavenged PGEs from seawater, also show large Pt/Pd ratios ranging from 6 to 272, whereas Au/ Pd ratios show even larger variations. Hence, we suggest that a simple comparison of these noble metal ratios to those of seawater is by no means an adequate way to prove or disprove their derivation. Instead, we suggest that the correlations between the noble metal ratio pairs are more useful to differentiate hydrothermal origin from seawater origin. The comparison of Chinese Ni-Mo sulfide ores with submarine hydrothermal exhalative sulfide ores and Fe-Mn nodules and crusts in Pt/Pd vs Pt/Pt*, Pt/Pd vs. Ir/Pd, Au/Ir vs. Au/Pd diagrams demonstrate the similarity between the Chinese Ni-Mo sulfide ores with Kuroko VMS-type sulfide ores and modern sea-floor metalliferous sediments and sulfides, but a distinct contrast to Fe-Mn nodules and crusts. Taken together, we suggest that the Chinese Ni-Mo ores are likely to have a similar hydrothermal origin to modern and ancient sea-floor massive sulfide deposits. 4 Conclusions The ore genesis for the Chinese polymetallic Ni-Mo-PGEAu ores within the Lowermost Cambrian Niutitang Formation has been hotly debated. The increasing amount of data from field geology, fluid inclusions, geochemistry (trace, rare earth elements, and platinum group elements), and isotopes support a formation of these deposits via submarine hydrothermal venting systems, in an anoxic environment where abundant organic matter promotes extreme enrichment of redox-sensitive metals. According to our systematic PGE investigation, we propose a genetic model for the submarine hydrothermal ore-forming process, and suggest this is a new type of sediment-host Sedex deposits. 3.3 Platinum group element ratios Acknowledgements The Platinum group element ratios are diagonastic tools to trace ore genesis. Lehmann et al. (2003) suggested that the Chinese Ni-Mo sulfide ores have Pt/Pd and Au/Pd ratios around 1, quite close to seawater ratios (Pt/Pd= 0.8, Au/Pd=0.3), but are different from the Serra Pelada AuPd-Pt deposit of northern Brazil and the Rammelsberg deposit of Germany (Au>Pd>Pt). However, we found that the Pt/Pd ratios of magmatic Ni-Cu sulfide deposits are also commonly close to 1 (Barnes et al. 1985; Brugmann et al. 1989). In fact, the Pt/Pd ratio for the Chinese Ni-Mo ores and their host rocks, as well as for many modern and ancient sea-floor massive-sulfide deposits and Fe-Mn crusts show a relative large variation. We found that the Pt/Pd ratios of the Chinese Ni-Mo sulfide ores (0.320) are similar to their host rocks (0.5-14), and are also comparable to the modern sea-floor metalliferous sediments This research was supported by China National Science Foundation grants (40221301, 40372059, 40172041). Profs. Zhu Maoyan, Zhang Junming, and Wu Xianhe are thanked for their very helpful assistance in field work and for critical discussion. This is a contribution to the Sino-German joint project of Biological and Geological Processes of the Cambrian Explosion. References Barnes SJ, Naldrett AJ, Gorton MP (1985) The origin of fractionation of platinium-group elements in terrestrial magmas. Chem Geol 53: 303-323 Brugmann GB, Naldrett AJ, MacDonald AJ (1989) Magma mixing and constitutional zone refining in the Lac des Iles Complex, Ontario: Genesis of platinum-group element mineralization. Econ Geol 84: 1557-1573 Close Chapter 7-12 · Platinum group elements as useful genetic tracers for the origin of polymetallic Ni-Mo-PGE-Au sulfide ores in Lower Cambrian black shales Chen Y-Q, Jiang S-Y, Ling H-F, Feng H-Z, Yang J-H, Chen J-H (2003) Pb-Pb isotope dating of black shales from the Lower Cambrian Niutitang Formation, Guizhou Province, South China. Progr Nat Sci 13: 771-776 Coveney RM Jr (2003) Re-Os dating of polymetallic Ni-Mo-PGE-Au mineralization in Lower Cambrian black shales of South China and its geological significance-A discussion. Econ Geol 98(3): 661-662 Coveney RM Jr, Murowchick JB, Grauch RI, Michael D, Glascock D, Denison JD (1992) Gold and platinum in shales with evidence against extraterrestrial sources of metals. Chem Geol 99: 101-114 Fan D, Yang R, Huang Z (1984) The Lower Cambrian black shales series and the iridium anomaly in south China. Development in Geoscience, Inter Geol Congr, 27th, Moscow, 1984, Beijing, Science Press, 215-224 Fan D, Yang X, Wang Y, Chen N (1973) Petrological and geochemical characteristics of a nickel-molybdenum-multe-element-bearing Lower Cambrian black shale from a certain district in south China. Geochim 3:143-163 Horan MF, Morgan JW, Grauch RI, Coveney RM Jr, Murowchick JB, Hul-bert LJ (1994) Rhenium and osmium isotopes in black shales and Ni-Mo-PGE-rich sulfide layers, Yukon Territory, Canada, and Hunan and Guizhou Provinces, China. Geochim Cosmochim Acta 58: 257-265 Jiang S-Y, Yang J-H, Ling H-F, Feng H-Z, Chen Y-Q, Chen J-H (2003) Re-Os isotopes and PGE geochemistry of black shales and inter- 767 calated Ni-Mo polymetallic sulfide bed from the Lower Cambrian Niutitang Formation, South China. Progr Nat Sci 13: 788-794 Lehmann B, Mao J, Li S, Zhang G, Zeng M (2003) Re-Os dating of polymetallic Ni-Mo-PGE -Au mineralization in Lower Cambrian black shales of South China and its geological significance-A reply. Econ Geol 98(3): 663-665 Li S, Gao Z (1996) Siliceous rocks of hydrothermal origin in the Lower Cambrian black rock series of South China. Acta Mineral Sinica 16: 416-422 Lott DA, Coveney RM Jr, Murowchick JB (1999) Sedimentary exhalative nickel-molybdenum ores in South China. Econ Geol 94: 1051-1066 Mao J, Lehmann B, Du A, Zhang G, Ma D, Wang Y, Zeng M, and Kerrich R (2002) Re-Os dating of polymetallic Ni-Mo-PGE-Au mineralization in Lower Cambrian black shales of South China and its geologic significance. Econ Geol 97: 1051-1061 Murowchick JB, Coveney RM Jr, Grauch RI, Eldridge CS, and Shelton KL (1994) Cyclic variations of sulfur isotopes in Cambrian stratabound Ni-Mo-(PGE-Au) ores of southern China. Geochim Cosmochim Acta 58: 1813-1823 Pasava J (1993) Anoxic sediments- an important environment for PGE: An overview. Ore Geol Rev 8: 425-445 Steiner M, Willis E, Erdtmann BD, Zhao YL, and Yang RD (2001) Submarine-hydrothermal exhalative ore layers in black shales from South China and associated fossils- insights into a Lower Cambrian facies and bio-evolution. Palaeogeo Palaeoclim Palaeoeco 169: 165-191 Close Close Chapter 7-13 7-13 Chemical and mineralogical characteristics of tourmaline in pegmatites from Vavdos, Chalkidiki peninsula, N Greece M.D. Laskou Department of Geology and Geoenvironment, Section of Mineralogy and Petrology, Athens University, Greece Abstract. Pegmatite veins crosscutting dunites and serpentinites of the ophiolitic complex of the Vavdos (Gioldaki and Loukoviti), northern Greece contain tourmalines with a wide variation in size and composition. Pegmatite veins mainly consist of quartz crystals, microcline, albite, perthitised-feldspars. The accessory minerals include mostly coarse to medium grained zoned tourmaline, and lesser amounts of sericite (only occasionally biotite). There are also trace amounts of some rare earth element minerals, such as morazite, xenotime and minerals of the bastnaesite group (epigenetic products of monazite). The pegmatite veins host also fine-grained tourmalile, which shows an orientation parallel to the schistosity of the rock. They are composed of quartz, low-T albite and K-feldspars. Hydroxy apatite, chlorite, Nb-bearing REE minerals (koragoite), garnet, zircon and talc are also present in lesser amounts. Keywords. Tourmaline, quartz, pegmatites, Chalkidiki Greece 1 Introduction Pegmatites occur in veins crosscutting dunites and serpentinites of the ophiolitic complex of Vavdos in the western part of the Chalkidiki peninsula, N. Greece (Fig. 1). The Vavdos ophiolitic complex forms an elongate faultbounded body within the Circum-Rhodope Belt. It is one of several similar complexes of Middle to Upper Jurassic age, extending in NW-SE direction, from north-east of Thessaloniki to Sithonia (Kockel et al. 1977; Musallam and Jung, 1986). It consists of dunite, websterite, olivine clinopyroxenite, gabbroic rocks and serpentinite. It also hosts a major deposit of cryptocrystalline magnesite (Dabitzias 1980). Pegmatites crosscutting the ultramafic sequence of the Vavdos ophiolite complex contain tourmaline dispersed throughout the whole tourmaline mass (Kassoli-Fournaraki 1990). The present study focuses on two particular occurrences of tourmaline within the unit. These occurrences have coarse, medium and also fine-grained tourmaline hosted in pegmatite. The description of the mineral assemblages and their composition are given. 2 Analytical methods The phase mineral analyses were carried out using SEM JEOL JSM-5600 combined with an Oxford Link ISIS Series 300 EDX (University of Athens). ZAF corrections were applied using SEMQuant™ software. Accelerating voltage and beam current were kept at 20.0 kV and 0.5 nA, respectively. 3 Mineralogical characteristics Pegmatites from the area of Vavdos (Gioldaki and Loukoviti) have a thickness ranging from 0.5 to 3m, and are characterized by a medium- to coarse-grained texture (Fig. 2). The coarse and medium grained pegmatite veins mainly consist of quartz crystals, microcline, albite, and perthitised-feldspars. The accessory minerals include coarse-grained, medium to fine-grained and the mostly zoned tourmaline, plus small quantities of sericite and rarely biotite. Lesser amounts of rare earth element minerals are also present (morazite, xenotime and minerals of the bastnaesite group, which are epigenetic products of monazite). Tourmaline occurs in sub to euhedral crystals. Optical zoning in coarse-grained tourmaline is well pronounced, with core color ranging from greenish-blue to brown, while rims range from green brown to olive- Close 770 M.D. Laskou Hydroxyapatite, chlorite, Nb-bearing REE minerals (koragoite), garnet, zircon and talc are present in lesser amounts. Tourmaline is visible in hand specimens and in thin section, and is identified as green grains with fine brown rims. The fine-grained tourmaline associated with quartz and microcline occurs along shear zones within the host pegmatite, which seem to have formed by re-crystallization during a subsequent event 4 Mineral chemistry Tourmalines from the area of Vavdos show wide compositional variation, in particular in the SiO 2 (33.9438.93wt%), Al2O3 (34.55-39.92wt%), FeO (3.78-12.29wt%), TiO2 (0.00-3.33wt%), NaO (0.00-1.51wt%), MgO (0.006.14wt%) and MnO (0.00-1.8wt%). The range of the FeO/(FeO+MgO+MnO) and Fe/ (Fe+Mg) ratios are generally comparable to those given in granitic systems (Deer et al. 1986). The majority of tourmaline cores fall in the schorl field. Tourmaline rims are depleted in FeO and enriched in Al203 in Table 2 only. All tourmaline cores data are plotted in two areas: the field 2 [Li-poor granitoids and their associated pegmatites and aplites] and the field 3 [Fe3+-rich quartz-tourmaline rocks (hydrothermally altered granites)] (Fig. 5). green. Tourmaline of medium size exhibits green-pale cores and olive-green rims. The textural association of tourmaline and quartz (Fig. 2) indicate that these two minerals are genetically related. Fine grained tourmalines in pegmatite veins occur in crystals with a wide range in grain size, from 250-500 µm to 1000-1500 µm. (Fig. 3). These pegmatites are composed of quartz, low-T albite, K-feldspars and tourmaline. 5 Concluding remarks Although much more research is required to establish the origin of the Vavdos tourmalines, their textural, mineralogical and chemical characteristics suggest a multistage genesis. Changes in the chemical composition of tourmalines and associated minerals are probably the result of epigenetic processes. Close Chapter 7-13 · Chemical and mineralogical characteristics of tourmaline in pegmatites from Vavdos, Chalkidiki peninsula, N Greece 771 Close 772 M.D. Laskou References Dabitzias S (1980) Petrology and genesis of the Vavdos cryptocrystalline magnesite deposits, Chalkidiki Peninsula, Northern Greece. Econ Geol 75:1138-1151 Deer WA, Howie RA, Zussman J (1986) Rock-forming minerals: volum 1B, Disilicates and ring silicates: London, Longman Scientific and Technical, 629p Henry DJ, Guidotti CV (1985) Tourmaline as a petrogenetic indicator mineral: an example from the staurolite-grade metapelites of NW Maine. Am. Mineral. 70, 1-15. Kassoli-Fournaraki A (1990) Chemical varuations in tourmalines from pegmatite occurrences in Chalkidiki Peninsula, Northern Greece. Scheiz Mineral Petrogr Mitt 70: 55-65 Kockel F, Mollat H, Walther HW (1977) Erlauterung zur geologischen Karte der Chalkidiki und angrenzender Gibiete 1:100000, Nordgriechenland. 119 S, Hanover Mussalam K, Jung D (1986) Petrology and geotectonic significance of salic rocks preceding ophiolites in the eastern Vardar Zone, Greece. Tscher Min Petr Mitt 35:217-242 Close Chapter 7-14 7-14 Geochemical characteristics of He-Ar and Pb isotopes in the Dajiangping pyrite deposit, western Guangdong, South China Kuang Li, Kai Hu, Shaoyong Jiang, Shiming Song State Key Laboratory for Mineral Deposits Research, Department of Earth Sciences, Nanjing University, Nanjing, 210093, China Abstract. He-Ar isotopes were measured from fluid inclusions in six samples of the Dajiangping pyrite orebody III and orebody IV., The 3 He/4He values range from 0.13 to 2.55Ra, and the 40Ar/36Ar values range from 348 to 443. These data indicate that mantle-derived fluids contributed to the ore-forming fluids. This study suggests that the hot fluids from the deep mantle intruded into the ore body along a thrust fault, and hydrothermed the orebody. This caused differentiation of the orebody resulting in the formation of the banded orebody III and the massive orebody IV. Pb isotopes from the ore and wall rocks were also measured in this study. 206Pb/204Pb values range from 18.075 to 18.292, 207Pb/204Pb values range from 15.654 to 15.737, and 208Pb/204Pb values range from 38.401 to 38.781. These ratios indicate that orebody III is very similar to the wall rock, whereas orebody IV has lower Pb/Pb ratios than wall rock. The data support the interpretation that mantle fluid intruded into the entrapping Pre-Sinian basement migmatite, causing lower Pb isotope ratios in orebody IV. Keywords. He-Ar isotope, Pb isotope, Crust fluid, Mantle fluid, Thrust fault 1 Introduction The Dajiangping pyrite deposit lies in the northeastern part of the of Yunkai ridge, south China. It is a unique ultra-large pyrite deposit in the south of Sinian (period) layer (Chen and Chen 1998). The ore genesis model for the Dajiangping deposit has long been in dispute, and the major debate focuses on whether the orebodies formed during hydrothermal sedimentation reform, by a vapourliquid superimposition event (Zhang et al. 1992, 1993, 1994), or whether formation was the product of hydrothemal sedimentation (Chang and Chang 1998). Noble gases, especially helium and argon have distinct isotopic compositions in the crust and mantle. Due to this characteristic, He and Ar isotopes have been widely applied in tracing the origins and water-rock interactions of contemporary crustal fluids. Recently, these isotope systematics have also been successfully applied to the study of the origin of ancient ore-forming fluids and mineralization (Turner and Stuart 1992; Turner et al 1993; Burnard et al. 1994; Hu 1997; Zhao et al. 2002; Sun and Wang 2003; Zheng et al. 2003). In this note, we report He and Ar isotopic data for the Dajiangping ore deposit first time, and discuss the origin and evolution of the hydrothermal fluid. 2 Sampling and analytical methods He and Ar isotope were measured in fluid inclusions from six pyrites in the Dajiangping Deposit. These samples were collected from orebody III, orebody IV, CK36 core and wall rock. The samples were dispersed to 0.1~0.2mm grain size, through dressing by both magnetic separation and heavy-liquid separation, then the pyrites were selected by stereomicroscope. The He and Ar isotope compositions were analyzed in the Open Laboratory for Isotope Geology at the Institute of Mineral Deposits at the Chinese Academy of Geological Sciences. All samples were cleaned for 20 min in ultra-sonic bath using acetone and then dried. The samples were heated under vacuum at 120oC for 24 h to remove absorbed atmospheric gases. They were crushed to extract inclusion-trapped noble gases. The released gases were purified four times through two titanium sponge pumps, a Zr-Al pump and an active-carbon cooling trap filled with liquid nitrogen. Active gases were frozen and completely absorbed. Then comparatively pure He and Ne were introduced into the analyzing system. He and Ne were purified further to remove traces of impure gases such as H2. and Ar using a titanium sublimation pump filled with liquid nitrogen. He isotopes were analyzed by mass spectrometer. Finally Ar was released at -78oC and Ar isotopes were then analyzed. The instrument used in this study is an MI 120l IG noble gas mass spectrometer. The 3He values were measured by an electronic multiplier detector. 4He was measured by a Faraday cup. The resolutions are 1200 for the electronic multiplier detector, and 760 for the Faraday cup. The standard gas air is atmospheric air with a 3He/4He ratio of l.4x10-6. 3 He-Ar isotope analysis and discussion The results of helium and argon isotope data are given in table 1. As shown in table 1, the fluid inclusions from pyrite have 3He/4He ratios of 0.18~3.55x10-6(0.13~2.55Ra). The values of 40Ar/36Ar ratios show slight variation between 348~443, which is higher than Air-saturated water’s 40 Ar/36Ar ratios of 295.5. Close 774 Kuang Li · Kai Hu · Shaoyong Jiang · Shiming Song Three possible noble gas sources exist in hydrothermal fluids (Burnard et al. 1999): (1)Air-saturated water (ASW), including meteoric water and seawater. This is characterized by atmospheric He and Ar isotopic compositions, i.e. 3He/4He=1.4 × 10–6 = 1Ra, 40Ar/36Ar=295.5. (2) Radiogenic He and Ar accumulated in the crust. In this source, the 3He/4He ratio varies from 0.01 to 0.05 Ra, and the 40Ar/36Ar ratio usually higher than 295.5. (3) Mantle-derived volatiles. These are characterized by high 3 He with a well-defined 3He/4He ratio of 6–9 Ra. The 40Ar/ 36Ar ratio varies widely, and are usually higher than 400. By comparing the isotopic composition of the sample to the isotopic compositions of the three possible sources of noble gases, we can determine the origin of the noble gases in hydrothermal fluids. As shown in the plot of 3He/4He vs. 40Ar/36Ar ratios (Fig. 1), the data fall among three sources district, which indicates that the hydrothermal fluid did not originate from the single source, and instead may be a product of crust-mantle mixture. There are two orebody IV samples, two orebody IV samples, one CK36 drill core sample (depth 133 m), and one wall sample of all the six samples. We find that the ore-forming fluids of orebody IV fall in between mantle-derived fluids and ASW. In contrast, the others lie lower on the graph; the CK-36 and DP-11 even lie between ASW and crust fluids. We can make use of the 3He/4He ratios to Figure out the mantle fluids (Rm) ratio and the crustal fluids (Rc) ratio of the ore-forming fluids. By following formula[13], we can Figure out the helium from mantle fluids: Helium from mantle fluids = [(R–Rc)/(Rm–Rc)] (1) The Rm, Rc and R represent the 3He/4He ratios of mantle fluids, crust fluids and the samples. Rm=6~9 Ra, Rc=0.01~0.05 Ra. According to formula (1), the six samples’ helium content from mantle fluids declines from orebody IV, orebody to wall rock, indicating that the degree of mantle fluids participating in the ore-forming processes was decreasing. The reason for this may be that the ore deposit’s formation passed through a few different stages. Zhu and Meng (1999) found that the Dajiangping pyrite deposit was located on the thrust slip fault of a nappe structure in the western Guangdong. The deposit was controlled by both a large overturned fold; which has an axial plane to the southeast; and a secondary rotational fault. We can find out the tectonic characteristics from Figure 2. It is conjectured that after the orebodies underwent the hydrothemal sedimentaion event, thrust faults formed by intensive crustal tectonic movement, which pushed the Sinian layer onto limestone of Devonian and Carboniferous. Then mantle fluids rose with the intensive tectonic movement. Finally the hydrotherm from deep mantle fluids entered into, and transformed the orebodies along the fault. Therefore, the characteristics of noble gas isotope signature changed systematically during formation, as shown in Figure 1. At the same time the hydrotherm transformed the shape of orebodies, and caused differentiation resulting in the formation of the banded pyrite ore (orebody III) and the massive pyrite ore (orebody IV). Close Chapter 7-14 · Geochemical characteristics of He-Ar and Pb isotopes in the Dajiangping pyrite deposit, western Guangdong, South China 4 775 Pb isotope geochemical characteristics Lead isotopes are a powerful tool to trace the origin of metal deposits. We also measured lead isotope of 11 samples including orebody III, orebody IV, and wall rock. The data in Figure 3 also incorporate Pb isotope data of Yunkai ridge area magmatic rock and basement migmatite in Pre-Sinian period, as well as other Pb isotope data from pyrites. The lead isotope data from the pyrites differs from the lead isotope data from the magmatic rocks. This indicates that the ore deposit must not be the product of igneous magmatism. It also shows that the lead isotope compositions of minerals and wall rocks are mainly consistent. Although the lead isotope compositions of the two ore types partially overlap, the massive orebody has lower Pb isotopic values than the banded orebody. It is possible that the lead from mantle fluid had been added to the orebody. Therefore, the Pb isotope characteristics of the Dajiangping pyrite deposit strengthen our conclusion that the orebody IV was formed by late mantle fluid, which migrated along a thrust fault and altered the original shape of the orebody. ment rocks, and eventually formed the mixing hydrotherm. Then, the fluid burst out of sea floor from growth faults and formed stratiform deposits in the reducing environment. The formation of the thrust fault was initiated by teconic movement at the spot of ore deposits. Later, the deep mantle hydrotherm entered into, and reformed the orebodies. Though no new element was added in, the hydrotherm changed the orebody shape and differentiated the deposit into two distinct members: the banded orebody III and the massive orebody IV. Acknowledgements This work was supported by the Youth Excellent-Group Program No.40221301 and No.40172035 in the National Science Foundation of China. References 5 Conclusions The ore-forming fluid of pyrites in Dajiangping orebodies mainly consists of air-saturated water (seawater), which leached lithospheric ore-forming material. The original R/Ra ratio of Helium Isotope was less than 1, but after the deposit was altered by the late mantle fluid, the R/Ra ratio rose by about 50 points. We conclude that in the Sinian layer, the air-saturated water (seawater) was cyclically heated in the growth faults, absorbed by the ore-forming matter of the crustal base- Burnard PG, Hu RZ, Turner G (1999) Mantle, crustal and atmosphere noble gases in Ailaoshan, yun-nan Province, China. Geochimica et Cosmochimica Acta, 63,pp. 1595-1604 Burnard PG, Stuart F, Turner G (1994) C-He-Ar variations with in a dunite nodule as a function of fluid inclusion morphology. Earth Planet Sci.Lett,128: 243-258 Chen D, Chen Q (1998) Characteristics of the hydrothermal sedimentation of the Dajiangping super-large pyrite deposit in Yunfu, Guangdong. Geochimica 27: 12-19 Chen DF (1998) Pb and Nd Isotopes of the dajiangping Pyrite deposit, Guangdong Province, and its metallic ore source. Mineral deposits: 215-222 Close 776 Kuang Li · Kai Hu · Shaoyong Jiang · Shiming Song Hu R (1997) Geochemistry of He, Ar isotopes in ore forming fluids. Bulletin of Mineralogy, Petrology and Geochemistry 16: 120-124 Li X, Mao J (2004) Helium and Argon Isotope Systematics in Fluid Inclusion of the Gold Deposits along the Daduhe River, Sichuan Province, Southwestern China. Acta Geologica Sinica 78: 203-210 Sun X, Wang M (2003) He-Ar isotopic systematics of fluid inclusions in pyrites from PGE-polymetallic deposits in lower Cambrian black rock series, southern China. Geological Journal of China Universities 9: 661-666 Turner G, Burnard PB, Ford JL (1993) Tracing fluid sources and interaction. Phil Trans R Soc Lond A 344: 127-140 Turner G, Stuart F (1992) Helium/heatratios and deposition temperatures of sulfides from the ocean floor. Nature 357: 581~583 Zeng Z, Qin YS (2003) He, Ne and Ar isotope compositions of fluid inclusions in massive sulfides from the Jade hydrothermal field, Okinawa Trough. Acta Oceanolog 25: 36-42 Zhang B, Zhang Q, Pan J (1994) Trace element characteristics and their geological significance of Dajiangping pyrite deposit, western Guangdong. Geology and Prospecting 30: 66-71 Zhang Q, Zhang B, Cao Y (1993) Preliminary discussion on sulfur and lead isotope compositions of the Dajiangping pyrite deposit in western Guangdong province. Acta Geologica Sinica, 67(3), pp. 232-242 Zhang Q, Zhang B, Pan J (1992) Silicalite characteristics and rareearth element model of Dajiangping pyrite deposit in western Guangdong province. Chinese Science Bulletin 37: 1588-1592 Zhao K, Jiang S, Xiao H (2002) Origin of ore-forming fluids of the Dachang Sn-polymetallic ore deposit: Evidence from helium isotopes. Chinese Science Bulletin 47: 1041-1045 Zu D, Meng X (1999) Primary study on the western Guangdong nappe structure in the hercynian and indo-Chinese epoch. Journal of geomechanics 5: 51-58 Close Chapter 7-15 7-15 Precise Re-Os dating of molybdenite from the east Qinling molybdenum belt in central China and its geodynamic implications Yong-Feng Li, Jing-Wen Mao, Feng-Jun Bai, Bao-Jian Guo Faculty of Geosciences and Resources, China University of Geosciences, Beijing 100083, China Zhi-Guang Wang Bureau of Geology and Mineral Resources for Nonferrous Metals, Henan Province, 107 Zhongyuandong Road, Zhengzhou 450052, Henan, China Abstract. Located in central China on the southern margin of the North China craton, the East Qinling molybdenum belt is one of the important large molybdenum belts in China. This study provides reliable Re-Os isotopic dating results for the metallogenetic epoch of four deposits by inductively coupled plasma mass spectrometry (ICP-MS), with analytical errors of Re and Os between 0.110.4% (2sigma). The results show that the Re-Os model ages are 141.8±2.1Ma for the Nannihu deposit, 145.4 ±2.0 to 144.5 ±2.2 Ma (averaging 145.0 ±2.2 Ma) for the Sandaozhuang deposit, 145.8±2.1 to 143.8±2.1 Ma (averaging 144.8 ±2.1 Ma) for the Shangfanggou deposit, and 133.1±1.9 to 131.6±2.0 Ma (averaging 132.4±2.0 Ma) for the Leimengou deposit. According to these ages, combined with the results of previous work in the molybdenum belt, it is suggested that the age of the molybdenite deposits in the East Qinling molybdenum belt is mainly ~140 Ma. These deposits are the product of transformation from the N-S to the nearly E-W tectonic regime in eastern China. Except for the Huanglongpu Mo deposit, which originated at ~220 Ma, the deposits appear to have geodynamically formed in the extensional stage of the post-collisional orogeny between the North China craton and the Yangtze craton. Keywords. Mo deposit, Re-Os dating, geodynamics, East Qinling, China 1 phyry Mo (Fe) deposit and Leimengou porphyry Mo deposit. These results, combined with the results of previous work in the Mo belt, provide further insight into the geodynamic setting for the formation of these ore deposits. 2 Geological setting Located on the southern margin of the North China craton, The East Qinling belt is used to be a part of the North China craton (Fig. 1). Recently, it has also been described as a component part of the northern margin of the Qinling orogen because of its involvement in the Qinling intracontinental orogenic movement during the MesoCenozoic, accompanied by intense magmatic activities dominated by acid magma (Jurassic to Cretaceous), as the Wuzhangshan batholith, the Haoping, Heyu and Huashan batholiths. Concomitantly with the intrusion of the above-mentioned large granite bodies, a number of small, hypabyssal to near-surface granite porphyries (such lntroduction The East Qinling molybdenum belt contains the most important large molybdenum deposits in China. This belt is the second largest molybdenum belt in the world subsequent to the Climax-Henderson porphyry molybdenum belt. The molybdenum deposits occur along a tectonic lineament of trending nearly east-west. They are mostly concentrated in a region extending from the JinduichengHuanglongpu area, south to the Shaanxi, eastward to the Nannihu area in Luanchuan County and the Leimengou area in Songxian County, western Henan. There are a total of more than 30 superlarge, large and intermediate molybdenum polymetallic ore deposits in the belt, which contribute 52 percent of the total identified Mo reserves in China (Zhang et al. 2001). Stein et al. (1997) have reported the Re-Os ages for the Jinduicheng-Huanglongpu area. This study provides the reliable Re-Os isotopic dating results for the other two clusters, including four large deposits: the Nannihu porphyry Mo (W) deposit, Sandaozhuang skarn Mo (W) deposit, Shangfanggou por- Close 778 Yong-Feng Li · Jing-Wen Mao · Feng-Jun Bai · Bao-Jian Guo · Zhi-Guang Wang as the Leimengou granite porphyry) and their genetically related cryptoexplosive breccias, were emplaced. They form a NW-trending tectonomagmtic belt in the region and provide the source of ore materials for molybdenum polymetallic mineralization. The Qinling molybdenum belt may be approximately divided into three molybdenum clusters. The first cluster is found in the JinduichengHuanglongpu area (Huang et al. 1984), and can be described as a mineralization cluster. The second cluster, is located in the Nannihu-Sandaozhuang area about 75 km ESE of the Jinduicheng-Huanglongpu area, and consists of porphyry skarn-type Mo-W mineralization,. The third cluster is located in the Leimengou area, and includes the Leimengou porphyry type Mo deposit and the Huangshuian Mo-Pb deposit, which occurs in carbonatite veins. According to the geological characteristics, ore element assemblage, ore genesis, mode of occurrence and metallogenic mechanisms of the ore deposits, the molybdenum deposits in the Qinling belt may be classified into three distinctly different groups; porphyry type, skarn-porphyry type and hydrothermal carbonate vein type. 3 Previous dating In the East Qinling molybdenum belt, there have been numerous attempts to date molybdenum mineralization. For many years the mineralization ages in this area were indirectly estimated by using the ages of mineralizationrelated granites, alteration minerals or by dating accessory minerals and nearby plutonic rocks. The development of new dating techniques, such as Re-Os dating of molybdenite, has allowed for direct dating of mineralization., In the past several years, Re-Os analyses of molybdenite from the East Qinling belt have been performed by Huang et al. (1994, 1996) and Stein et al. (1997). These data are summarized in Table 1. 4 Samples and analytical methods A total of eight ore samples were collected from the East Qinling Mo deposits for Re-Os dating in this study. One of them came from the Nannihu deposit, three from the Sandaozhuang deposit, two from the Shangfanggou deposit, and two from the Leimengou deposit. The samples were carefully identified under the binocular microscope and then molybdenite separates were picked out by hand. The separates were fresh, non-oxidized and pollution-free. Samples were sealed in tubes and dissolved, following the Carius tube digestion technique (Mao et al. 2003b). The Re and Os isotopic compositions were determined by using the ICP-MS (VG PQ-EXCELL). In this study, the average blanks for the Carius tube procedure as described above are ca.10 pg for Re and ca.1 pg for Os. Close Chapter 7-15 · Precise Re-Os dating of molybdenite from the east Qinling molybdenum belt in central China and its geodynamic implications 5 Results Common Os was not detected in the eight samples of molybdenite Table2.shows the isotopic components of the samples. The decay constant used for 187Re of 1.666×1011 -1 yr , which has an uncertainty of about ±1.02%. The results show that the Re-Os model ages are 141.8±2.1 Ma for the Nannihu deposit, 145.4 ±2.0 to 144.5 ±2.2 Ma (averaging 145.0 ±2.2 Ma) for the Sandaozhuang deposit, 145.8±2.1 to 143.8±2.1 Ma (averaging 144.8 ±2.1 Ma) for the Shangfanggou deposit, and 133.1±1.9 to 131.6±2.0 Ma (averaging 132.4±2.0 Ma) for the Leimengou deposit. 6 Metallogenic environment and geodynamical setting The North China craton had been in a stage of steady development from the Cambrian until the Early Triassic. The isotopic age data suggest the following: the Yangtze craton collided and converged with the North China craton at about 218 to 238 Ma (Li et al. 1989), This was followed by an intracontinental orogeny, which ended in the Jurassic (Chen and Fu 1992). During the late Jurassic and early Cretaceous, the regional tectonic regime in the whole of eastern China began to change. The main stress field began to shift from N-S to nearly E-W, signaling the beginning of the Pacific tectonic evolution stage (Ren 1991). During this stage the southern margin of the North China craton, including the East Qinling area, transformed into the extensional tectonic environment. The IndosinianYanshanian magmatic activity corroborates the features of the tectonic evolution in this period. First, in the Middle-Late Jurassic mafic magma rose and intruded along tenso-shear steep-dipping fractures, forming diabase dikes or dike swarms in the area. Later, widespread acid magmatic activity formed large granite batholiths and numerous granite porphyry stocks and dikes. During the Early Cretaceous, large amounts of intermediate-acid magma were erupted along the Sanmenxia-Lushan deep fault, forming volcanic basins at Tianhu of Songxian 779 County, Jiudian of Ruyang County and other areas (Wang et al. 1997). Magmatism intensified, and the magma evolved successively from the alkaline through subalkaline to calcalkaline compositions. This suggests a change in the character of the magamitic activity during that period. The fact that more than 80% of Mesozoic intrusive rocks occurred in the Early Cretaceous indicates that the transition of the tectonic regime began at the turn of the JurassicCretaceous. The Re-Os isotope model ages obtained in this study are between 145.8±2.1 and 131.6±2.0Ma. It can be concluded that the East Qinling metallogenic molybdenum belts originated during this great transition of the tectonic regime in eastern China. This time period belongs to the second phase of large-scale metallogenesis in East China during the Mesozoic (Mao et al. 2000; 2003b). Acknowledgements This study was supported by the National Natural Science Foundation of China (grant 40434011) and the State Development and Planning Program for Basic Researches in Key Areas of China (grant 1999043211). References Chen Y, Fu S (1992) Mineralization of gold deposits in Henan, China. Beijing: Seismological Press: 1-146 (in Chinese) Huang D, Du A, Wu C, Liu L, Sun Y, Zhou X, (1996) Metallochronology of Mo(-Cu) deposits in the North China plateform: Re-Os age of molybdenite and its geological significance. Mineral Deposits 15: 365-373 Huang D, Wu C, Du A, He H (1994) Re-Os isotope ages of molybdenum deposits and in East Qinling their geological significance. Mineral Deposits 13; 221-230 (in Chinese with English abstract) Li S, Hart SR, Zheng S (1989) The collision time of North China plate and South China plate: evidence from Sm-Nd ages. Scientia Sinica(B):19: 312-319 (in Chinese) Li Y, Mao J, Guo B (2004) Re-Os dating of molybdenite from the Nannihu Mo(W) orefield in the east Qinling and Its Geodynamic significance. Acta Geologica Sinica 78: 463-470 Mao J, Wang Z (2000) A preliminary study on time limits and geodynamic setting of large-scale metallogeny in East China. Mineral Deposits 19:289-296 (in Chinese with English abstract) Close 780 Yong-Feng Li · Jing-Wen Mao · Feng-Jun Bai · Bao-Jian Guo · Zhi-Guang Wang Mao J, Yang J, Qu W, Du A, Wang Z, Han C (2003b) Re-Os age of CuNi ores from the Huangshandong Cu-Ni sulfide deposit in the east Tianshan Mountains and its implication for geodynamic process. Acta Geol Sinica 77: 220-226. Mao J, Zhang Z, Yu J, Wang Y, Niu B (2003a) The geodynamics setting of Mesozoic large-scale mineralization in North China: the revelation from accurate timing of metal deposits. Science in China (series D) 33:289-299 Ren J (1991) A discussion on the basic features of the lithosphere tectonics in Chinese continents. Regional Geology of China 2: 289-293 (in Chinese with English abstract) Stein HJ, Markey RJ, Morgan JW, Du A, Sun Y (1997) Highly precise and accurate Re-Os ages for molybdenite from the east Qinling molybdenum belt, Shaannxi Province, China. Economic Geology 92:827-835 Wang Z, Cui B, Xu M (1997) The tectonic evolution and mineralization in the south margin of North China block. Beijing: Metallurgical Industry Press. pp1-296 (in Chinese) Zhang Z, Zhu B, Chang X, Qiang L, Wen M (2001) Petrogenetic metallogenetic background and time space relationship of the East Qinling molybdenum ore belt, China. Geological journal of China University 7(3):307-315(in Chinese with English abstract) Close Chapter 7-16 7-16 Studies on the genesis of adjacent Changkeng goldand Fuwang silver-deposits, Guangdong Province, China Hua-Ying Liang, Ping Xia, Xiu-Zhang Wang Laboratory of Marginal Sea Geology, Guangzhou Institute of Geochemistry and South China Sea Institute of Oceanology, Chinese Academy of Sciences, 510640 Guangzhou, China Heng-Xiang Yu Guilin Institute of Technology, Guilin 541004, China Abstract. The Changkeng Au- and Fuwang Ag-deposits represent an economically significant and distinct member of the Au–Ag deposit association in China. The two deposits are immediately adjacent, but the Au- and Ag-orebodies separated from each other. Changkeng is hosted in brecciated cherts and jasperoidal quartz and is characterized by disseminated ore minerals. Fuwang, hosted in the Lower Carboniferous Zimenqiao group bioclastic limestone, has vein and veinlet mineralization associated with alteration comprised of quartz, carbonate, sericite, and sulfides. The Changkeng gold and Fuwang silver deposits overlap in homogenous temperature and salinity of fluid inclusions. The δDH2O, δ18OH2O, δ13CCO2 and 3 He/4He values of the fluid inclusions suggest the ore fluids of the Changkeng Au-ore come from the meteoric water and the ore fluids of the Fuwang Ag-ore are derived from mixing of magmatic water and meteoric water. The Changkeng gold- and the Fuwang silver deposits show different Pb isotope signatures, suggesting different sources of ore-forming material. Rb-Sr isochron age (68 ± 6 Ma) and 40Ar-39Ar age (64.3 ± 0.1 Ma) of the ore-related quartz veins from the Ag-deposit indicate that the Fuwang deposit formed during the Cenozoic Himalayan tectono-magmatic event. The adjacent Changkeng and Fuwang deposits could, however, represent a single evolved hydrothermal system. The deposits are alternatively the product of the superposition of two different geological events. Our work indicates that the Pacific Coastal Volcanic Belt in the South China Fold Belt has greater potential for Himalayan precious metal mineralization than previous realized. gold deposit is hosted in brecciated siliceous rocks on the top of rocks of the Zimenqiao Group bioclastic limestone and is characterized by disseminated mineralization. Ore minerals in the gold deposit include disseminated anhedral pyrite, native gold, stibnite, realgar, and orpiment. Gangue minerals include quartz, illite, dickite, calcite, less fluorite, and barite (Du et al. 1993). The silver content in the gold orebodies is low (generally <11 ppm). The Fuwang silver deposit is hosted in Early Carboniferous Zimenqiao bioclastic limestone along the contact fault zones between the limestone and the overlying Changkeng gold-hosting siliceous rocks. The Fuwang silver is characterized by vein and veinlet mineralization with zones of silicification. The main sulphide minerals are sphalerite and galena, with lesser pyrite and rare arsenopyrite, chalcopyrite, and bornite. The deposit is poor in gold (< 0.2 ppm). The crosscutting relationship indicates that the gold deposit is older than the silver deposit. Keywords. Himalayan, gold, silver, Guangdong, ore genesis 1 Geological setting The adjacent Changkeng gold- and Fuwang silver-deposits are located along the southwestern rim of the Shanshui basin (Fig. 1). Sedimentary rocks in the region range from Proterozoic to Cenozoic.(Bureau of Geology and Mineral Resource of Guangdong Province 1985; Du et al. 1993). Eocene volcanic and sedimentary rocks are widespread (Tang 1987) and a small Tertiary volcanic rocks hostedsilver deposit was discovered (Fig. 1). The adjacent Changkeng gold- and Fuwang silver- deposits differ in their geologic characteristics, stratigraphic position, and metal contents, but are both located at the same locality (Fig. 1), The Changkeng gold orebodies are present in the upper part of the stratigraphic section (Du et al. 1993). The Fuwang silver orebodies are located in the lower parts of the stratigraphic section. The gold and silver ore bodies are separated from each other. The Changkeng Close 782 Hua-Ying Liang · Ping Xia · Xiu-Zhang Wang · Heng-Xiang Yu 2 Genesis of the gold-hosting siliceous rocks Genesis of the gold-hosting siliceous rocks has been debated extensively. Du et al. (1993) argues that the goldhosting siliceous rocks are jasperoid quartz formed from limestone. However, Xia et al. (1996) suggest that these rocks are syngenetic chert. Gold-hosting silicious rocks consist of thin-bedded and laminated, massive, and brecciated black material. Some radiolaria, which suggest an age of between Carboniferous and Permian, are present in some of the laminated and massive siliceous material. This suggests that some parts of the gold-hosting siliceous laminated and massive material is radiolarian chert. The limestone-siltstone contacts are common sites of deep burial diagenetic silicification. Some of the massive zones contain framboidal pyrite, and therefore may have formed by diagenetic processes as diagenetic chert. The Changkeng gold ore is hosted mainly in the breccia. Thus, the gold-bearing breccias imply that the gold was introduced after the diagenetic silicification. The gold-hosting rocks, therefore, formed by multistage silicification that at least includes syngenetic-, diagenetic-, and hydrothermal- silicification. The hydrothermal silicification is related to gold deposition. The syngenetic silicification and the diagenetic silicification have high background abundances of gold and may indicate that a pre-existing enriched of gold in the stratigraphic section contributed to the Changkeng gold deposit, similar to processes suggested for the Meikle and neighboring Carlin-type deposits of Nevada (Emsbo et al. 2003). 3 Geochemical studies of the adjacent Changkeng gold and Fuwang silver deposits 3.2 Pb Isotopes of the adjacent Changkeng gold- and Fuwang silver- deposits The adjacent Changkeng gold- and Fuwang silver- deposits show different lead isotopic signatures. The Changkeng gold deposit has Pb isotope ratios (206Pb/204Pb: 18.580-19.251, 207Pb/204Pb: 15.672-15.801, 208Pb/204Pb: 38.700-39.104) similar to those (206Pb/204Pb: 18.578-19.433, 207Pb/204Pb: 15.640-15.775, 208Pb/204Pb: 38.925-39.920) of its host rocks and different from those (206Pb/204Pb: 18.82018.891, 207Pb/204Pb: 15.848-15.914, 208Pb/204Pb: 39.57939.786) of the Fuwang silver deposit. The Pb in the gold deposit is derived from the local sources. The Pb isotope composition of the Fuwang silver deposit is similar to those of the Neoproterozoic metamorphic basement of the western Guangdong region (Zhang et al. 1993), suggesting that the Pb of the Fuwang silver deposit is derived from the Neoproterozoic metamorphic basement. 3.3 40Ar/39Ar age and Rb-Sr isochron age of mineralized quartz veins The mineralized quartz sample from the Fuwang silver deposit yields 40Ar/39Ar a plateau age of 64.3 ± 0.1 Ma and isochron age of 64.0 ± 0.1 Ma with an initial 40Ar/36 ratio of 294.5 ± 0.4. The Rb and Sr isotopic data obtained from six samples define an Rb-Sr isochron, with an age of 68 ± 6 Ma, MSWD = 4.14. Quartz 40Ar/39Ar age s and Rb-Sr isochron age are concordant within error, and correspond to the Himalayan tectono-magmatic event (Himalayan is a period <90 Ma; Wang and Mo 1995). 4 Origin of Changkeng gold and Fuwang silver deposits 3.1 Geochemistry of the ore-forming fluid The gold and silver deposits overlap in homogenization temperature, in the ranging 210 ± 80 °C and 230 ± 50 °C, respectively. Salinities of the fluid inclusion from the gold and silver deposits are also overlap, ranging from 1.6 - 7.3 wt % and 1.6 - 2.6 wt % equiv. NaCl, respectively. The adjacent Changkeng gold- and Fuwang silver- deposits are different in δDH2O, δ18OH2O, δ13CCO2 and 3He/4He isotope composition (Guo et al. 1996; Sun et al. 1999). The δDH2O, δ18OH2O, δ13CCO2 and 3He/4He values of the fluid inclusions from the Changkeng gold deposit range from –80 to -30 ‰, -7.8 to –3.0 ‰, -16.6 to -17.0 ‰ and 0.0100 to 0.0054 Ra, respectively. The δDH2O, δ18OH2O, δ13C CO2 and 3He/4He values of fluid inclusions from the Fuwang silver deposit range from –59 to -45 ‰, -0.9 to 4.1 ‰, -6.7 to –0.6 ‰ and 0.5930 to 0.8357 Ra, respectively. The δDH2O, δ18OH2O, δ13CCO2 and 3He/4He values of the fluid inclusions suggest the ore fluids of the Changkeng gold ore come from the meteoric water and the ore fluids of the Fuwang silver ore come from mixing of magmatic water and meteoric water. The Changkeng gold deposit is hosted in siliceous rocks and limestone and shows similar mineralization and mineral associations to many Carlin-type deposits (Hofstra and Cline 2000; Hu et al. 2002; Peters et al. 2002). Age evidence suggests that the Fuwang silver deposit bear a genetic relation to the Himalayan magmatic event in the Shanshui Basin. Given the close temporal and broad spatial association of the silver deposit with Early Tertiary magmatism, the D, O, C, and He isotope data are consistent with ore fluids that consisted of a mixture of deeply sourced magmatic and local meteoric water. The most plausible explanation is to ascribe these combined mineralized ages and isotopic results for the Fuwang silver deposit to the Himalayan tectono-magmatic event. The presence of disseminated gold in brecciated siliceous rocks along with epigenetic quartz, orpiment, realgar, and stibnite, together with meteoric D, O, C, and He isotopic values and fluid inclusion salinity and temperature data that overlap those from Fuwang silver deposit, suggests that the gold was deposited by an epigenetic meteoric hydrothermal system. Close Chapter 7-16 · Studies on the genesis of adjacent Changkeng gold- and Fuwang silver-deposits, Guangdong Province, China The adjacent Changkeng gold- and Fuwang silver-deposits could represent a single evolved hydrothermal system where the ore fluids deposited gold at first in the brecciated silicification, and then mixed with the magmatic water and deposited silver in the fracture zone in the limestone. Alternatively, the second ore genetic model is that the adjacent Changkeng gold- and Fuwang silver-deposits may have resulted from the superposition of different geological events. Given the close proximity of the two deposits and the overlap of fluid inclusions salinities and temperatures, the adjacent Changkeng gold and Fuwang silver deposits were most likely formed by the first model. Early Tertiary isotopic ages from the Fuwang silver deposit and the nearby Xiqiaoshan Tertiary volcanic rockhosted silver deposit suggest that the South China Fold Belt underwent a Himalayan event of precious metal mineralization. Acknowledgements The work was supported by the the NSFC (No.49872035, 40472049), and the important project of CAS (No. KZCXZSW-117 and No. GIGCX-03-04). References Bureau of Geology and Mineral Resource of Guangdong province (1985) Regional geology of Guangdong province. Geol Pub House, Beijing, China, 1-350 (in Chinese) Du JE, Ma CH, Zhang GH (1993) Mineralization characteristics of the Changkeng gold-silver deposit, Guangdong province. Guangdong Geology 8: 1-8. (in Chinese with English abstract) 783 Emsbo P, Hofstra AH, Lauha EA, Griffin GL, Hutchinson RW (2003) Origin of high-grade gold ore, source of ore fluid components, and genesis of the Meikle and Neighboring Carlin-type deposits, Northern Carlin trend, Nevada, Econ Geol 98: 1069-1105 Guo XS, Du JE (1996) Study on the fluid inclusions and geochemistry of the Changkeng Gold-Silver deposit. Min Res Geol 10: 187193. (in Chinese with English abstract) Hofstra A H, Cline JS (2000) Characteristics and models for Carlintype gold deposits, Rev Econ Geol 13: 163-220. Hu RZ, Su WC, Bi XW, Tu GZ, Hofstra AH (2002) Geology and geochemistry of Carlin-type gold deposits in China. Miner Depos 37: 378-392 Peters SG, Huang JZ, Jing CG (2002) Introduction to and classification of sedimentary rock-hosted Gold deposits in P.R. China. In: Peters S.G. (ed), Geology, geochemistry, and geophysics of sedimentary rock-hosted gold deposits in P. R. China. Open-File Rep 02-131, versi 1.0: 1-60 Sun XM, Norman DI, Sun K, Chen BH (1999) Characteristics and source of ore-forming fluids of Changkeng Gold-Silver deposits in middle Guangdong province, evidences from N2-Ar-He. Scie China (Series D) 29: 240-246 (in Chinese) Tu GZ (2000) The super-large deposits in China. Vol. 1. Scie China Press, Beijing, pp. 3-9 (in Chinese) Wang HZ, Mo XX (1995) An outline of the tectonic evolution of China. Episodes 8: 6-16 Xia P, Zhang H, Wang XZ, Chen JP (1996) Geology-geochemistry and genesis of chert from Changkeng Au-Ag deposit, west Guangdong province, China. Geochemica 25: 129-139 (In Chinese with English abstract) Zhang Q, Zhang BG, Pang JY, Cao YB, Hong DH (1993) The isotope signature and source rocks of Chadong Silver-Gold deposit. Mineral Deposits 12: 349-355 (in Chinese with English abstract) Zhang WH, Lu WJ, Jiao YQ, Li ST (2000) Composition and source study of ore-forming fluid in the Changkeng gold-silver deposits, Guangdong province, China. Acta Petrol Sinica 16: 521-527 (in Chinese with English abstract) Close Close Chapter 7-17 7-17 Fluid inclusion and stable isotope geochemistry of the Ernest Henry Fe oxide-Cu-Au deposit, Queensland, Australia Geordie Mark1, Patrick J. Williams, Nick H.S. Oliver School of Earth Sciences, James Cook University, Townsville 4811, Australia 1 Current address: School of Geosciences, Monash University, Melbourne 3168, Australia Chris Ryan CSIRO Exploration and Mining, School of Geosciences, Monash University, Melbourne 3168, Australia Terry Mernagh Geoscience Australia, GPO Box 378, Canberra 2601, Australia Abstract. Ernest Henry is an iron oxide-copper-gold deposit characterized by magnetite>>hematite, chalcopyrite as the only significant hypogene copper mineral. It occurs within a large, zoned, medium to high temperature alteration system. Pre- to synmineralization quartz contains three broad populations of fluid inclusions. Type 1 (L-VH±nS) inclusions decrepitate or homogenise at 200-500° C, have salinities of 32-55 wt% NaClequiv, display chemical variations that parallel the paragenetic sequence of alteration, and have variable Br/Cl mostly less than magmatic brines. Type 2 (L-V) inclusions homogenise at temperatures of 120-350°C have salinities up to 20 wt% NaClequiv and inferred to contain CaCl2. Type 3 L-rich CO2 inclusions were entrapped at 130-370MPa. dD and dO of pre- to synmineralisation fluids are estimated to have been -23 to -66 and 8 to 11 per mil respectively. dS in main ore pyrite and chalcopyrite is -1.6 to +5.4 per mil. The data are compatible with a substantial magmatic contribution to Ernest Henry fluids but also suggest the system was complex and involved fluids and other components with different sources. Ernest Henry is distinguished from the giant Olympic Dam deposit by evidence for high temperature/salinity fluids and for no major involvement of surficial waters during mineralization. Keywords. Ernest Henry, copper, gold, fluid inclusions, stable isotopes 1 Introduction The sources of ore fluids and mechanisms of mineralization in iron oxide-copper-gold (IOCG) deposits are poorlyunderstood and could differ amongst the geologically diverse members of the group (e.g. Barton and Johnson 2004). Ernest Henry is the largest known magnetite-dominated IOCG deposit in Australia (Mark et al., in press; cf. Williams and Pollard 2003). In contrast to the giant hematite-rich Olympic Dam deposit in South Australia, it is characterized by complex high temperature alteration zoning and has chalcopyrite as the only significant copper mineral (Mark et al. in press; cf. Reeve et al. 1990). This paper reports on fluid inclusion and stable isotope studies that were undertaken to characterize Ernest Henry ore fluids. It is the first fluid inclusion study to have been attempted at the deposit where such work is challenging because of the low abundance of quartz compared to most other hydrothermal deposits and a general tendency for fluid inclusions to be small and difficult to work with. New stable isotope data augment earlier work by Twyerould (1997) and include the first reported δD data for the deposit. 2 Geological context Ernest Henry is the largest of several magnetite bearing IOCG deposits in the Cloncurry mining district, which encompasses the eastern part of the Proterozoic Mount Isa inlier in northwest Queensland, along with its extensions beneath shallow cover in the surrounding area (Williams and Pollard 2003). Late Palaeoproterozoic supracrustal rocks and early ca 1.74 and 1.66 Ga intrusions were deformed and metamorphosed at greenschist to amphibolite facies between 1.58 and 1.50 Ga and extensively intruded by granitoids from 1.55 to around 1.50 Ga (Page and Sun, 1998; Williams and Pollard, 2003). The Ernest Henry deposit is hosted in a sequence of metamorphosed, predominantly intermediate volcanic rocks and is spatially-associated with bodies of ca 1.66 Ga diorite. U-Pb dating of titanite from pre-ore alteration assemblages suggests that the Ernest Henry hydrothermal system was broadly contemporaneous with the later (1.551.50) granitoids, examples of which are present within 15 km of the ore deposit (Mark et al. in press). Proterozoic basement near Ernest Henry is obscured by Mesozoic to recent cover. However, extensive drilling around the deposit has demonstrated there is a very large volume of altered rocks that extends for at least several kilometres in all directions near the current erosion level (Mark et al. in press). 3 Paragenesis of alteration and mineralization Twyerould (1997) and Mark et al. (in press) documented the time-space evolution of the Ernest Henry hydrothermal system. Distal stage 1 alteration produced secondary albitic plagioclase and calc-silicates and was similar to regional-scale sodic-calcic metasomatism elsewhere in the Close 786 Geordie Mark · Patrick J. Williams · Nick H.S. Oliver · Chris Ryan · Terry Mernagh district (De Jong and Williams 1994). It is preserved with variable overprints by younger alteration at distances of 1-3 km from the orebody. Stage 2 formed a potassic-iron(manganese) association represented predominantly by biotite, magnetite, K feldspar, almandine-spessartine garnet and quartz rich veins. Stage 2 alteration is preserved around the periphery of the mine and along NE-trending structures extending away from it. Stage 3 potassic alteration was pervasive in the immediate vicinity of the orebody where the rocks were replaced by hematitestained and variably barian K-feldspar. Stage 3 altered rocks were selectively affected by Stage 4 which formed a SE-plunging breccia lens up to 300m thick in which magnetite, sulphides and a very complex association of other minerals form the matrix to K-feldspar-dominated clasts. Stage 5 calcite-dominated veins are predominantly localized near the footwall contact of the ore lens. 4 Sampling and methods Samples were obtained from drill cores where the geological context and paragenetic setting was well known from detailed logging undertaken as part of general geological description of the deposit and the surrounding altered rocks (Mark et al. in press). The fluid inclusion study focussed on interpreted primary inclusions hosted by quartz from paragenetic stages 2, 3 and 4 (i.e. pre- to synmineralization). The inclusions were investigated by conventional and electron microscopy, subjected to microthermometric experiments, and selected examples were analyzed by Laser Raman spectrometry and proton induced X-ray excitation (PIXE) analysis (cf. Ryan et al. 2001). Hand-picked separates were prepared of minerals from stages 1-5 and analyzed using conventional methods as appropriate for δD in biotite and amphibole (n=10, SUERRC, East Kilbride, Scotland), δ13C and δ18O in carbonates (n=36, Monash University), δ18O in silicates and magnetite (n=42, Monash University) and δ 34 S in sulphides (n= 32, University of Tasmania). 5 Fluid inclusion types and geochemistry Quartz-hosted fluid inclusions from stages 2 to 4 can be classified into three broad groups (Fig. 1). Type 1 (L-VH±nS) inclusions contain liquid, a small H2O vapour bubble (<10% of total volume) and a halite solid at room temperature. Most have additional solids in a variety of assemblages containing one or more of ferropyrosmalite, sylvite, Fe-chloride, magnetite, hematite, calcite and kutnahorite (CaMn(CO3)2). Brown ice forms on freezing and low first melting temperatures indicate the presence of Ca and other divalent metals. A small proportion of Type 1 inclusions decrepitate without homogenising on heating while the remainder homogenise by halite or ferropyrosmalite dissolution at temperatures between 200 and 520°C (65% > 300°C). Salinities estimated from halite dissolution temperatures are 32-55 wt% NaClequiv. Type 2 (L-V) inclusions occur in both primary and secondary Close Chapter 7-17 · Fluid inclusion and stable isotope geochemistry of the Ernest Henry Fe oxide-Cu-Au deposit, Queensland, Australia settings (i.e. some of them represent the youngest fluid type). At room temperature they contain liquid and an H2O vapour bubble which occupies up to 25% of the volume of the inclusion. They homogenise at temperatures of 120-350°C. Type 2 inclusions form brown ice on freezing and are deduced to be CaCl2-bearing. Salinities range up to 20 wt% NaClequiv. Type 3 inclusions are dominated by CO2 and are liquid-rich (>90%) at room temperature. Some contain a small proportion of liquid H2O and/or a nahcolite (NaHCO3) solid. Their densities suggest entrapment at pressures of 130-370 MPa during stages 2 to 4. PIXE studies were undertaken on populations of single fluid inclusions from stages 2, 3 and 4 (total analyses = 40). The results are quantitative at an accuracy of around ±50% for Cl, K, Ca, Mn, Fe, Cu, Zn, As, Br, Rb, Sr, Ba and Pb. Accuracy for many interelement ratios is far better than this as the main sources of error have similar effects on all elements. Analytical detection limits were mostly in the range 30-300 ppm. Type 1 inclusions display systematic stage to stage variation. All are distinguished by high Mn:Fe ratios (mostly > 1) compared to complex brine inclusions from other Cloncurry Fe oxide Cu-Au deposits such as Osborne, Starra and Eloise (Williams et al. 1999; 2001). Stage 3 (K feldspar-related) Type 1 inclusions have lower (Mn+Fe)/K than those from stages 2 and 4 (magnetite/biotite/garnet-related). With the exception of one outlying result, Br/Cl ratios in Type 1 inclusions are less than 0.0013 and in some cases in which Br was undetected must be less than 0.0005. Cu was only detected in Type 1 inclusions at concentrations of 30-200ppm. Analyses of the eight analyzed ore stage Type 1 inclusions have previously been reported by Mark et al. (2005). These are distinguished by the highest K/Ca ratios and absolute concentrations of Ba (mean 2.8 wt%), Zn (mean 4800 ppm), As (mean 590 ppm), and Pb (mean 2300 ppm) but all had estimated Cu below 120 ppm. 6 Stable isotope results δD values are -80 to -88 per mil in three stage 1 amphiboles, -85 and -91 per mil in two stage 2 biotites, - 69 to -95 in four stage 4 biotites, and -72 in a stage 5 amphibole. Allowing for the likely fractionations this suggests that the fluids in the Ernest Henry system had δD of -23 to 66 per mil Mean δ18O values (per mil) are: Stage 1, amphibole = 5.8, calcite = 15.7; Stage 2, biotite = 6.4, calcite = 12.5, K feldspar = 11.3, magnetite = 4.6, quartz = 10.7; Stage 3, biotite = 5.7, calcite = 12.5, K feldspar = 9.0, magnetite = quartz = 11.8; Stage 4, biotite = 6.2, calcite = 12.6, K feldspar = 10.1, magnetite = 3.1, quartz = 11.7; Stage 5, amphibole = 10.5, calcite = 14.9. In conjunction with data from Twyerould (1997) these results suggest that fluid δ18O remained in the range 8-11 per mil in the time period represented by stages 1-4. The data for carbonate-rich stage 5 are consistent with an influence from metamorphosed 787 carbonates either involving an external fluid with higher δ18O of 13-16 per mil that had equilibrated with such rocks or from their presence in the protoliths of the highly deformed rocks in the footwall of the deposit where the carbonate veining is localized. Mean δ13C values (per mil) in calcite are; Stage 1, -2.4; Stage 2, -4.2; Stage 3, -3.5; Stage 4 -3.0; Stage 5, -2.1. 34S ranged from - 0.5 to +5.4 per mil (mean 2.2) in ore stage chalcopyrite and from -1.6 to +4.8 (mean 1.6) in ore stage pyrite. The two common sulphide minerals are not preserved in isotopic equilibrium. 7 Discussion The pre- to synmineralization (Stages 2-4) mineral parageneses at Ernest Henry that distinguish the system from from regionally sodic-calcic altered rocks are deduced to have formed in a hydrothermal system dominated by compositionally complex fluids. Type 3 (high density CO2) inclusions may have formed by unmixing from aqueous brine phase. The Type 1 and 2 inclusions imply that at least two fundamentally different types of aqueous brine were present echoing the situation that has been found in other Cloncurry district Cu-Au deposits (e.g. Williams et al. 2001). High salinity brines are most likely to have cotransported Cu and Au in the system though ore-stage Type 1 inclusions studied by PIXE have much lower Cu concentrations than were found at the much smaller Starra Au-Cu deposit (Williams et al. 2001). They do however high concentrations of Zn, Pb and Ba compared both to premineralization Type 1 inclusions and the relatively Cu-rich brines from Starra. This suggests ore deposition was associated with the influx of a distinct mineralizing brine and although the studied Type 1 inclusions could indicate that the ore was deposited by efficient Cu precipitation from a very large mass of fluid a more plausible explanation maybe that the analyzed inclusions represent a “spent” fluid after chalcopyrite precipitation (cf. Mark et al. 2005). Assuming that fluid Br/Cl ratios would have been essentially insensitive to fluid-rock interactions, then the variable measured values in Type 1 inclusions imply they derived their salinity from more than one source and including a component with Br/Cl similar to evaporitic halite. The rocks near Ernest Henry have evidently undergone extensive fluid-rock interactions at elevated temperatures. The O-H stable isotopic data are consistent with substantial magmatic contributions of these elements during the main presyn mineralization stages but given that immediate host rocks are igneous, cannot be taken to demonstrate an exclusively magmatic fluid source. Compared to Olympic Dam, Ernest Henry seems to have formed from relatively high temperature and salinity fluids without a significant contribution from surfice waters (cf. Oreskes and Einaudi 1992). Close 788 Geordie Mark · Patrick J. Williams · Nick H.S. Oliver · Chris Ryan · Terry Mernagh Acknowledgements This research was supported by the Australian Research Council, Ernest Henry Mining and MIM Exploration. The project was planned and executed in collaboration with Richard Crookes and Rick Valenta. References Barton MD, Johnson DA (2004) Footprints of Fe-oxide(-Cu-Au) systems. SEG 2004: Predictive Mineral Discovery Under Cover. Centre for Global Metallogeny, The University of Western Australia, Special Publication 33: 112-116 De Jong G, Williams PJ (1995) Giant metasomatic system formed during exhumation of mid crustal Proterozoic rocks in the vicinity of the Cloncurry Fault, NW Queensland: Australian Journal of Earth Sciences 42: 281-290 Mark G, Oliver NHS, Williams PJ (in press) Mineralogical and chemical evolution of the Ernest Henry Fe oxide-Cu-Au ore system, Cloncurry district, northwest Queensland, Australia: Mineralium Deposita Mark G, Wilde AR, Oliver NHS, Williams PJ (2005) Predicting alteration patterns in the outflow zones of hydrothermal ore systems: a case study using the “spent” fluids from the Ernest Henry Fe-oxide-Cu-Au deposit: Journal of Geochemical Exploration 85: 31–46 Oreskes N, Einaudi MT (1992) Origin of hydrothermal fluids at Olympic Dam: preliminary results from fluid inclusions and stable isotopes: Economic Geology 87: 64-90 Page RW, Sun S-S (1998) Aspects of geochronology and crustal evolution in the Eastern Fold Belt, Mt Isa Inlier: Australian Journal of Earth Sciences 45: 343-361 Reeve JS, Cross KC, Smith RN, Oreskes N (1990) Olympic Dam copper-uranium-gold-silver deposit: Australasian Institute of Mining and Metallurgy Monograph 14:1009-1035 Ryan CG, McInnes BM, Williams PJ, Guoyi Dong, Tin Tin Win, Yeats CJ (2001) Imaging fluid inclusion content using the new CSIROGEMOC nuclear microprobe: Instruments and Methods in Physics Research B 181: 570-577 Twyerould SC (1997) The geology and genesis of the Ernest Henry Fe-Cu-Au deposit, NW Queensland, Australia: Unpublished PhD thesis, University of Oregon. 494pp Williams PJ, Dong Guoyi, Pollard PJ, Perring C, Ryan CG Mernagh TP (1999) Fluid inclusion geochemistry of Cloncurry (Fe)-CuAu deposits: In: Stanley CJ et al. (eds) Mineral Deposits: Processes to Processing. Balkema, Rotterdam, pp 111-114 Williams PJ, Guoyi Dong, Ryan CG, Pollard PJ, Rotherham, JF, Mernagh TP, Chapman LH (2001) Geochemistry of high salinity fluid inclusions from the Starra (Fe)-Cu-Au deposit, Cloncurry district, Queensland: Economic Geology 96: 875-883 Williams PJ, Pollard PJ (2003) Australian Proterozoic iron oxide-CuAu deposits: An overview with new metallogenic and exploration data from the Cloncurry district, northwest Queensland. Exploration and Mining Geology 10: 191-213 Close Chapter 7-18 7-18 The Re-Os age for molybdenite from the Variscan Strzegom-Sobótka massif, SW Poland Stanislaw Z. Mikulski Department of Economic Geology, Polish Geological Institute, 4 Rakowiecka St., 00-975 Warsaw, Poland Holly J. Stein AIRIE Program, Department of Geosciences, Colorado State University, Fort Collins, CO 80523-1482 USA Norges Geologiske Undersøkelse, Leiv Eirikssons vei 39, 7491 Trondheim, Norway Abstract. Molybdenites from quartz veins in a late Variscan granite from the Fore-Sudetic block in southwest Poland yield ages of 309 to 304 Ma with the Re-Os method. The ages of the molybdenites reflect post-magmatic hydrothermal activity associated with leucogranite porphyry (aplogranite) related to regional uplift and shear deformation during Westphalian time within this part of the Saxothuringian zone of the European Variscan belt. Keywords. Molybdenite, Re-Os, Strzegom-Sobótka granites, ForeSudetic block, SW Poland, Bohemian Massif 1 Introduction Re-Os dating of molybdenite has been successfully employed to date magmatic and metamorphic pulses within orogenic cycles (Bingen and Stein 2003; Requia et al. 2003). Magmatism associated with deformation and hydrothermal activity in regional scale shear zones has also been dated using molybdenite geochronology (Stein et al., in press). In northern Sweden, over 100 m.y. of Svecofennian orogenic history is recorded in molybdenite, both within magmatic and metamorphic assemblages, and low Re concentrations are attributed to molybdenite derived by local biotite breakdown (Stein, in press). In the northeastern part of the Bohemian massif that constitutes the Saxothuringian zone of the European Variscan belt, exposed crystalline rocks in the Western Sudetes continue under the Cenozoic cover across the Sudetic Marginal fault into the Fore-Sudetic block to the Odra Fault Zone, which defines the northeastern boundary of the massif. During the Carboniferous and early Permian, a major post-orogenic episode of granitic magmatism and coeval volcanism occurred. Most of the granites in this region are generally late to post-tectonic I-type and S-type intrusions with a span of Rb-Sr ages from ~330 to 280 Ma (Pin et al. 1989; Duthou et al 1991; Oberc-Dziedzic et al. 1996; Kennan et al. 1999). 2 for the SSG range from 0.703 to 0.707 (Kennan et al. 1999). However, for some of petrographic variants this ratio is as high as 0.708-0.709 probably due to crustal contamination (Pin et al. 1989). The Strzegom-Sobótka granites are calcic to calc-alkaline in character (Oberc-Dziedzic et al. 1999). Using the Pearce et al. (1984) classification scheme, the SSG are within the late orogenic to syn-collisional granite groups. Numerous faults divide the SSGM into an elevated western part and downthrown middle and eastern parts. The SSGM contains three petrographic varieties (Majerowicz 1972; Maciejewski and Morawski 1975; Puziewicz 1985, 1990): 1. equigranular to porphyritic monzonite granite (Kostrza type, western SSGM), 2. equigranular biotite granodiorite (Chwalków type, central and eastern SSGM), 3. equigranular two-mica monzonite granite (eastern SSGM). The Strzegom-Sobótka granitoid Massif The Strzegom-Sobótka granites (SSG) are classified as Itype granites, based on their generally low A/CNK (commonly less than 1.1). The 87Sr/86Sr initial ratios determined Close 790 Stanislaw Z. Mikulski · Holly J. Stein 3 The granite intrusion has two phases. A younger phase is represented by Kostrza-type granite and leucogranite from the Paszowice quarry. Rb-Sr ages for two-mica granite from the SSGM provide an age of ca. 330-325 Ma (± 22 Ma), whereas some of monzogranites have a reported age of ca. 290 Ma (Pin et al. 1989). Based on Rb-Sr wholerock isochron ages, Kennan et al. (1999) suggest that posttectonic Carboniferous granites in the Western Sudetes, including some of the Strzegom-Sobótka massif, were emplaced over a short time interval at ~328 Ma and derived from a source with similar 87Sr/86Sr initial ratios. The present U/Pb dating of monazite and xenotime from two-mica granites of SSGM yielded ages of 309.1 ± 0.8 Ma and 306.4 ± 0.8 Ma, respectively and indicate for the younger emplacement of the two-mica granites during the late Westphalian (Turniak and Bröcker 2002). The relation of the leucogranite porphyry (aplogranite) from the Paszowice quarry to the entire SSGM is not well understood (Pendias and Walenczak 1956; Majerowicz 1972). Molybdenite mineralization from the Paszowice quarry In the NW part of the Strzegom-Sobótka granitoid massif (SSGM), numerous occurrences of molybdenite mineralization have been documented (Pendias and Walenczak 1956; Salacinski 1978). Among other localities, Mo mineralization is found in the abandoned aplogranite quarry near the Paszowice village (Fig. 1). Here, mineralization occurs in a system of gray quartz veinlets up to 2 cm thick that cut fine-grained leucogranite porphyry (aplogranite). The veins are oriented at 290300° and dip steeply to the NE. The ore veinlets are cut by massive but barren milky quartz veinlets striking 240°. Molybdenite is a major sulfide present in veinlets forming either monomineral concentrations or may occur in paragenetic association with other sulfides (chalcopyrite, pyrite) native bismuth, or rarely with oxides such as wolframite and cassiterite (Pendias and Walenczak 1956; Salacinski 1973). The ore mineralization is accompanied by feldspathization, albitization, silicification, sericitization and chloritization. The deposit has a moderate to high temperature hydrothermal origin based on ore paragenesis (Salacinski 1978). According to fluid inclusion studies of sulfide-bearing quartz veinlets the deposit has been classified as mesothermal based on temperatures and pressures of 361-236°C and ~0.9 MPa, respectively (Ilnicki 1998). Ore-bearing quartz veinlets have also been found in three oriented prospecting holes drilled in 1957 in the surrounding area (Chilinska, unpublished). The average content of Mo is 0.34 wt% and of Cu 0.13 wt%. Existing data from these boreholes and from the surface geochemical prospecting led to the classification of the mineralization as Mo-Cu stockwork type (Kanasiewicz and Mikulski 1989). Two zones of quartz vein Mo-Cu mineralization are now identified, extending to 100 m below the surface (Fig. 2). They occupy shear zones oriented NWSW and dipping 70-80° NE. The shear zones range from about 2 to 5 m in thickness. 4 Sample description for Re-Os data Two molybdenite samples for Re-Os dating were collected from the lowest level in the central part of the quarry within the Strzegom-Sobótka granitoid massif. Molybdenite in quartz veins represents the main stage of mineralization. Euhedral molybdenite was selected from finecrystalline gray quartz veins (up to 2 cm thick) cutting fine-grained leucogranite porphyry (aplogranite). Some crystals form rosette aggregates 3-5 mm in diameter. The length of single molybdenite flakes is usually <1 mm with a width of ~0.1 mm. Larger molybdenite crystals are curved and overgrown by chalcopyrite or pyrite, or they may contain fine-grained chalcopyrite and pyrite grains Close Chapter 7-18 · The Re-Os age for molybdenite from the Variscan Strzegom-Sobótka massif, SW Poland intergrown within molybdenite crystal cleavage, indicating an intimate temporal relationship. Albite crystals may be found within quartz veinlets, but more commonly albite together with chlorite (after biotite) is found marginal to the quartz veins. 5 Methods and results Re-Os dating of molybdenite is described in Stein et al. (2001). We present the results of high precision Re-Os age determinations for two molybdenite samples using procedures and techniques outlined in Markey et al. (2003). A mixed double Os spike was used (185Re, 188Os-190Os). The samples have low Re contents, all < 1 ppm, and the resulting ages range from 309 to 304 Ma. A replicate of sample #3, is provided in MDID-315. Sample weights ranged from 41 to 73 mg. 6 Discussion Re-Os dating of molybdenites from the Paszowice quarry from the western part of the Strzegom-Sobótka granitoids massif yields ages from 309 to 304 Ma. Their markedly low Re concentrations (<1 ppm) are consistent with a derivation related to metamorphic processes (Stein, in press). The Mo mineralization clearly postdates emplacement of leucogranite porphyry (aplogranite), but is considered as either (1) related to post-magmatic processes associated with the emplacement of evolved and Mo-specialized leucogranite magma (Kanasiewicz and Mikulski 1989), or (2) related to metamorphic processes and the development of shear zones. Field relationships permit an interpretation whereby the Paszowice leucogranite and mineralized quartz veins were emplaced during shear deformation in late Variscan time. Re-Os dating of molybdenite provides an age for this deformation of about 310-305 Ma. Thus, the Mo mineralization formed during 791 uplift of the Variscan orogen. The unidirectional NW-SE strike of the ore veinlets at the Paszowice quarry and the vein-hosted Mo zones recognized by boreholes are similar to the direction of the Marginal Sudetic fault, which was also active during the Upper Carboniferous (Zelazniewicz et al. 1997). Mo mineralization of similar type and age (307 ± 3 Ma) has been reported from the southern margin of the Variscan orogen (Langthaler et al. 2004) and similarly, but slightly younger Re-Os ages from Sardinia are also latest Variscan (289 ± 1 Ma; Boni et al. 2003). In Sardinia, at least two ages of leucogranites are recognized, with only the younger one displaying Mo mineralization and the older (~310-300 Ma) being barren (Boni et al. 2003). The molybdenite Re-Os ages from the SSGM also coincide with a sharp increase in the rate of uplift in the Massif Central (310-305 Ma; Bouchot et al. 2000) that consitute the western part of European Variscides. Acknowledgements The analytical work was supported by the National Committee Scientific Research, Grant 5 T12B 001 22. Special thanks goes to Dr. S. Ilnicki for providing one of molybdenite samples. References Bingen B, Stein HJ (2003) Molybdenite Re-Os dating of biotite dehydration melting in the Rogaland high-temperature granulites, S Norway. Earth and Planet Scientific Letter 208: 181-195 Boni M, Stein HJ, Zimmerman A, Villa IM (2003) Re-Os age for molybdenite from SW Sardinia (Italy): A comparison with Ar/Ar dating of Variscan granitoids. In: Eliopoulos et al (eds), Mineral Exploration and Sustainable Development: pp 247-250. Millpress, Rotterdam Bouchot V, Milesi JP Ledru P (2000) Crustal scale hydrothermal Paleofield and related Au, Sb, W orogenic deposits at 310-305 Ma (Massif Central). SGA News 10: 6-10 Duthou JL, Couturie JP Mierzejewski MP, Pin C (1991) Next dating of granite sample from the Karkonosze Mountains using Rb-Sr total rock isochrones method. Przeglad Geologiczny 39:75-79 Ilnicki S (1998) Conditions of hydrothermal alterations in aplite from Paszowice (Strzegom-Sobótka massif). Mineralogia Polonica 29: 29-42 Kanasiewicz J, Mikulski SZ (1989) On the occurrence possibility of the molybdenium deposit of Cu-Mo formation on the Strzegom granites massif. Przeglad Geologiczny 37: 129-133 Kennan PS, Dziedzic H, Lorenc MW Mierzejewski MP (1999) A review of Rb-Sr isotope patterns in the Carbo-niferous granitoids of the Sudetes in Poland. Geologia Sudetica 32: 49-53 Kural S, Morawski T (1968) Strzegom-Sobótka granitic massif. Biuletyn Instytutu Geologicznego 227: 33-85 Langthaler KJ, Raith JG, Cornell DH, Stein HJ, Melcher F (2004) Molybdenum mineralization at Alpeiner Scharte, Tyrol (Austria): results of in-situ U-Pb zircon and Re-Os molybdenite dating. Mineralogy and Petrology 82: 33-64 Maciejewski S, Morawski T (1975) Petrographic diversity of granites of the Strzegom massif. Kwartalnik Geologiczny 19: 47-65 Close 792 Stanislaw Z. Mikulski · Holly J. Stein Majerowicz A (1972) The Strzegom-Sobótka granite massif. Geologia Sudetica 6: 7-96 Markey R, Hannah JL, Morgan JW, Stein HJ (2003) A double spike for osmium analysis of highly radiogenic samples. Chemical Geology 200: 395-406 Oberc-Dziedzic T, Zelazniewicz A, Cwojdzinski S (1999) Granitoids of the Odra Fault Zone: late- to post-orogenic Variscan intrusions, SW Poland. Geologia Sudetica 32: 55-71 Pearce JA, Harris NB, Tindle AG (1984) Trace Element Discrimination Diagrams for the Tectonic Interpretation of Granitic rocks. Journal Petrology 25: 956–983 Pendias H, Walenczak Z (1956) Signs of mineralization in the NW part of Strzegom Massif. Biuletyn Instytutu Geologicznego 227: 209-228 Pin C, Puziewicz J, Duthou JL (1989) Ages and origins of a composite granitic massif in the Variscan belt: a Rb-Sr study of the Strzegom-Sobótka Massif. Neues Jahrbuch Mineralogische Abhandlungen 160: 71-82 Puziewicz J (1985) Origin of chemical, structural and textural variations in aplites from Strzegom granite (Poland). Neues Jahrbuch Mineralogische Abhandlungen 153: 19-31 Puziewicz, J., 1990. Strzegom-Sobotka granitic massif (SW Poland). Summary of recent studies. Archiwum Mineralogiczne 45: 135-154 Requia K, Stein HJ, Fontboté L, Chiaradia M (2003) Re-Os and Pb-Pb geochronology of the Archean Salobo iron oxide copper-gold deposit, Northern Brazil. Mineralium Deposita 38: 727-738 Salacinski R (1973) Ore mineralization in granite at Paszowice. Acta Geologica Polonica 23: 587-596 Salacinski R (1978) Ore mineralization and its origin in the granitoids of the Strzegom massif. Biuletyn Instytutu Geologicznego 308: 41-90 Smoliar MI, Walker RJ, Morgan JW (1996) Re-Os ages of group II1, IIIA, IVA and IVB iron meteorites. Science 271: 117-133 Stein HJ, Hannah JL, Zimmerman A, Markey R, Sarkar SC, Pal AB, in press, A 2.5 Ga porphyry Cu-Mo-Au deposit at Malanjkhand, central India: implications for Late Archean continental assembly. Precambrian Research. Stein HJ, in press, Low-rhenium molybdenite by metamorphism: recognition, sampling, genesis, economics, and regional implications based on examples from northern Sweden. Lithos. Stein HJ, Markey RJ, Morgan JW, Hannah JL, Scherstén A (2001) The remarkable Re-Os chronometer in molybdenite: how and why it works. Terra Nova 13: 479-486 Turniak K, Bröcker M (2002) Age of the two-mica granite from the Strzegom Massif: new data from U/Pb monazite and xenotime study. Mineralogical Society of Poland Special Papers 20: 211-213 Zelazniewicz A, Cwojdzinski S, England P, Zientara P (1997) Variscides in the Sudetes and the reworked Cadomian orogen: evidence from the GB-2A seismic reflection profiling in southwestern Poland. Geological Quarterly 41 (3): 289-308 Close Chapter 7-19 7-19 Re-Os ages for auriferous sulfides from the gold deposits in the Kaczawa Mountains (SW Poland) Stanislaw Z. Mikulski Department of Economic Geology, Polish Geological Institute, 4 Rakowiecka St., 00-975 Warsaw, Poland Richard J. Markey1, Holly J. Stein1, 2 1 AIRIE Program, Department of Geosciences, Colorado State University, Fort Collins, CO 80523-1482 USA 2 Norges Geologiske Undersøkelse, Leiv Eirikssons vei 39, 7491 Trondheim, Norway Abstract. A Re-Os six-point isochron age of 317 ± 17 Ma has been obtained for auriferous sulfides from sheeted quartz-veins representing the first stage of ore precipitation at the Radzimowice AuAs-Cu deposit. The age uncertainty is dominated by the fact that sulfides contain very little common Os. Extremely low Re concentrations for gold-bearing sulfides from another gold district, KleczaRadomice, permitted dating of only one Co-arsenopyrite sample G-4 from Klecza – analyzed as a Low Level Highly Radiogenic (LLHR) sample. A precise age of 316.6 ± 0.4 Ma was obtained. Re-Os ages indicate gold mineralization in Late Namurian time associated with post-collisional extension and regional uplift in a continental arc setting. Opening of deep-seated structures, marked also by the presence of lamprophyre dykes, may have allowed for the migration of post-magmatic mineralizing fluids from various magmatic sources at about 317 Ma. Keywords. Gold, Re-Os, low level and highly radiogenic sulfides (LLHR), Kaczawa Mountains, SW Poland, Bohemian Massif 1 Introduction The Re-Os method has been successfully applied to molybdenite and can be similarly applied to other sulfides with much lower concentrations of Re and Os, provided the Re/Os ratio is very high. These sulfides have been named LLHR (low level highly radiogenic), as their Os isotopic composition mimics molybdenite (Stein et al. 2000). LLHR sulfides are samples whose 187Os dominates the total Os. They are common in some hydrothermal environments, and may be particularly common in small crustally-derived deposits (Stein et al. 2000). The first Re-Os isotopic ages for LLHR sulfides closely associated with Au mineralization were reported from Bendigo, Australia (Arne et al. 2001). Recently, the giant Muruntau Au deposit was successfully dated using LLHR samples of arsenopyrite (Morelli et al. 2004). Analysis of samples with extremely low-level Os contents is dominated by Os contributions from procedural blanks (Markey et al. 2003). Subtraction of blank contributions in such cases may result in significant adjustments to the 187Os/188Os ratio, with a commensurate increase in the uncertainties of both the isotopic composition and the concentration of Os in the samples. 2 Geological setting In the northwestern part of the Bohemian Massif, i.e., the Western Sudetes that constitute the eastern fragment of the Saxothuringian Zone of the European Variscides, several abandoned small and medium size gold-bearing arsenic-polymetallic deposits are found (Manecki 1965; Paulo and Salamon 1974; Mikulski 2001). Among them, there is still a high potential for exploration in vein deposits in Radzimowice and the Klecza-Radomice gold ore district (KROD) in the Kaczawa Mountains. In these deposits the major gold, silver, and arsenic production came from the sheeted quartz-sulfide veins, and vein arrays in folded flysch-like sediments deformed and metamorphosed to lower greenschist facies during Upper Devonian-Lower Carboniferous. At the Radzimowice and Klecza deposits the most important ore minerals are refractory gold-bearing Co-arsenopyrite and pyrite. This stage of mineralization underwent strong cataclasis and was later overprinted by base metal sulfides and non-refractory gold associated with quartz and carbonates. The Radzimowice auriferous ore mineralization is considered transitional between a porphyry and epithermal type around the Upper Carboniferous composite Zelezniak porphyry intrusion of subalkaline to alkaline igneous rocks formed in a post-collisional arc setting (Mikulski 2005). The genesis of gold mineralization at the KleczaRadomice ore district was commonly assumed to be a hydrothermal type connected with Variscan KarkonoszeJizera granites. Recently auriferous mineralization is classified as orogenic type (Mikulski 2003). 3 Sample description for Re-Os data The auriferous sulfide samples for Re-Os dating were collected from the old mining wastes and underground workings of the Luis shaft in the northern part of the Radzimowice Au-As-Cu deposit and from the old mining wastes of the Klecza Northern Ore Field of the KROD. Auriferous sulfide mineralization occurs as massive or semi-massive ores in quartz veins that have been brecci- Close 794 Stanislaw Z. Mikulski · Richard J. Markey · Holly J. Stein ated and cemented by a younger generation of quartzcarbonate and base metal sulfides with non-refractory gold. For Re-Os measurements we selected medium-, and fine-grained (0.5 to 3 mm) euhedral Co-arsenopyrite, pyrite and chalcopyrite non-fractured crystals. Arsenopyrite crystals from Radzimowice display compositional variability in their As contents (34.8 to 37.4 at.%) and high admixtures of cobalt (up to 6.4 at.%) and refractory gold. Refractory gold (ca. 70 ppm) appears as sub-microscopic inclusions within Co-bearing arsenopyrite and is less abundant in pyrite. Arsenopyrite from Klecza has arsenic contents between 31.5 and 33.4 at.% and a cobalt admixture from 0.1 to 0.9 at.%. 4 Methods and results Re and 187Os concentrations in selected sulfides were determined at AIRIE, Colorado State University, using procedures and techniques outlined in Stein et al. (2000) and Markey et al. (2003). Analyses of auriferous Co-arsenopyrites from the Radzimowice Au-As-Cu deposit yield Re concentrations of 0.13-3.5 ppb with total Os in the very low ppt range (Table 1). Nearly all analyzed auriferous sulfide samples from the KROD were characterized by extremely low Re concentrations (near blank level), so age information based on those samples, with the exception of one, is not possible. Co-arsenopyrite sample G-4 from Klecza – analyzed as a LLHR sample – gave an age 316.6 ± 0.4 Ma assuming an initial 187Os/188Os ratio of 0.2 (Table 1). The LLHR arsenopyrite from Radzimowice with the highest Re content (run LL-99) yields a Re-Os model age of 317 Ma that is fairly insensitive to the assumed 187Os/188Os initial ratio (187Re/188Os > 105). A four-point isochron based on auriferous Co-arsenopyrites yields a Re-Os age of 314 ± 31 Ma (initial ratio = 0.8 ± 2.2, MSWD = 2.1). However, the large uncertainties for two Co-arsenopyrite analyses (LL-28, 29) resulting from extremely low Os contents, precludes a precise age. We note that there Close Chapter 7-19 · Re-Os ages for auriferous sulfides from the gold deposits in the Kaczawa Mountains (SW Poland) is general agreement between model ages for these samples when an Os initial ratio of 0.2 is used. We support our arsenopyrite analyses by additional analyses of a pyrite and chalcopyrite sample from the Radzimowice deposit. These sulfides also contained low to very low ppt level Re and Os (Table 1). Collectively, all sulfide analyses from Radzimowice provide a six-point isochron with a Re-Os age of 317 ± 17 Ma (Fig. 2). The six-point isochron has a reduced uncertainty compared to the four-point isochron based only on Co-arsenopyrite samples. The still relatively large uncertainty is due to the very low Os concentrations of most of the samples (<5 ppt total Os in all cases but one). Within uncertainty, the Re-Os isochron age overlaps with a much more precise model age of 316.6 ± 0.4 Ma for Co-arsenopyrite sample G-4 (run MDID350) from the Klecza deposit. 5 Discussion According to 40Ar/39Ar data presented by Marheine et al. (2002), in the Western Sudetes, host rock schists of Ordovician-Lower Carboniferous represent shaly flysch-type sediments that were recrystallized during regional uplift-related greenschist metamorphism in the Viséan at 344-333 Ma and the upper limit of the Variscan tectonometamorphic and magmatic activity was dated at 314-312 Ma (Namurian / Westphalian boundary). ReOs data suggest that refractory gold- sulfide mineralization in the Kaczawa Mountains postdates regional metamorphism of host rocks and orogenic deformation. Refractory gold mineralization is related to Late-Namurian tectonometamorphic and magmatic processes. At the Radzimowice Au-As-Cu deposit, the schist unit was intruded by the Zelezniak Intrusion (ZI) (Mikulski 2005). Gold-bearing sulfide veins cut dacite porphyries and postdate lamprophyre dykes, but are spatially associated with the dykes. SHRIMP ages for zircons from the fine-grained rhyolite are similar to zircon ages from the mediumgrained microgranites of ZI, and indicate that the main 795 magmatic event was restricted to the Late Namurian (weighted mean 206Pb/238U at 316.7 ± 1.2 Ma; Muszynski et al. 2002). The Re-Os age of ca. 317 Ma for arsenopyrite sample LL-99 in the context of SHRIMP ages from ZI support an association between post-orogenic felsic magmatism and auriferous Co-arsenopyrite mineralization. This is further supported by the six point 317 ± 17 Ma Re-Os isochron age. The spatial association of quartzsulfide veins with lamprophyre dykes implicates them in the ore-forming process, and suggests they are also of similar age. Genesis of the gold mineralization in Klecza, like other Au deposits and occurrences in the KROD, is suggested to be of orogenic type (Mikulski 2003). The KROD deposit is located in the Intra Sudetic Fault zone that separates two different terranes (Aleksandrowski et al. 1997). At KROD there is no evidence for a direct magmatic origin for hydrothermal fluids responsible for the gold mineralization, despite the widely held belief that mineralization is related to the Karkonosze-Jizera granites located ca. 10 km to the south. Re-Os data for auriferous Co-arsenopyrite from Klecza (316.6 ± 0.4 Ma), the first stage of refractory gold mineralization, may be slightly younger than the porphyritic granites of the KarkonoszeJzera pluton dated at 325-330 Ma by the Rb-Sr method (Duthou et al. 1991) or date at 320 ± 2 Ma by 40Ar/39Ar on biotite (Marheine et al. 2002). Au mineralization is most likely associated with lamprophyre dykes dated at 314 ± 6 Ma 40Ar/39Ar (Marheine et al. 2002) or with aplitic granites date at 310 ± 5 Ma by Rb-Sr (Duthou et al. 1991). Summarizing, our Re-Os results indicate that one of the major Late Namurian post-orogenic extension episodes and regional uplift in the Kaczawa Mountains took place ca. 317 Ma. Deep-seated structures allowed mineralizing fluids, mostly likely associated with magmatic sources, to migrate upwards, forming auriferous sulfide mineralization. The age of auriferous mineralization (ca. 317 Ma) recognized in the Kaczawa Mountains is not coeval with gold events described from the Central Bohemian province (ca. 338 Ma; Bouchot et al. 2001; or at 344 ± 2.8 Ma by Re-Os method on molybdenite by Zachariáš et al. 2001) and Massif Central (310-305 Ma; Bouchot et al. 2000). Acknowledgements The analytical work was supported by NCSR, Grant no. 5 T12B 001 22. References Aleksandrowski P, Kryza R, Mazur S, Zaba J (1997) Kinematics data on major Variscan strike-slip faults and shear zones in Sudetes. Geol Magazine 134: 727-739 Arne DC, Bierlein FP, Morgan JW, Stein HJ (2001) Re-Os dating of sulfides associated with gold mineralization in Victoria, Australia. Economic Geology 96: 1455-1459 Close 796 Stanislaw Z. Mikulski · Richard J. Markey · Holly J. Stein Bouchot V, Faure M, Feybesse JL, Correira P, Zachariáš J (2001) Variscan orogenic Au district related to a regional Visean detachment in the Central Bohemian province. In: Eliopoulos et al (eds) Mineral Exploration and Sustainable Development. Millpress, pp 747-750 Bouchot V, Milesi JP Ledru P (2000) Crustal scale hydro-thermal Palaeofield and related Au, Sb, W orogenic deposits at 310-305 Ma (Massif Central). SGA News 10: 6-10 Duthou JL, Couturie JP, Mierzejewski MP, Pin C (1991) Rb/Sr whole rock samples isochrones method of the age determination of the Karkonosze granite (in Polish). Przeglad Geologiczny 32: 75-79 Manecki A (1965) Petrographic-mineralogical studies of the polymetallic veins from Wojcieszow vicinities (Lower Silesia). Prace Mineralogiczne PAN, 47 (2): pp 65 Marheine D, Kachlik V, Maluski H, Patocka F, Zelazniewicz A (2002) The 40Ar/39Ar ages from the West Sudetes (NE Bohemian Massif): constraints on the Variscan polyphase tectonothermal development. In: Winchester JA, Pharaoh TC, Verniers J (eds) Palaeozoic Amalgamation of Central Europe. Geological Society of London Special Publication 201: 133-155 Markey R, Hannah JL, Morgan JW, Stein HJ (2003) A double spike for osmium analysis of highly radiogenic samples. Chemical Geology 200: 395-406 Mikulski SZ (2001) Late-Hercynian gold-bearing arsenic-polymetallic mineralization in Saxothuringian zone in the Polish Sudetes, NE Bohemian Massif. In: Piestrzynski et al (eds), Mineral Deposits at the Beginning of the 21st century. Balkema, pp 787-790 Mikulski SZ (2003) Orogenic quartz-sulfide-gold veins from the Klecza-Radomice ore district in the Kaczawa Mountains (Western Sudetes) – NE part of Bohemian Massif. In: Eliopoulos et al (eds), Mineral Exploration and Sustainable Development, Millpress, pp 787-790 Mikulski SZ (2005) Geological, mineralogical and geochemical characteristics of the Radzimowice Au-As-Cu deposit from the Kaczawa Mts. (Western Sudetes, Poland) - an example of the transition of porphyry and epithermal style. Mineralium Deposita 39: 904-920 Morelli, R, Creaser, RA, Seltmann, R (2004) The age of gold mineralization at the Muruntau Au deposit, Uzbekistan, from Re-Os arsenopyrite geochronology. Geological Society America Abstracts with Programs 36 (5): 444 Muszynski A, Machowiak K, Kryza R, Armstrong R (2002) SHRIMP U-Pb zircon geochronology of the Zelezniak rhyolite intrusion, Sudetes – preliminary results. Mineral Society of Poland – Special Papers 19: 156-158 Paulo A, Salamon W (1974) Contribution to the knowledge of the Stara Gora deposit. Kwartalnik Geol 18: 266-276 Stein HJ, Morgan JW, Scheresten A (2000) Re-Os of low level highly radiogenic (LLHR) sulfides: The Harnas gold deposit, southwest Sweden, records continental-scale tectonic events. Economic Geology 95: 1657-1671 Zachariáš J, Pertold Z, Pudilová M, Zák K, Pertoldová J, Stein H, Markey R (2001) Geology and genesis of Variscan porphyry-style gold mineralization, PetrácÌŒkova hora deposit, Bohemian Massif, Czech Republic. Mineralium Deposita 36: 517-541 Close Chapter 7-20 7-20 Dating of gold occurrences in the Sayan-Baikal Fold Belt, Southern Siberia, Russia A.G. Mironov Geological Institute of SB RAS, Sakhyanova 6a, Ulan-Ude, 670047, Russia H. Stein, A. Zimmerman AIRIE Program, Department of Geosciences, Colorado State University, Fort Collins, CO 80512-1482 USA S.M. Zhmodik Institute of Geology UIGGM SB RAS, Koptyuga 3, Novosibirsk, 630090, Russia Abstract. The complex geologic history of the Tain gold-porphyry deposit in the Sayan-Baikal Fold Belt (South Siberia) makes direct age determinations problematic. Timing of porphyry gold mineralization, magmatism, and hydrothermal alteration are constrained to an interval of 670-280 Ma based on dating of the host granodiorites, altered rocks, and ores by the Rb-Sr, Ar-Ar, and Re-Os techniques, respectively. Keywords. Sayan-Baikal Fold Belt, gold-porphyry deposit, dating, ArAr, Rb-Sr, Re-Os techniques 1 Introduction The gold-bearing Sayan-Baikal Fold Belt is known for its important ore reserves. Both quartz lode deposits (Pioneer, Granite, Dynamite, Irokinda, etc.) and gold-sulfide polymetallic deposits, along with sub-economic ore occurrences (Zun-Kholba, Zun-Ospin, etc.), are located in the Belt (Mironov and Zhmodik 1999). Only recently, new types of gold mineralization such as those at Tain, Konevinskoye, and Kharalginskoye have been discovered. The Tain deposit is of particular significance as it appears genetically different from previously studied deposits in the region and has unique geolocial features. The Tain gold deposit lies in the central Ospin-Kitoi massif of ultrabasic rocks comprising the ophiolitic Ilchir plate. Regionally, the Gargan Craton consists of ArcheanProterozoic volcanogenic-sedimentary strata, ophiolite sequences of the Neo-Proterozoic age, and granitoids of the Sumsunur (PZ1-2) and Samsal (PZ2-3) sequences. The Ospin-Kitoi ultrabasic massif is defined by the convergence of ophiolite outcrops from north to south in the eastern Gargan Craton. The massif is suggested to be a single unit later dissected by erosion associated with uplift of the Gargan Craton and preserved along its periphery (Belichenko et al. 1988). 2 Gold deposit description The Tain deposit is localized in 300 m by 700 m granodiorites and plagiogranites stocks that crosscut local serpentinites and serpentinized harzburgites (Fig. 1). The massif hosting gold mineralization is shaped like two attached lenses. The inner massif is composed of the grey mid- to fine-grained diorites and quartz diorites (granodiorites) that are variably altered and deformed. The marginal areas of the massif are variably enriched in yet to identified carbonaceous matter. The carbonaceous matter is commonly encountered as fine dust in quartz, along zone planes, or as dust-like spotted disseminations in plagioclase. The carbonaceous matter is also observed in the cross-cutting microfractures, occasionally associated with epidote-clinozoisite. The granulated aggregates of albite replacing calcic plagioclase are also pigmented by dustlike carbonaceous matter (Mironov et al. 2001). The beresitized rocks and beresites (mineral association of quartz, sericite, pyrite, and calcite) are the dominant rock type in the massif. They are greenish-grey fineand medium-grained rocks composed of sericitized plagioclase, quartz, sericite, calcite, chlorite, sulfides (pyrrhotite predominates), leucoxene, apatite, and zircon. Quartz is characterized by two varieties, i.e., pressed, fractured grains (quartz 1) and almost undeformed aggregates (quartz 2). Sulfides are represented by impregnations (0.1-1.5mm) of pyrrhotite. Pyrite is associated with quartz 2, iron hydroxides, and calcite or chlorite. The low SiO2 concentrations, higher concentrations of MgO and CaO and dominantly more Na2O than K2O are characteristic of beresitized rocks. In the southern part of the massif, accompanying and hosting gold mineralization are medium to dark grey, variably grain-sized, porphyritic plagiogranites. They have an irregularly grained texture of quartz and plagioclase aggregates 0.2-5mm in size and porphyry-like quartz impregnations with traces of deformational cataclasite. Muscovite is developed along fractures in plagioclase and locally intense alteration results in completely replaced plagioclase. Calcite (up to 1-2 wt.%), sulfides (to 3-5 wt.%), sericite, biotite, sphene, rutile, apatite, and carbonaceous matter (0.1-0.5 wt.%). The carbonaceous matter gives the dark grey colour to the rock and is best developed on altered plagioclase, infilling of microfractures in quartz grains, and along fractures intersecting mineral aggregates. Close 798 A.G. Mironov · H. Stein · A. Zimmerman · S.M. Zhmodik Geochemically all the varieties of the stock granitoids have low Th and U concentrations, moderate Ba and Sr concentrations with Sr prevailing in the unaltered or weakly altered rocks, and sharp increase of Ba concentrations in muscovitized and dyke formations. The precious metal contents significantly vary, reaching maximum in the muscovitized and carbonatized rocks. Three types of orebodies: (1) quartz-veined low sulfide bodies, (2) quartz-muscovite-pyrrhotite ores and (3) veinlet-impregnated ores are identified at the Tain deposit. Quartz veined low sulfide bodies occur as 0.3 to 1.5 m thick bodies observable for 230 m along strike. The quartz veins are characterized by the carbonaceous matter-induced dark gray color and intensive boudinage structures with a clear tectonic orientation. Quartz grains within the boudins elongate by unidirectional fracturing and dislocation with equigranular grains showing pressureinduced dissolution-reprecipitation. In some locations brittle deformation is seen as cataclasis and brecciation of host granitoids.. Muscovite, chlorite, biotite, amphibole and iron hydroxides (1-3 wt.%) are locally developed in microfractures. The major ore minerals (0.1-10 wt.%) occur as nest-like features (1-8cm across) of pyrite, pyrrhotite, galena, sphalerite and chalcopyrite. These minerals also occur as fine impregnations. Rare ore minerals hessite, wehrlite, argentite, native gold and silver are associated with netlike features as well. Quartz-muscovite-pyrrhotite ores are differientiated by high sulfide contents, mainly pyrrhotite, comprising up to 70% of the total rock, hosted in light grey and white quartz muscovite granitoids. The vein-like bodies are up to 0.6 m thick in the quarry walls, hardly accessible, and dominantly studied from rockfall in talus piles. In contrast to the quartz veins, this type of ore is characterized by lighter colored quartz without carbonaceous matter, high precious metal contents between 150 to 200 ppm Au and 300 to 450 ppm Ag, and a peculiar paragenesis of gold and sulfide minerals. Hexagonal pyrrhotite is the dominant sulfide mineral comprising 95-98 vol.% of ore minerals. Chalcopyrite (0.1-3 vol.%) occurs as thread veinlets and impregnations at the contact between massive pyrrhotite ores and quartz-muscovite aggregates. Pyrite, cobaltite, sphalerite, galena, kustelite, and native gold occur in subordinate amounts. Cobaltite (CoAsS) is always seen as impregnations of small (0.01-0.09mm) crystals in pyrrhotite. The important peculiarity of this ore type is the partitioning of Au and Ag into kustelite rather than other Au and Ag minerals. Kustelite forms isometric grains 0.01-0.06mm in size that localize at the contact of pyrrhotite with chalcopyrite and quartz. Ores of veined-impregnated type are found within the dark grey carbonatized, muscovitized and cataclased porphyry-like plagiogranites. The ore consists of quartz veinlets 0.5-3 cm thick and a few meters long with impregnations (0.1-5 mm) of pyrrhotite and chalcopyrite (0.5-5 vol.%) and noticably subordinate pyrite, sphalerite and galena. The plagiogranite host rocks are five to thirty meters thick and 100’s of meters long zones made of quartz-sericite-muscotite rocks with variable amounts of calcite, sulfides, and carbonaceous matter. Mineralogical analysis of this ore type identify native gold, silver, argentite, and Ag-bearing bornite. Gold is present as two distinctly different morphologies. The first is represented by middle and large native gold particles (0.1-0.3 mm and 0.7-1.0 mm, respectively) of bright yellow color and cloddy-laminar shape with high purity (915-965). The second variety is composed by small and middle (0.010.3 mm) gold particles of low purity (429-323) and kustelite. Molybdenite is found as flakes and little nests in both dark grey quartz and beresite ores. In the veinlets of dark grey quartz, molybdenite is found together with gold and, in beresite ore, it is found as “dry” veinlets along fractures. The Tain gold deposit has a number of features that are atypical of East Sayan hydrothermal deposits. The veinlet-impregnated type of ore mineralization in porphyry-like granitoids are dominant here unlike the Pioneer, Barun-Kholba, Granite, and other lode deposits. The presence of carbonaceous material, predominance of pyrrhotite among sulfides, that of kustelite among gold minerals, and of methane in the gas phase are peculular as well. In our view, it is interpreted that the Tain deposit formed in different conditions and due to the magmatism of another type. Close Chapter 7-20 · Dating of gold occurrences in the Sayan-Baikal Fold Belt, Southern Siberia, Russia The granitoids of the Tain stock belong to the granitoids of the island arc type based on geochemical data. Although variable in absolute composition, the stocks generally corresponds to the island arc granites according to the main indices (for example, Nb-Y, Rb-(Nb+Y) ratios) in discrimination plots. Predominance of Sr and Ba and low contents of U and Th are typical of unaltered varieties. Ba, Cu, and Zn concentrations increase in the beresitized and carbonatized granodiorites and granites. The maximum contents of Ba (1100-1600 ppm) have been found in the carbonatized dykes of granite-porphyries. Co and Ni predominance as well as low concentrations of U (1.33.2 ppm) and Th (0.4-3.9 ppm) are also characteristic of the granite porphyries. Analyzed rare earth elements form a trend similar to the REE trend of granitiods from the Amur-Alyaska island arc system. Some decrease of their contents is observed in ores at their enrichment in quartz and pyrrhotite. The massif rocks are intensly tectonized by subhorizonal faulting. Small, spotted occurences of plagiogranites, diorites and dacite-porphyries are known in other areas of the ophiolite cover (Ekhe-Shigns, Borto-Gol rivers, etc.). All this testifies to the fact that the Tain stock granitoids and analogous rocks formed in the island arc stage suffered deformation during the subsequent collision and obduction. In contrast, the granitoids of the Sumsunur and other younger sequences (PZ2-3) are clearly syn- and postcollisional. 3 Dating results The study of absolute age in rocks and ores of the Tain deposit shows significant variations in obtained data. A Rb-Sr isochron indicates 670±19 Ma and 87Sr/86Sr =0.7120±0.0010 on the altered porphyry-like granites and muscovite. Two Ar-Ar ages of 435±9 Ma (samples Th–330 and Th–331) and 280±4.1 Ma (Th–329) were obtained from amphiboles taken from the Tain massif diorite. Those ages are likely to indicate the later metamorphism and hydrothermal alteration of rocks. The question arises which process is associated with and/or reponsible for gold mineralization. The answer may be obtained from Re-Os data on molybdenite associated with gold mineralization. A sample of molybdenite as a rosette-like inclusion in a veinlet (6mm thick) of dark grey quartz (TN-1) and a sample of molybdenite from a “dry” veinlet (molybdenite powdery coating on the fracture surface 0.5-1.5mm thick) (sample TN-2) were selected. 799 TN-1 was taken from a single molybdenite bleb in an 0.8 cm vein of dark gray quartz, of the variety associated with Au mineralization. Although the rock is quite weathered and Fe stained, the vein and molybdenite are moderately fresh. The rock appears to be a fine-grained granitoid that is highly altered, including silicification and a vuggy nature due to leaching of mm scale feldspar. This molybdenite-bearing vein yielded a Re-Os age of about 550 Ma, but additional molybdenite separates will be taken and dated to confirm this result. TN-2 is also a fine-grained granitoid with mm scale euhedral crystals of feldspar with diffuse margins due to silicification. The rock is also sericitized. Fe-oxide staining is locally prevalent. Molybdenite occurs in abundance along a surface that appears to be the margin of an irregular, not planar, vein. The Re-Os age is about 860 Ma, but additional mineral separates are necessary to affirm geologic accuracy of this somewhat weathered occurrence. Thus, the gold mineralization in the massif has the age that is close to the island arc and island arc type granitoid formation (800-600 Ma). The Tain gold deposit contains the mineralization formed by reducing fluids and has obvious features typical of gold porphyry deposits. Its specific features are caused by granitoid emplacement in an area of ultrabasites and black shales that are enriched in carbonaceous matter of both biogenic and mantle nature. It is likely the earliest gold mineralization in the region in the massif of island arc granitoids that were subsequently subjected to obduction within the ophiolite cover and accompaning turbidite and craton terranes (Bogatikov and Tsvetkov 1988). Acknowledgements The work has been carried out with the grant support of the leading research schools No -2208.2003.5 and RFBR grant 03-05-65162. References Belichenko VG, Butov YuP, Dobretsov NL (1988) Geology and metamorphism of the East Sayan. Novosibirsk, Nauka. Bogatikov OA, Tsvetkov AA (1988) Magmatic evolution of island arcs. Moscow, Nauka. Mironov AG, Zhmodik SM (1999) Gold deposits of the Urik-Kitoi metallogenic zone (East Sayan, Russia). Geology of ore deposits. V. 41, N1, 54-69 Mironov AG, Zhmodik SM, Ochirov YuCh, Borovikov AA, Popov VD (2001) The Tain gold deposit (East Sayan, Russia) is rare type of gold-porphyry formation. Geology of ore deposits. N5, 395–413 Close Close Chapter 7-21 7-21 Jurassic magmatism and Au-Ag mineralization in the Deseado Massif (Patagonia Argentina): Lead and sulfur isotopic studies P. Moreira, R.R. Fernández, I.A. Schalamuk, R.O. Etcheverry Instituto de Recursos Minerales (INREMI), Universidad Nacional de La Plata, CICBA, Argentina A.P. Rolando Pará-Iso Laboratory, Instituto de Geociencias, Universidade Federal do Pará, Belém, Brazil Abstract. Lead isotope analyses of volcanic rocks and hydrothermal minerals and sulfide isotope analyses of sulfurs from Au-Ag La Josefina prospect (Deseado Massif geological province, Argentina) are reported. Lead isotope ratios for sphalerite and pyrite have mean values of 18.48, 15.69 and 38.61 for 206Pb/204Pb, 207Pb/204Pb and 208Pb/204Pb, respectively, and are similar to Pb isotope ratios for the Jurassic volcanic rocks of Bajo Pobre and Chon Aike Formations. δ34S ‰ values of sphalerite, pyrite and galena cluster between 1.3 and 3.8 ‰, suggesting that the sulfur at La Josefina was primarily of magmatic origin. These results are interpreted to indicate that the Jurassic volcanic rocks are closely related with low sulfidation Au-Ag occurrences. Keywords. Pb isotopes, S isotopes, epithermal deposits, Jurassic volcanism, Patagonia Argentina 1 Introduction The Deseado Massif (DM) is located in the southern Argentinean Patagonia (Fig. 1). In this region, the most important unit is a volcanic complex of upper to middle Jurassic age with bimodal features marked by andesitic and rhyolitic magmas that conform the Bajo Pobre and Chon Aike Formations, respectively. These units crop out over more than half the area of a wide plateau. The geochemical analyses of the Jurassic volcanism show a calc-alkaline magmatism with a volcanic arc affinity. These volcanic rocks are related to the early history of the Gondwana break-up and were deposited in the backarc Patagonian Andes during a long period (187 to 144 My) of extension (Riley et al. 2000). The geotectonic environment of Patagonia in the Jurassic times was characterized by very slow subduction in the Pacific margin of Gondwana (Ramos 1988). Pankhurst et al. (2000) support the idea that the volcanic rocks were probably generated by a variety of mechanism, among which the melting of pre-existing continental crust was a dominant process. These volcanic rocks host the Au-Ag veins of Cerro Vanguardia, the principal ore deposit currently in production, and also host the Ag-ore shoot worked in the Marta Mine, as well as some other important prospects like Manantial Espejo, Huevos Verdes-Cerro Saavedra-El Pluma, El Dorado-Monserrat, Cerro Negro and La Josefina. Most of these prospects (Schalamuk et al. 1997) correspond to the low sulfidation epithermal type of deposits. The last prospect, currently under exploration, is located in the central part of the DM and the mineralization is represented by Au-Ag bearing vein systems (up to 300 g Au/t). The objective of this paper is to present the lead and sulfur isotopic data from samples of hydrothermal sulfides and volcanic rocks obtained at the La Josefina prospect. There are few isotopic studies of the DM, only two lead isotope data for the Jurassic volcanic rocks are indicated by Kay and Gorring (1999) and five lead isotope measurements on galena from several ore deposits of the DM were showed by Schalamuk et al. (1997). Theses analyses show isotopic values between 18.48-18.72, 15.73-15.95 and 38.70-39.53 for 206Pb/204Pb, 207Pb/204Pb and 208Pb/204Pb, respectively. Isotope sulfur ratios carried out in samples from AuAg epitermal prospects (Cerro Vanguardia, Manantial Espejo, El Dorado-Monserrat and Cerro León) in the DM, were reported by Echavarría (1997), Schalamuk et al. (1998) and Jovic et al. (2004). The δ34S values range between –2.8 and 4.2 ‰, indicating a magmatic source for the sulfur. 2 La Josefina geology The La Josefina prospect (Fig. 1) includes lower Paleozoic low grade metamorphic muscovitic schists, metavolcanic and calk-silicate rocks with minor magnetitic levels and tourmalinites of La Modesta Formation (Moreira et al. 2005). The Bajo Pobre and Chon Aike Formations represent the Jurassic volcanic rocks. The Bajo Pobre Formation, mainly andesitic-dacitic rocks, include porphyritic and aphanitic flows partially self-brecciated, porphyries, sills that intrude the low angle dip schist of the La Modesta Formation, and ring-dikes surrounding rhyolitic domes. The Chon Aike Formation cover approximately a 60 % of the area. The lower member outcrop on the west part, and consists of crystal-rich quartz-feldspar-biotite welded ignimbrite with some flatten pumice-rich levels that was dated at 153.2 ±3.6 My (K/Ar on biotite; Arribas et al. Close 802 P. Moreira · R.R. Fernández · I.A. Schalamuk · R.O. Etcheverry · A.P. Rolando 1996). On the eastern part dominate a welded pumicerich, crystal-poor welded ignimbrite whose lower levels carrying 5-20 cm crystal-rich-ignimbrite lithic fragments, whereas in the upper levels these lithics are smaller and sporadic. A rhyolitic dome-complex outcrops on 10 km2 in the north-northwest of the area and some smaller rhyolitic domes extend to the northwest, both with slowly propylitic, pyritic and argillic patch of hydrothermal alteration. These domes intruded the Paleozoic metamorphic rocks (La Modesta Formation). Paleogene and neogene basaltic flows cover the Jurassic volcanic rocks. 3 La Josefina Au-Ag epithermal ocurrences The mineralization at the La Josefina prospect consists of system of low sulphidation epithermal veins and veinlets filled mainly by quartz and chalcedony with minor adularia, barite and platy calcite. The primary assemblages are composed by native gold, electrum, specularite and pyrite, arsenopyrite, galena with freibergite inclusions, sphalerite, chalcopyrite and bornite and a supergenic association consist in limonites, chalcocite-covelite, cerusiteanglesite and malachite. These occurrences are distributed in a curved belt about N-S 12 km long and between 500 and 1200 m wide. The age of the mineralization is not well constrained; a Rb-Sr errorchron gave an age of 156 ± 2 My (Fernández et al. 1999). The veins are spatially associated with superficial epithermal occurrences, like hydrothermal eruption breccias, silica sinter terraces, geyserites, carbonate stromatolitic deposits, and steam heated blankets, mainly to the north of the prospect. 4 Samples and results 4.1 Samples The samples collected for the lead isotopic study of the La Josefina prospect consisted in intermediate-acid Jurassic volcanic rock from Bajo Pobre and Chon Aike Formation (feldspar separates) and hydrothermal minerals from veins (pyrite and sphalerite). The isotopic Pb composition were determinate on 13 samples in the Pará-Iso Laboratory, Instituto de Geociencias, Universidade Federal do Pará, Belém, Brazil. Seven sulfide paragenetic samples, including separates of pyrite (3), sphalerite (3), and galena (1), were analyzed for their sulfur isotope composition. Analyses were carried out at the Stable Isotopic Service from Salamanca University (Spain). The results are given as δ34S ‰ values relative to the CDT standard. 4.2 Results The analyses of Pb in samples from La Josefina prospect are summarized in the Table 1 and plotted in the Zartman and Doe (1981) diagrams (Fig. 2). The volcanic Jurassic samples have an average ratios of 206Pb/204Pb= 18.44, 207Pb/204Pb= 15.65 and 208Pb/204Pb= 38.50 and the elongate trends in the general cluster indicate mainly an orogenic model fit, suggesting variable mixing of lead from different sources, mainly model upper crust and to a lesser extent model mantle and lower crust reservoirs. The Pb isotopic compositions of pyrite and sphalerite from La Josefina are near 206Pb/204Pb= 18.48, 207Pb/204Pb= Close Chapter 7-21 · Jurassic magmatism and Au-Ag mineralization in the Deseado Massif (Patagonia Argentina): Lead and sulfur isotopic studies 15.69 and 208Pb/204Pb= 38.61. The lead isotope composition of these sulfides are in general slightly more radiogenic than the volcanic host rocks. The analyses of δ34S ‰ are summarized in the Table 2. Sulfur samples in La Josefina show δ34Smineral values between 1.3 and 3.8 ‰. The δ34S high value for sphalerite (13.1 ‰) demonstrate an overall increase. This could be explained by changes of the hydrothermal fluid pH produced by the interaction with the volcanic rocks. 803 Lead isotopes obtained from galena samples by Schalamuk et al. (1997) although have slightly higher values, do not show significant differences from the samples studied here. The δ34S results in La Josefina are similar to those in several ore deposits in the DM. Based on these features, there is a genetic link between the DM low sulfidation epithermal deposits and the bimodal magmatism of the Bajo Pobre and Chon Aike Formation. Acknowledgements The authors are grateful to the Agencia Nacional de Promoción Científica y Tecnológica (FONCyT) and the Santa Cruz state mining company (FOMICRUZ S.E.) for the support and close cooperation during this research. References 5 Conclusions δ34S The values of pyrite, sphalerite and galena indicate that their sulfur was derived from a magmatic sulfur source with scarce supergene activity. Pb isotope ratios of pyrite and sphalerite, are most similar to those of the volcanic rocks and suggest that they are the likely source. The correspondence of both sets of values with the orogenic growth curve of Zartman and Doe (1981) suggests further that varied sources contributed to the lead of the magma. Arribas Jr A, Schalamuk I, de Barrio R, Fernández R, Itaya T (1996) Edades Radimétricas de Mineralizaciones Epitermales Auríferas del Macizo del Deseado, Provincia de Santa Cruz, Argentina. In: XXXIX Congresso Brasileiro de Geología, pp 254-257 Echavarría LE (1997) Estudio geológico-minero del área El DoradoMonserrat, Departamento Magallanes, provincia de Santa Cruz. Tesis Doctoral Facultad de Ciencias Naturales y Museo, Universidad Nacional de La Plata. Unpublished Fernández R, Echeveste H, Tassinari C, Schalamuk I (1999) Rb-Sr age of the La Josefina ephitermal mineralization and its relation with host volcanic rocks. Macizo del Deseado, Santa Cruz Province, Argentina. In: 2º Simposio Sudamericano de Geología Isotópica, pp 462-465 Close 804 P. Moreira · R.R. Fernández · I.A. Schalamuk · R.O. Etcheverry · A.P. Rolando Jovic SM, Guido D, Tiberi P, Schalamuk I (2004) Cerro Leon, una variación del modelo epitermal de baja sulfuración del Macizo del Deseado. In: VII Congreso de Mineralogía y Metalogenia, pp 225-230 Kay SM, Gorring ML (1999) Evolution of the Patagonian Mantle: evidence from isotopic studies of Tertiary to recent plateau lavas. II South American Symposium on Isotope Geology, pp 556-565 Moreira P, González P, Fernández R, Echeveste H, Schalamuk I, Etcheverry R (2005) El basamento de bajo grado de las Estancias La Modesta y La Josefina, Macizo del Deseado, Provincia de Santa Cruz. Revista de la Asociación Geológica Argentina 60-1 Pankhurst RJ, Riley TR, Fanning CM, Kelley SR (2000) Episodic silicic volcanism in Patagonia and the Antarctic Peninsula: chronology of magmatism associated with the break-up of Gondwana. J Petrol 41: 605-625 Ramos V. (1988) Late Proterizoic-Early Paleozoic of South America. A collisional history. Episodes, 11:168-175 Riley T, Leat P, Pankhurst R, Harris C (2000) Origin of large volume rhyolitic volcanism in Antartic Peninsula and Patagonia by crustal melting. J Petrol 42: 1043-1065 Schalamuk I, Echeveste H, Etcheverry RO, Ametrano S (1998) Metalogénesis del yacimiento “Manantial Espejo”,Macizo del Deseado, provincia de Santa Cruz. In: Academia Nacional de Ciencias Exactas, Físicas y Naturales, Anales 50: 217-236 Schalamuk I, Zubia M, Genini A, Fernández R (1997) Jurassic epithermal Au-Ag deposits of Patagonia, Argentina. Ore Geol Rev 12: 173-186 Zartman RE, Doe BR (1981) Plumbotectonic-the model. Tectonophys 75: 135-162 Close Chapter 7-22 7-22 Re-Os ages for molybdenite from the Tepeoba breccia-centered Cu-Mo-Au deposit, western Turkey: Brecciation-triggered mineralization Hiroyasu Murakami Institute for Geo-resources and Environment, Geological Survey of Japan, AIST, 1-1-1 Higashi, Tsukuba 305-8567, Japan Yasushi Watanabe Institute for Geo-resources and Environment, Geological Survey of Japan, AIST, 1-1-1 Higashi, Tsukuba 305-8567, Japan Holly Stein AIRIE Program, Department of Geosciences, Colorado State University, Fort Collins, CO 80523-1482 USA, and Norges Geologiske Undersøkelse, Leiv Erikssons vei 39, 7491 Trondheim, Norway Abstract. The Tepeoba breccia-centered Cu-Mo-Au deposit is associated with the Miocene Eybek granodiorite complex in western Turkey. The ages for molybdenite samples in the hydrothermal breccia and two molybdenite samples in veins surrounding breccia, one in metasedimentary rocks and one in the granodiorite, were dated by the Re-Os method using a double Os spike. Re-Os ages of molybdenite are 25.03 ± 0.14 and 25.11 ± 0.14 Ma for the veins and 25.62 ± 0.09 Ma for the breccia-hosted sample. These results indicate that the hydrothermal breccia in the Tepeoba deposit formed prior to the vein formation. We conclude, based on the Re-Os ages, that hydrothermal activity at Tepeoba lasted at least half a million years. Keywords. Re-Os, 188Os-190Os double spike, hydrothermal breccia, CuMo-Au deposit, Turkey 1 Introduction Re-Os dating of molybdenite (MoS2) is an effective tool for directly dating mineralization. Notably, molybdenite posses the unique property of accommodating Re at the ppm level, while incorporating essentially no initial (common) Os, thus providing a suitable single mineral chronometer utilizing the 187Re-187Os method (Stein et al. 2001). The 188Os-190Os double spike may be essential for young or low Re molybdenites (Markey et al. 2003). This method can precisely determine and correct for common Os and mass fractionation. The method thus provides a precise mineralization age associated with formation of molybdenite even in young samples with low Re contents. In this study, we report three Re-Os ages of molybdenite, dated by the double Os spike method, in the Tepeoba Cu-Mo-Au deposit in western Turkey. We discuss duration of mineralization and the spatial and temporal evolution of the Tepeoba hydrothermal system. 2 Geologic background Western Turkey is comprised of Permo-Triassic metamorphic and sedimentary rocks (Fig. 1A). A series of intru- sions was emplaced into these basement rocks during the Oligocene and Early Miocene period. A ~24 Ma rapidly exhumed high-grade metamorphic core complex in the Kazdað mountain range was uplifted from ~14 km to ~7 km along a thick shear zone (Okay and Satir 2000). The Eybek granodiorite is situated on eastern margin of the Edremit graben bounded by ENE-WSW trending highangle normal faults. The granodiorite is a typical calcalkaline, I-type, magnetite-series. Granite body with Stype and ilmenite-series signatures occurs locally along the margin of the granodiorite body (Fig. 1B). A two-component mixing pattern of strontium isotope values suggests the “granite” formed by mixing between the granodiorite and the host meta-sedimentary rocks. Early to Middle Miocene volcanic and sedimentary rocks overlie the basement rocks. 3 Tepeoba breccia-centered Cu-Mo-Au deposit The Tepeoba deposit was discovered in 2002, by diamond drilling conducted by the General Directorate of Mineral Research and Exploration of Turkey. A drill hole shows the upper 100 m with an average grade of 0.5 % Cu and ~1 g/t Au, with the upper 53 m at 1 % Cu, and 0.05 % Mo. The deposit occurs along and above the south granite body, located at the southern margin of the Miocene Eybek granodiorite complex. This deposit is hosted by metamorphic and sedimentary rocks of Permo-Triassic age, metamorphosed to andalusite-biotite schist due to the contact metamorphism by the granodiorite. The deposit consists of semicylindrical hydrothermal breccia 200 m wide, and extends for 800 m southwards with a maximum thickness of 100 m (Fig. 1B). This hydrothermal breccia includes fragments of surrounding rocks (e.g., andalusitebiotite schist and granite) except granodiorite in a matrix mainly of phlogopite. The ratio of granite fragments to andalusite-biotite schist fragments is greater nearer to the granite. The breccia ore is composed of chalcopyrite Close 806 Hiroyasu Murakami · Yasushi Watanabe · Holly Stein and phlogopite with accessory molybdenite, pyrite, calcite, quartz, tourmaline, sphalerite, and electrum. In the hydrothermal breccia, post-brecciation hydrothermal activity is limited to thin quartz veining. It has been proposed that the Tepeoba deposit has been tilted almost 90° with its top to the south due to Miocene normal faulting, resulting in full exposure of hydrothermal alteration zones associated with the granodioritegranite complex on the present surface (Murakami et al, 2004). We suggest that alteration and mineralization at Tepeoba resemble types seen at porphyry-style Cu-Mo deposits. The alteration sequence in order of increasing proximity to mineralized breccia is a propylitic zone, muscovite zone, and K-silicate zone. The propylitic and muscovite zones are characterized by the presence of small amounts of chlorite and pyrite, and the presence of muscovite partly replacing biotite and quartz-calcite-molybdenite veins, respectively. These alteration zones surround the breccia dominated by K-silicate alteration, depicted by phlogopite with disseminated chalcopyrite and molybdenite. K-Ar ages for phlogopite in the matrix of the mineralized breccia are 23.8 ±1.2 and 23.8 ±1.4 Ma (hereafter, all ages are shown with two sigma uncertainty), and K-Ar ages for muscovite surrounding the breccia are 22.8 ±1.4, and 24.6 ±1.4 Ma. Ages of the intrusions have also been dated by K-Ar. Biotite in the granodiorite is dated at 20.3 ±1.0 and 21.4 ±1.2 Ma. K-feldspar in the granite is older at 34.7±2.0 Ma. Integration of stable isotope data, together with geologic relations and fluid inclusion data indicate that boiling, high-salinity fluids were responsible for the K-silicate and muscovite alteration and Cu-Mo- Au mineralization is related to the granodiorite intrusion and subsequent brecciation (Murakami et al. 2004). 4 Samples and analytical procedures of Re-Os dating The three molybdenite samples used for Re-Os dating are (A) molybdenite cementing a matrix of a granite-fragment rich hydrothermal breccia, with phlogopite, quartz and chalcopyrite, (B) molybdenite in a hydrothermal calcite-quartz vein in andalusite-biotite schist, and (C) molybdenite in a vein containing chlorite (after igneous biotite) found along cracks in the granodiorite (Fig. 1B). Molybdenite was extracted from these samples in a targeted, occurrence-specific manner using a diamondtipped, slow-speed drill (Stein et al. 2003). Chemical procedures follow Markey et al. (2003). Isotopic compositions were determined using NTIMS on two NBS spectrometers at AIRIE. Age is calculated by applying the equation 187 Os=187Re (eλt-1), where λ is the decay constant for 187Re and t is the age. The 187Re decay constant used is 1.666 · 10-11 yr-1 with an uncertainty of 0.31%. During this study, blanks were Re = 4.77 ± 0.04 pg, total Os = 4.09 ± 0.02 pg, and 187Os/188Os = 0.229 ± 0.002 pg. 5 Relationship between granodiorite and hydrothermal alteration Re-Os and K-Ar ages for hydrothermal minerals, granodiorite and granite from the Tepeoba Cu-Mo-Au deposit are summarized in Figure 2. Close Chapter 7-22 · Re-Os ages for molybdenite from the Tepeoba breccia-centered Cu-Mo-Au deposit, western Turkey: Brecciation-triggered mineralization Re-Os dates are consistently older than all K-Ar dates. The Re-Os system has been shown to remain closed at the scale of the molybdenite phase even through high-grade ductile deformation and metamorphism of a porphyry system (Stein et al. 2004b). On the contrary, the temperatures where minerals begin to lose radiogenic argon are of 300 ± 50 ºC, 350 ± 50 ºC, and the interval ranging from 400 to 470ºC, for biotite, muscovite, and phlogopite, respectively (Dodson and McClelland-Brown 1985). Additionally, K-Ar dates in a contact metamorphic aureole generally reflect cooling ages for the associated intrusion. A pluton showing a close temporal and spatial association with the Eybek granodiorite has a Rb-Sr age of 25 ± 0.4 Ma (Yilmaz and Karacik 2001 and references therein), which is close to the Re-Os molybdenite ages. Therefore, K-Ar ages for biotite in the granodiorite should correspond to final cooling of the granodiorite, and that of hydrothermal minerals rejuvenated due to contact metamorphism. During cooling of the granodiorite, contact metamorphism may cause continuous loss of radiogenic argon from hydrothermal minerals, because the youngest age of granodiorite is accord with that of hydrothermal muscovite. The K-Ar age of the hydrothermal phlogopites is somewhat older than that of muscovite, which is consistent with the observation that phlogopite commonly retains its radiogenic argon better than muscovite at higher temperature (Dodson and McClelland-Brown 1985). 6 Style of Tepeoba mineralization relative to porphyry copper 807 Re-Os ages for molybdenites yield a time-span from 25.62 ± 0.09 to 25.03 ± 0.14 Ma, a period > 0.5 m.y., slightly longer than 0.3 m.y. estimates for the Far Southeast porphyry deposit (Arriibas et al. 1995) and 0.16 m.y. for the Batu Hijau porphyry deposit (Garwin 2002). Recent ReOs dating indicates that some porphyry Cu-Mo deposits have longer mineralization periods (e.g. Los Pelambres, El Teniente, Stein et al. 2004a). Dilles et al. (2004) interpreted extended mineralization at Butte to overprint of multiple mineralization events. There is no syn- or post-hydrothermal activity except a single stage of mineralized breccia at the Tepeoba deposit with a lack of significant veining in the hydrothermal breccia body. Molybdenite of ca. 25.03 Ma also coexists with low-temperature assemblages compare to those in the breccia. These occurrences suggest that the 0.5 m.y.mineralization period of Tepeoba is more likely to represent an extended mineralization event such as pro and retro-grade alteration in skarn type deposit, rather than possible multiple mineralization events. We have determined formation pressure for the granodiorite using plagioclase-hornblende geobarometry. The crystallization pressure is estimated at ~2 kbar. According to geobarometry, if rock density is 2.7 g/cm3, depth of crystallization of the Eybek granodiorite is considered to be ~7.5 km, which is consistent with depth estimates for surrounding metasedimentary rocks (Okay and Satir 2000). Such a deeper depth relative to many other porphyry copper deposits (ca. 1-4 km) may utilize a more static regime for skarn formation (e.g. controlled by diffusion rate rather than infiltration), and to limit hydrothermal activity accompanying mineralization in the vicinity of hydrothermal source without disturbance such as meteoric water circulation. This may be supported by the presence of small-scale skarn type Cu-Fe deposits which are sporadically distributed in and around the Eybek granodiorite at almost the same depth as the Tepeoba deposit. Although a period of hydrothermal activity at the Tepeoba deposit related to the granodiorite and subsequent brecciation is consistent with the time interval for common porphyry-style deposits, there is a huge difference in the scale between these types. This is interpreted that volume and scale of mineralization of intrusion-related style should be controlled by number of cycles of hydrothermal alteration linked to magmatic fluid derived from intramineral intrusion (e.g., giant Cu-Mo porphyry deposits in Chilean Andes). Acknowledgements For porphyry-style Cu deposits, hydrothermal breccia generally forms at the close of major hydrothermal activity, although there are exceptions (e.g. Sillitoe 1985). Based on Re-Os dating results, mineralized hydrothermal breccia at the Tepeoba deposit formed prior to the vein formation. We are grateful to Dr R Sari and Mr S Küçükefe of the General Directorate of Mineral Research and Exploration of Turkey for helping a field survey and providing geologic data of the Tepeoba deposit. Close 808 Hiroyasu Murakami · Yasushi Watanabe · Holly Stein References Arribas AJr, Hedenquist JW, Itaya T, Okada T, Concepción RA, Garcia, JSJr (1995) Contemporaneous formation of adjacent porphyry and epithermal Cu-Au deposits over 300 ka in northern Luzon, Philippines. Geology 23: 337-340. Dilles JH, Stein H.J, Martin MW (2004) Re-Os and U-Pb ages for the duration of the giant Butte, Montana, porphyry Cu-Mo and Cordilleran base metal lode ore deposit. IAVCEI general assembly Pucón, Chile Dodson MH, McClelland-Brown E (1985) Isotopic and paleomagnetic evidence for rates of cooling, uplift and erosion. Geol Soc Mem 10: 315-325 Garwin S (2002) The Geologic Setting of Intrusion-Related Hydrothermal Systems near the Batu Hijau Porphyry Copper-Gold Deposit, Sumbawa, Indonesia, Global Exploration 2002: Integrated Methods for Discovery, Colorado, USA. Soc Econ Geol 9: 333-366 Markey R, Hannah JL, Morgan1 JW, Stein HJ (2003) A double spike for osmium analysis of highly radiogenic samples. Chemi Geol 200: 395-406 Murakami H, Watanabe Y, Sari R, Küçükefe S (2004) Newly discovered Tepeoba breccia-centered Cu-Mo-Au deposit in western Turkey: (electronic, session 1c) IAVCEI general assembly Pucón, Chile Okay A, Satir M (2000) Coeval plutonism and metamorphism in a latest Oligocene metamorphic core complex in northwest Turkey. Geol Mag 137: 495-516 Sillitoe RH (1985) Ore-Related Breccias in Volcanoplutonic Arcs. Econ Geol 80: 1467-1514 Stein HJ, Cannell J, Cooke D, Sillitoe R, Perelló J (2004a) Metalliferous moments inside the lifespan of porphyry-style Cu-Au-Mo deposits: (electronic, session 12a) IAVCEI General Assembly, Pucón, Chile Stein HJ, Hannah JL, Zimmerman A, Markey R, Sarkar SC, Pal AB (2004b) A 2.5 Ga porphyry Cu-Mo-Au deposit at Malanjkhand, central India: implications for Late Archean continental assembly. Precambr Res 134: 189-226 Stein HJ, Markey, RJ, Morgan JW, Hannah JL, Scherstén, A (2001) The remarkable Re-Os chronometer in molybdenite: how and why it works. Terra Nova 13: 479-486 Stein HJ, Scherstén, A, Hannah, JL, Markey R (2003) Sub-grain scale decoupling of Re and 187Os and assessment of laser ablation ICPMS spot dating in molybdenite. Geochim Cosmochim Acta 67: 3673-3686 Yilmaz Y, Karacik Z (2001) Geology of the northern side of the Gulf of Edrem it and its tectonic significance for the development of the Aegean grabens. Geodin Acta 14: 31-43 Close Chapter 7-23 7-23 U-Pb SHRIMP dating of zircon from quartz veins at the Yangshan gold deposit: Evidence for multiple magmatic-hydrothermal events Qi Jinzhong, Li Li, Yuan Shisong, Liu Zhijie Gold Geological Institute of China Armed Police Force, Langfang 065000, China Abstract. The Yangshan gold deposit is a fine-grained disseminated gold deposit located in south Gansu province. The metallogenic age was determined by cathodoluminescence imaging and U-Pb SHRIMP techniques. Zircons associated with quartz veins containing finegrained disseminated gold ore have typical magmatic features including pillar idiomorphism, rhythmic zoning, and Th/U ratio of 0.5 to 1.5. Average 206Pb/238U ages of 197.6 ±1.7 Ma, 126.9±3.2 Ma, and 51.2±1.3 Ma define three primary zircon populations. The former age correlates to K-Ar ages (189.4±7.2 Ma mean) for plagiogranite dikes, while the later two ages suggest buried Cretaceous and Tertiary intrusives in or near the ore field. The Yangshan gold deposit is genetically related to the three magmatic-hydrothermal events. Keywords. Disseminated gold, zircon, quartz vein, SHRIMP dating, Gansu 1 Introduction The recently discovered found Yangshan gold deposit, located in south Gansu province, China, is a large deposit containing fine-grained disseminated gold. Four discovered ore blocks occur in metamorphosed Devonian sandstone, phyllite and limestone. The ore belt is primarily controlled by the Anchanghe- Guanyinba fault as well as small secondary faults. Locally, plagiogranite dikes lie along the fault, and gold mineralization is concentrated in the contact zone between the dikes and the Devonian phyllite. The orebodies, roughly sigmoidal in plane and tabular in profile, are hosted in pyritized, arsenopyritized, sericitized and argillized phyllite and plagiogranite. Late-stage pyrite-quartz veinlets crosscut the orebodies. Native gold, mainly electrum, is found as microscopic to sub-microscopic (<3µm) inclusions in pyrite and arsenopyrite. Previous K-Ar and 39Ar-40Ar dating of the deposit give early Jurassic ages for the plagiogranite dikes, which were spatially associated with the mineralization (Qi 2003). In order to refine the metallogenic age of the Yangshan gold deposit, zircons from quartz veinlets are analyzed using cathodoluminescence images (CL) combined with SHRIMP U-Pb dating. 2 Sample description and experimental method Sample YM is from 305# gold vein in the Caopingliang adit while sample AB from 314# gold vein in the Anba adit. Both samples are from pyrite-quartz veinlets host- ing fine-grained disseminated gold ore. The quartz veinlets (often 1 to 2 cm wide) occur in the contact zone between the plagiogranite dikes and the Devonian phyllite. The samples consist mainly of quartz (95 wt.%) with subordinate sericite and clay minerals (4 wt.%), minor arsenopyrite and pyrite (1 wt.%), and rare electrum. Representative zircon grains from the samples were selected under microscope. The grains together with a slice of standard zircon SL13 and grains of standard zircon TEM from Australia State University were mounted in epoxy, ground, and polished to expose the interior. Cathodoluminescence (CL) images were made on the zircons prior to analyses at the electronic probe laboratory of Institute of Mineral Deposits, CAGS. U, Th, Pb isotopic compositions of zircons were analyzed on a SHRIMP II at the ion probe center of Geological Institute, CAGS. Analyses followed the established methods of Composton et al (1992) and Williams et al (1998). Programs SQUID 1.02 and ISOPLOT were utilized for data processing. Reported uncertainties for U/Pb ratios are at the 1σ level. Common Pb is corrected from measured 204Pb. Weighted mean ages are quoted at the 95% confidence level. 3 Result of SHRIMP dating Fourteen analyses were made on zircon grains from sample YM representing fine-grained disseminated ore. Three age groups are defined and shown in the U-Pb concordia diagram (Fig. 1). The first group consists of three analyses giving 206Pb/238U ages of 195.4 to 200.9 Ma. These zircons are prismatic with concentric zoning (Fig. 3) suggesting a magmatic genesis (Yang 2002; Wu 2002). The second group consists of six analyses yielding 206Pb/238U ages between 121.8 and 137.0 Ma with a 128.2±5.5 Ma mean. These oscillatory zoned zircons are also prismatic (Fig. 3) and regarded as magmatic. The third group consists of four analyses giving 206Pb/238U ages between 48.1 and 51.7 Ma (50.0±3.0 Ma mean). These zircons are also prismatic with clear oscillatory zoning and are interpreted as magmatic (Fig. 3). The remaining analyses are scattered in the diagram. Zircon samples YM-13 and YM-15 are short prisms with concentric zoning yielding 206Pb/238U ages of 1069±22 Ma and 809±17 Ma, respectively. They likely represent Close 810 Qi Jinzhong · Li Li · Yuan Shisong · Liu Zhijie 4 captured zircons from late Proterozoic intrusives. Analysis on zircon YM-12 gives an 206Pb/238U age of 375±11 Ma and might be captured from the Devonian strata. 16 zircons from sample AB representing the quartz veinlet of fine-grained disseminated ore were analyzed. These zircons are small and their common lead concentrations are slightly high. One analysis with significantly high common lead content was rejected. Two age groups were obtained as shown in the U-Pb concordia diagram (Fig. 2). The first group consists of five analyses giving 206Pb/238U ages between 121.4 and 130.2 Ma (125.3±4.9 Ma mean). These zircons are interpreted to be magmatic from their prismatic morphology and oscillatory zoning (Fig. 4). The second group consists of eight analyses which yield 206Pb/238U ages of 49.8 to 55.3 Ma (51.7±1.6 Ma in average). These concentrically zoned zircons are also primsatic (Fig. 4) and regarded as magmatic zircons. Geological significance of the SHRIMP age and discussion With high U-Pb isotope closure temperature of 700 to 750°C (Harrison et al. 1987; Tilton et al. 1991) and a strong resistence to thermal disturbance (Meger et al. 1997), zircon is widely used to constrain the timing of geological events. Although it has been proposed that “hydrothermal zircon” may form at lower temperatures (Corfu et al. 1984; Claoue-long et al. 1990), published ages of “hydrothermal zircons” from quartz veins in some gold deposits are very close to the ages of their host rocks, so whether “hydrothermal zircon” do exist in quartz veins is suspicious (Luo et al. 2000). The relatively low temperature of the hydrothermal fluid (150 to 250oC, Qi et al. 2003) at Yangshan could hardly result in the formation of “hydrothermal zircon”. Furthermore, among the 30 analyses, only 3 zircons have Th/U ratios close to or less than 0.1, indicating that typical metamorphic zircons are not well-developed in the district (Gebauer et al, 1985; Yang J S et al. 2002). Therefore, zircons from the quartz veins in the district should be the ones captured during hydrothermal activity. The zircons may be captured from intrusives (including intrusives in the source area and those near the path of the hydrothermal fluid flow) and those captured from strata (mainly from older rocks that supplied source material to the Devonian strata). Three analyses on zircons from sample YM constitute the first group age, giving the 206Pb/238U ages between 195.4 and 200.9 Ma. Having short prism form with concentric zoning and Th/U ratios of 0.44 to 0.87, these are regarded as Jurassic igneous zircons. As the age is consistent with the whole rock K-Ar ages of five plagiogranite samples in the gold field (171 to 209 Ma, Qi et al. 2003), these zircons may be captured from the plagiogranite dikes. Furthermore, the age coincides with the 39Ar-40Ar plateau age of 195.40±1.05 Ma of the quartz veinlet (Qi et al. 2003), suggesting that the intrusion of the plagiogranite dikes is responsible for hydrothermal activity in the district. Cretaceous and Tertiary zircon groups were detected in samples YM and AB. Analyses revealed eleven Cretaceous zircons yielding an average 206Pb/ 238U age of 126.9±3.2 Ma and twelve Tertiary zircons give an average 206Pb/238U age of 51.2±1.3 Ma. These zircons are prismatic with concentric oscillatory zoning and dominant Th/U ratios between 0.5 and 1.5 indicating their magmatic genesis. These zircons could not be captured from the nearby strata as no Cretaceous or younger strata is found in the district. Furthermore, no intrusives other than the Jurassic plagiogranite are found related to the ore belt suggesting these zircons are captured from buried Cretaceous and Tertiary intrusives. Consequently, after the intrusion of plagiogranite dikes, two major magmatic events occurred in early Cretaceous and in early Tertiary, with a later ore fluid capturing the zircons from the intrusives. Close Chapter 7-23 · U-Pb SHRIMP dating of zircon from quartz veins at the Yangshan gold deposit: Evidence for multiple magmatic-hydrothermal events Therefore, the gold field was influenced by three magmatic and associated hydrothermal events. Comparing Yangshan magmatic-hydrothermal events with the magmatic events in western Qinling, we can see that the early Jurassic hydrothermal epoch coincides with one fastigium of felsic intrusions in western Qinling (190Ma to 220Ma, Zhang et al. 1994), while the early Cretaceous hydrothermal epoch corresponds to another fastigium of granite activities in western Qinling (120Ma to 150Ma, Du et al. 1998). These two epochs were also considered to be the fastigiums of gold mineralization in China (Zhai et al. 2002; Mao et al. 2002). The early Tertiary magmatic-hydrothermal epoch is consistent with the major metallogenic age of gold deposits in southwestern China (Chen et al. 2001), and the magmatic-hydrothermal activity may be linked to 811 the continental-continental collision of the penetrating Indian plate and Eurasian plate. The gold mineralization at Yangshan may be directly linked to multiple, localized magmatic-hydrothermal events in the district and major magmatic-tectonic events in the region. 5 Conclusion 1. Zircons from quartz veinlets associated with ore are dominantly prismatic with concentric oscillatory zoning and Th/U ratios of 0.5 to 1.5 indicating a magmatic genesis. 2. The magmatic zircons with 206Pb/238U ages of 195.4 to 200.9 Ma in quartz veinlet sample YM are captured from the early Jurassic plagiogranite intrusives. Close 812 Qi Jinzhong · Li Li · Yuan Shisong · Liu Zhijie 3. The two zircon groups with average 206Pb/238U ages of 126.9±3.2 Ma and 51.2±1.3 Ma in quartz veinlets are captured from buried Cretaceous and Tertiary intrusives, respectively. The early Jurassic, early Cretaceous, and early Tertiary magmatic-hydrothermal events affected Yangshan gold field and the deposit was genetically related to the three magmatic-hydrothermal events. References Chen YC, Wang DH (2001) Study of Himalayan endogenic mineralization. Bejing: Seismic Publishing House. 1-138 (in Chinese with English abstract) Claoue-long J, King RW, Kerrich R (1990) Archean hydrothermal zircon in the Abitibi greenstone belt: constrains on the timing of gold mineralization. Earth Planet Sci. Letters 98:109-128. Composton W, Williams IS, Kirschvink JL, Zhang Z, Ma G (1992) Zircon U-Pb ages for the Early Cambrian time scale. Journal of the Geological Society London 149:171-184. Corfu F, Ayres LD (1984) U-Pb age and genetic significance of heterogeneous zircon populations in rocks from the Favourable Lake area, Northwestern Ontario. Contrib Mineral Petrol 88: 86-101 Du ZT, Wu GG (1998) Study on tectonic systems and gold metallogenic tectono-dynamics in the region of west Qinling. Bejing: Geological Publishing House. 1-145 (in Chinese with English abstract) Gebauer D, Lappin MA, Grunenfelder M (1985) The age and origin of same Norwegian eclogite: A U-Pb zircon and REE study. Chemical Geology 52: 227-248 Harrison TM, Aleinkoff JN, Compston W (1987) Observation and controls on the occurrence of inherited zircon in concord-type granitoids, New Hampshire. Geochem Cosmochim Acta5 1: 2549-2568 Luo ZK, Miao LC, Guan K (2000) Discussion on the metallogenetic epoch of gold deposit on north fringe of North China platform, Gold Geology 6: 70-75 (in Chinese with English abstract) Mao JW, Qiu YM, Goldfarb RJ, Zhang Z, Garwin S, Fengshou R (2002) Geology, distribution, and classification of gold deposits in the western Qinling belt, central China, Mineralium Deposita 37:352-377 Mezger K, Krogstad E J (1997) Interpretation of discordant U-Pb zircon ages: An evaluation. J. Metamorphic Geol. 15:127-140 Qi JZ, Yuan SS, Li L, Sun B, Guo JH (2003) Geological and geochemical study of yangshan gold deposit, gansu province. Mineral Deposits. 22:24-31 (in Chinese with English abstract) Tilton GR, Schreyer W, Schertl HP (1991) Pb-Sr-Nd isotopic behavior of deeply subducted crustal rocks from the Dora Maira massif, Western Alps, Italy-II: what is the age of the ultra-high pressure metamorphism? Contrib. Mineral. Petrol, 108:22-33 Williams I S. (1998) U-Th-Pb Geochronology by Ion Microprobe, in McKibben MA, Shanks III WC and Ridley WI (eds), Applications of microanalytical techniques to understanding mineraling processes. Reviews in Economic Geology 7:1-35. Wu CL, Jone W, Yang JS, Li HB (2002) margin of Qilian mountains: evidence from zircon SHRIMP age of the Aolaoshan granite, Acta Geologica Sinica, 76(1): 118-125 Yang JS, Xu ZQ, Wu CL, Liu FL, Shi RD, Wooden J, Maruyama S (2002) SHRIMP U-Pb dating on coesite bearing zircon: Evidence for Indosinian ultrahigh-pressure metamorphism in Su-Lu, East China, Acta Geologica Sinica, 76(3): 354-372 (in Chinese with English abstract) Zhai YS, Miao LC, Xiang YC, Deng J, Wang JP (2002) Preliminary discussion on ore-forming system in greenstone belt-type of north China Craton. Earth Science-Journal of China University of Geosciences. 27: 522-529 (in Chinese with English abstract). Zhang BR, Gao S, Luo TC (1994) Lithosphere structure of Qinba area and metallogenic geochemistry. Wuhan: Publishing House of China University of Geosciences. 1-446 (in Chinese with English abstract) Close Chapter 7-24 7-24 87Sr/86Sr, 3He/4He, REE and stable isotope (δ δ 34S, δ 18O) δ δ constraints on the hydrothermal fluid evolution of the PACMANUS system, Manus Basin Stephen Roberts School of Ocean and Earth Science, Southampton Oceanography Centre, University of Southampton, Southampton, SO14 3ZH, UK Wolfgang Bach Department of Marine Chemistry and Geochemistry, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA Adrian Boyce Scottish Universities Environmental Research Centre, Scottish Enterprise Technology Park, Rankine Avenue, East Kilbride, G70 0QF, UK Ray Burgess Department of Earth Sciences, University of Manchester, Manchester, M13 9PL, UK Abstract. δ34S, 87Sr/86Sr, δ18O, REE and 3He/4He analyses of anhydrite from the PACMANUS hydrothermal system suggest a complex interplay between hydrothermal fluid, magmatic fluid, and seawater during alteration and mineralization. These new data significantly expand the subsurface data on seafloor hydrothermal systems and may begin to explain the earliest processes of multistage mineralization and alteration history that typify ancient massive sulfide systems. Keywords. Hydrothermal vents, sulfides, anhydrite, isotopes 1 The 87Sr/86Sr and δ34S data for anhydrite from Snowcap (Site 1188) and Roman Ruins (Site 1189) suggest contrasting fluid evolution and flow regimes. The rare-earth element (REE) contents of anhydrite from PACMANUS show extreme variability, in terms of both absolute concentrations (e.g., 0.08–28.3 ppm Nd) and pattern shape (LaN/SmN=0.08–3.78, SmN/YbN=0.48–23.1, Introduction Ocean Drilling Program Leg 193 investigated two sites of hydrothermal activity along the crest of the Pual Ridge in the eastern Manus Basin. A site of low-temperature diffuse venting, Snowcap (Site 1188), and a high-temperature black smoker site, Roman Ruins (Site 1189), were drilled to depths of 386 and 206 meters below sea floor, respectively (Binns et al. 2002; Roberts et al. 2003; Bach et al. 2003; Vanko et al. 2004). Although the two sites are <1000 m apart, the geochemical signatures of anhydrite recovered at both sites are very different. Measured anhydrite 87Sr/86Sr ratios vary between 0.7050 and 0.7086; the most radiogenic values occur just beneath the variably altered dacitic cap at both sites (Fig. 1). At Snowcap (Site 1188) there is a clear trend downhole to less radiogenic 87Sr/86Sr values, from 0.7086 beneath the dacite cap to values of 0.7060 at ~100 mbsf, and these low values are broadly maintained to the base of the hole. The measured anhydrite δ34S values vary between 18.1‰ and 22.5‰. For Snowcap, most of the values are less than 21.0‰ and trend significantly toward lower values downhole. In contrast, anhydrite δ34S values at Roman Ruins are mostly equal to or greater than the seawater value and show no obvious downhole trends. Close 814 Stephen Roberts · Wolfgang Bach · Adrian Boyce · Ray Burgess Eu/Eu*=0.59–6.1). The range of REE patterns in anhydrite includes enrichments in the middle and heavy REEs and variable Eu anomalies (Fig. 2a,b). The REE patterns of anhydrite from hole 1188 differ markedly from those of anhydrite recovered during ODP Leg 158 from the TAG hydrothermal system at the Mid-Atlantic Ridge, which display uniform LREE-enriched patterns, in contrast the 1189 data are more comparable. The anhydrite and sulfides from both sites show variable 3He/4He ratios with R/Ra in the range 0.29-6.91 (R/Ra Seawater = 1.05) (Fig. 3). The data show correlations with depth, δ34S and 87Sr/86Sr data. Oxygen isotope data for the anhydrite are relatively uniform, δ18O varies between 8 and 10‰, and show no downhole correlation. 2 Discussion The Snowcap data are consistent with higher sulfate concentrations of the hydrothermal end-member fluid. If the sulfate concentration is increased because of magmatic SO2 disproportionation and dissociation, it would predict a lower fluid pH. This is consistent with the dominance of pyrophyllite at Snowcap and secondary feldspar at Roman Ruins. Furthermore, Bach et al. (2003) have suggested that the range of REE patterns in the anhydrites from Snowcap reflects the waxing and waning input of magmatic volatiles (HF, SO2) and variable complexation of REEs in the fluids. Taken together, these observations strongly suggest a magmatic contribution to the hydrothermal system drilled at Snowcap. In contrast, Roman Ruins data are characterized by 87Sr/86Sr ratios of ~0.7065, with significant intrasample variation, and δ34S ratios that are at seawater or slightly elevated values. The 87Sr/86Sr and S isotope data show no systematic downhole trends and are very similar to data reported for anhydrites recovered during the TAG drilling, ODP Leg 158 and are consistent with the mixing of a low-sulfate hydrothermal fluid and seawater. Close δ 34S, δ 18O) constraints on the hydrothermal fluid evolution of the PACMANUS system, Manus Basin Chapter 7-24 · 87Sr/86Sr, 3He/4He, REE and stable isotope (δ 815 Overall, the data suggest a complex interplay among hydrothermal fluid, magmatic fluid, and seawater during alteration and mineralization of the PACMANUS system. References Bach W, Roberts S, Vanko DA, Binns RA, Yeats CJ, Craddock PR, Humphris SE (2003) Controls of fluid chemistry and complexation on rare earth element contents of anhydrite from the PACMANUS subseafloor hydrothermal system, Manus Basin, Papua New Guinea. Mineralium Depos, 38: 916-935 Binns RA, Barriga FJAS, Miller DJ (2002) Proc. ODP, Init. Repts., 193 [CD-ROM]. Available from: Ocean Drilling Program, Texas A&M University, College Station TX 77845-9547, USA Roberts S, Bach W, Binns RA, Vanko DA, Yeats CJ, Teagle DAH, Blacklock K, Blusztajn J.S, Boyce AJ, Cooper MJ, Holland N, McDonald B (2003) Contrasting evolution of hydrothermal fluids in the PACMANUS system, Manus Basin: The Sr and S isotope evidence. Geology 31: 805-808 Vanko DA, Bach W, Roberts S, Yeats CJ, Scott SD (2004) Fluid inclusion evidence for subsurface phase separation and variable fluid mixing regimes beneath the deep-sea PACMANUS hydrothermal filed, Manus Basin back arc rift, Papua New Guinea. J Geophys Res 109: B03201-03214 Close Close Chapter 7-25 7-25 U-Pb dating of micro-inclusions: The age of the Ehrenfriedersdorf tin deposit (Erzgebirge, Germany) R.L. Romer, R. Thomas GeoForschungsZentrum Potsdam, Telegrafenberg, D-14473 Potsdam, Germany Abstract. Multiple reworking of ore deposits may disturb geochronologic systems and eventually render incorrect ages for ore deposition or different stages of ore formation. Micro-inclusions may beprotected from later disturbances by their host mineral and, thus, yield reliable age information. Major problems in dating micro-inclusions include their genetic connection with various stages of ore formation and technical aspects, such as loss of daughter isotopes by α-recoil and the initial isotopic composition of the daughter element. The problem of daughter-loss from a high-µ microinclusion (µ = 238U/204Pb)by α-recoil can be avoided by analyzing the inclusion together with its low-µ host. The philosophy behind the presented analytical approach is to “trade” radiogenic composition of the daughter element (i.e., high 206Pb/204Pb, 207Pb/204Pb, and 208 Pb/204Pb) against closed-system behavior. This approach is demonstrated for <10 microns small uraninite inclusions in darkmica from Ehrenfriederdorf, Erzgebirge, Saxony. Our data demonstrate that micro-inclusions may yield precise and accurate age data for early ore forming processes. Keywords. Micro-inclusions, U-Pb dating, Ehrenfriederdorf, tin deposits 1 Introduction Precise and accurate dating of many kinds of ore deposits is problematic because later hydrothermal and tectonic overprint (resulting in the repeated redistribution of elements or the introduction of various metals at different time) may disturb geochronometers that are genetically and texturally related to early stages of deposit formation. For instance, U deposits in the Aue-Niederschlema district (Erzgebirge, Saxony) yield ages of c. 280-270 Ma, 190 Ma, 120 Ma, 80 Ma, and 30 Ma (Förster 1996), the oldest age related with the introduction of U into the deposit, the younger ages reflecting redistribution of U in conjunction with multiple tectonic reactivation of the Gera-Jachymov zone, along which numerous U deposits occur. Many of the ambiguities and complexities arising from the redistribution of the ore metals during multiple overprint and alteration can be avoided by (i) dating the economically interesting minerals, which is possible for minerals of the columbite-tantalitetapiolite series (e.g. Romer and Wright 1992; Romer and Smeds 1996), molybdenite (e.g. Stein et al. 1998, 2001; Stein and Bingen 2002), and U-minerals (e.g. Ludwig and Simmons 1991; Förster 1996), (ii) by dating minerals that have formed cogenetically with the economically interesting minerals, which for skarn ores may involve titanite, vesuvianite, and garnet (e.g., Romer 1992; Romer and Soler 1995) and for hydrothermal vein deposits may involve gangue minerals such as white mica or quartz (e.g. Franzke et al. 1996; Romer and Linnemann 2004), and (iii) by dating fluid inclusions in economically interesting minerals or associated gangue minerals (e.g. Glodny 1997; Pettke and Diamond 2000). In this paper, we demonstrate that U-Pb dating of microinclusions is technically possible and yields accurate results as long as precautions are taken (i) to avoid microminerals along grain-boundaries and fractures and (ii) to sample in a way that compensates for recoil-related open-system behavior in the U-Pb system. 2 Advantages and disadvantages of the use of micro-inclusions in mineral dating Dating micro-inclusions entirely enclosed in other minerals has the advantage that the host prevents interaction of the micro-inclusion with later fluids. The host-mineral represents a container that makes the geochronologic system of the inclusion behave as a closed system even for inclusions (e.g., uraninite) that are known to react readily with fluids. The host mineral, however, should neither react with the inclusion nor incorporate those elements that define the geochronologic system of the inclusion. Otherwise there may be exchange of the geochronologically relevant element between host and inclusion. The major problem in the use of micro-inclusions for dating originates from ambiguities in the genetic connection between inclusion and host and the representativity of the inclusion. 3 Requirements on micro-inclusions to be suitable for dating There are basically three requirements that must be fulfilled for micro-inclusions to become potentially attractive for dating attempts: (i) closed system, (ii) strong daughter-to-parent (D/P) fractionation, and (iii) high P contents. i. Closed system behavior requires that neither the P nor the D element is lost from the inclusion. Major processes for possible daughter loss include diffusion and recoil, both of which are more likely to become more important for smaller grain size. Loss by diffusion de- Close 818 R.L. Romer · R. Thomas pends not only on temperature, the diffusion constant of the considered element, the cooling history of the sample, and the distance to the grain surface, but also on the transport of the lost ions away from the grain surface. If a host that does not accept ions lost from the inclusion, these ions will concentrate at the contact between the two minerals and prevent additional loss from the inclusion. An example for an inclusion that remained a closed system to high temperature has been presented by Kühn et al. (2000). They showed that biotite in Sveconorwegian granulite-facies garnet recorded this older event rather than the Caledonian eclogite facies overprint. α-recoil refers to the displacement of the daughter isotope due to the emission of an α-particle (Fig. 1). The daughter nucleus typically is displaced by some 20 to 30 nm (e.g., Matzke 1982). At the contact between a high-µ phase and a low-µ phase, the loss of daughter isotopes from the high-µ phase is more important than the addition of daughter isotopes. Thus, the high-µ phase eventually shows a deficit in daughter isotopes and the low-µ phase shows an excess (cf. Ludwig 1978; Mattinson et al. 1996; Romer 2001, 2003). This effect becomes more important, the smaller the high-µ phase (cf. Romer 2003). Because of α-recoil, isolated small high-µ inclusions are beyond doubt open systems showing a daughter deficit. The same inclusion and its immediate host in combination, however, may represent a closed system as the daughter isotopes lost from the inclusion are collected in the host. This behavior is shown in Figure 1. Note that the isolated inclusion would fall below the concordia and the separated host would fall above the concordia. ii. High P/D values result with time in highly radiogenic D-element compositions, which makes uncertainties about the initial composition of D irrelevant for the age calculation and allows to constrain the slope of an isochron more closely, i.e., to deduce more precise ages. High P/D are restricted to element-pairs of contrasting geochemical behavior, such as Rb-Sr, U-Pb, and Th-Pb and to mineral phases that strongly prefer P over D. iii. Analytical uncertainties originating from counting statistics depend on signal intensity. To obtain small uncertainties, the signal has to be strong, i.e., many ions have to be available for counting. For small inclusions to yield high signal intensities, the content of D has to be high, which is a function of time and P. Thus, for an optimal analytical result, P has to be high. Only few phases fulfill above three requirements. For the U-Th-Pb systems, minerals that have high P/D and high P contents include xenotime, monazite, and uraninite; for the Rb-Sr system, the requirements may be fulfilled by micas and Rb-rich phases. To obtain a closed system, the inclusions should be analyzed together with their host. Thus, the host should yield very low or no contributions of P and D to the bulk sample. 4 High-µ inclusions (monazite, xenotime, and uraninite) Because of alpha-recoil, micro-inclusions are notoriously open systems. Separating inclusions results in too young apparent 206Pb/238U ages as there is a deficit in radiogenic Pb. Drilling the inclusions together with a rim of their host directly from thin sections solves the problem. (i) Recoiled daughter isotopes are collected by the host. (ii) U-rich and Th-rich minerals are readily recognized by their pleochroitic haloes (Fig. 2) and can be iden- Close Chapter 7-25 · U-Pb dating of micro-inclusions: The age of the Ehrenfriedersdorf tin deposit (Erzgebirge, Germany) tified by micro-Raman. For sampling, special care should be taken to collect only inclusions that are entirely enclosed in the host. Outcropping inclusions always show a deficit in radiogenic Pb. (iii) The radius of pleochroitic haloes is more than 100 times larger than the distance of recoil displacement of U-daughters. Thus, drilling samples that include the entire pleochroitic halo must yield closed systems. In thoroughly altered or multiply overprinted rocks, inclusions that are protected by their host mineral from interaction with late fluids may represent the only datable minerals from the early evolution of the altered rock. 5 Uraninite inclusions in mica from the Ehrenfriederdorf tin deposit Extensive high-temperature Sn-mineralizations that form skarns, pegmatites, greisen, and pneumatolyitc- hydrothermal vein deposits are closely associated with Late Variscan granites in the Ehrenfriedersdorf-Geyer area (cf. Oelsner 1952). The granite is dominated by quartz, alkali-feldspar, plagioclase (<An12), and up to 5 vol-% mica. Accessory minerals include topaz, cassiterite, zircon, monazite, xenotime, uraninite, apatite, tourmaline, and Sn-rich pyrrhotite. Melt inclusions in topaz prove that this mineral is magmatic and did not form during pneumatolytic or hydrothermal overprinting. High Sn contents (up to 800 ppm) in melt inclusions in quartz demonstrate that 819 the granite is closely related with the formation of the Sn deposits in the marginal greisen and skarns (Thomas et al. 2003). The radioactive elements U and Th are predominantly hosted in tiny crystals of zircon, uraninite, monazite, and less common xenotime that are readily recognized as they show distinctive pleochroitic haloes in mica (Fig. 2). The small crystal size of the radioactive minerals and the distinctive pleochroitic haloes are typical for most late Variscan granites of the Ehrenfriedersdorf-Geyer district. We analyzed three uraninite inclusions that gave concordant data (filled symbols, Fig. 3). The best age estimate, obtained from the weighted mean of the 206Pb/238U ages, is 323.9±3.5 Ma (2sigma). It falls within the expectation range for these post-kinematic granites, which is defined by 40Ar/39Ar ages of intruded metamorphic rocks and the age of tectonically comparable granites from Fichtelgebirge, Oberpfalz, and the Bavarian Forrest (e.g., Werner and Lippolt 2000; Siebel et al. 2003). The age also agrees well with chemical ages obtained on uraninite, monazite, and xenotime from numerous geochemically corresponding granites of the Erzgebirge (Förster et al. 1999). Thus, our data demonstrate that complete dissolution of inclusion and host yields concordant data that give accurate age constraints. Data from samples with incompletely dissolved monazite and xenotime (open symbols, Fig. 3) show an excess of radiogenic Pb that represents Pb implanted by α-recoil into the host. Close 820 R.L. Romer · R. Thomas References Förster B (1996) U/Pb Datierung an Pechblenden der U-Lagerstätte Aue-Niederschlema (Erzgebirge). Dissertation, Universität Giessen Förster H-J, Tischendorf G, Trumbull RB, Gottesmann B (1999) Late-collisional granites in the Variscan Erzgebirge, Germany. J Petrol 40: 1613-1645 Franzke HJ, Ahrend H, Kurz S, Wemmer K (1996) K-Ar Datierungen von Illiten aus Kataklasiten der Flossbergstörung im südöstlichen Thüringer Wald und ihre geologische Interpretation. Z geol Wiss 24:441-456 Glodny J (1997) Der Einfluß von Deformation und fl uidinduzierter Diaphthorese auf radioaktive Zerfallssysteme in Kristallingesteinen. Dissertation, Universität Münster Kühn A, Glodny J, Iden K, Austrheim H (2000) retention of Precambrian Rb/Sr phlogopite ages through Caledonian eclogite facies metamorphism, Bergen Arc Complex, WNorway. Lithos 51: 305-330 Ludwig KR (1978) Uranium-Daughter Migration and U/Pb Isotope Apparent Ages of Uranium Ores, Shirley, Basin, Wyoming. Econ Geol 73: 29-49 Ludwig KR, Simmons KR (1991) U-Pb dating of uranium ores in collapse-breccia pipes, Grand Canyon region. In: Pagel M, Leroy JL (eds) Source, transport and deposition of metals. A.A. Balkema, Rotterdam, pp 405-408 Mattinson JM, Gaubard CM, Parkinson DL, McLelland WC (1996) U-Pb reverse discordance in zircons: the role of fi ne-scale oscillatory zoning and sub-microscopic transport of Pb. Am Geophys Union Geophys Monogr 95: 355-370 Matzke H (1982) Radiation damage in crystalline insulators, oxides and ceramic nuclear fuels. Rad Effects 64: 3-33 Nasdala L,Wenzel M,Vavra G, Irmer G,Wenzel T, Kober B (2001) Metamictisation of natural zircon: Accumulation versus thermal annealing of radioactivity-induced damage. Contrib Mineral Petrol 141: 125-144 Oelsner O (1952) Die pegmatitisch-pneumatolytischen Lagerstätten des Erzgebirges mit Ausnahme der Kontaktlagerstätten. Freib Forschh 9: 80 pp Pettke T, Diamond LW (2000) Rb-Sr Dating of Sphalerite based on fl uid inclusion-host mineral isochrons: A clarifi -cation of why it works. Econ Geol 91: 951-956 Romer RL (1992) Vesuvianite — a new tool for the U-Pb dating of skarn ore deposits. Mineral Petrol 46: 331-341 Romer RL (2001) Isotopically heterogeneous initial Pb and continuous 222Rn loss in fossils: The U-Pb systematics of Brachiosaurus brancai. Geochim Cosmochim Acta 65: 4201-4213 Romer RL (2003) Alpha-recoil in U-Pb geochronology: effective sample size matters. Contrib Mineral Petrol 145: 481-491 Romer RL, Linnemann U (2004) U-Pb dating the Schlottwitz agate-amethyst vein (Erzgebirge, Saxony). Eur J Mineral 16 (Beiheft 1): 116 Romer RL, Smeds S-A (1996) U-Pb columbite ages of pegmatites from Sveconorwegian terranes in southwestern Sweden. Precambr Res 76: 15-30 Romer RL, Soler A (1995) U-Pb age and lead isotopic characterization of Au-bearing skarn related to the Andorra granite (central Pyrenees, Spain). Mineral Deposita 30: 374-383 Romer RL, Wright JE (1992) U-Pb dating of columbites: a geochronologic tool to date magmatism, metamorphism, nand ore deposits. Geochim Cosmochim Acta 56: 2137-2142 Siebel W, Chen F, Satir M (2003) Late-Variscan magmatism revisited: new implications form Pb-evaporation zircon ages on the emplacement of redwitzites and granites in NE Bavaria. Int J Earth Sci 92: 36-53 Stein HJ, Bingen B (2002) 1.05-1.01 Ga Svenconorwegian metamorphism and deformation of the supracrustal sequence at Saesvatn, South Norway: Re-Os dating of Cu-Mo Mineral occurances. In: Blundell DJ, Neubauer F, von Quadt A (eds) The timing and location of major ore deposits in an evolving orogen. Geol Soc London Spec Publ 204: 319-335 Stein HJ, Markey RJ, Morgan JW, Hannah JL, Schersten A (2001) The remakable Re-Os chronometer in molybdenite: how and why it works. Terra Nova 13: 479-486 Close Chapter 7-26 7-26 U-Pb data of Au-Pd-Pt-bearing quartz-hematite veins, Quadrilátero Ferrífero, Minas Gerais, Brazil R.L. Romer, V. Lüders GeoForschungsZentrum Potsdam, Telegrafenberg, 14473 Potsdam, Germany D.A. Banks School of Earth Sciences, University of Leeds, Leeds, LS2 9JT, UK J. Schneider Inst. Geowissenschaften und Lithosphärenforschung, Universität Gießen, 35390 Gießen, Germany Abstract. Fluid inclusions hosted in specular hematite from auriferous (jacutinga) and barren veins in the Quadrilátero Ferrífero either contain fluid inclusions assemblages of high-temperature aqueouscarbonic and multiphase high-salinity, high-temperature aqueous inclusions or multiphase aqueous fluid inclusions showing narrow ranges of salinity and homogenization temperatures. Fluid inclusions in quartz and hematite are characterized by uniform Na/K ratios and considerable SO4 contents indicating similar formation conditions and perhaps fluid origin from a common source. The formation of specular hematite veins may be related to retrograde metamorphic fluids being released during the Brazilian orogenic cycle (600-700 Ma). The Pb isotopic characteristics of all jacutinga-type samples is readily reconciliated in a simple model that (i) involves different Palaeoproterozoic or Archaean source lithologies for lead and gold and that (ii) possibly reflects contrasting depths of fluid percolation during the Braziliano orogeny and (iii) heterogeneous Au distribution in the greenstone source. Keywords. Fluid inclusions, U-Pb, jacutinga, Au-Pd-Pt, Minas Gerais 1 Introduction 2 Results Fluid inclusions have been studied in specular hematite from two auriferous jacutinga-style mineralization and two barren hematite veins using infrared microscopy. Hematite from barren veins of the Fábrica and Córrego do Feijão iron ore mines contain only one compositional type of fluid inclusions. These are aqueous inclusions with a vapour bubble and with more than 90% having one or more solid phases. Hematite-hosted fluid inclusions from the jacutinga style mineralization of Gongo Soco are similar to those of barren veins. Hematite from jacutinga-style mineralization at Itabira contain two compositional types of fluid inclusions, (i) aqueous carbonic inclusions, and (ii) multiphase aqueous inclusions with at least one solid phase. Both types of inclusions occur together in isolated clusters or as isolated fluid inclusion pairs within individual samples. Two-phase and multiphase aqueous inclusions with solid phases in specular hematite from jacutinga veins of Palladian gold mineralization is unusual worldwide and only Brazilian occurrences are of economic importance. In the Quadrilátero Ferrífero of Minas Gerais, which includes Paleoproterozoic clastic and chemical sedimentary sequences (Minas Supergroup) underlain by an Archean greenstone belt (Riodas Velhas Supergroup) and granitegneiss terrains (Fig. 1), the auriferous portions of itabirites have traditionally been denoted as jacutinga. This peculiar mineralization occurs as Au-Pd-Pt-bearing quartzspecular hematite veins crosscutting the metamorphosed host itabirites. The gold is coarse-grained and commonly black (ouro preto) due to coatings of Pd-O species and Feoxyhydroxide. A number of jacutinga-style gold deposits were worked in the 18 th and 19 th centuries in the Quadrilátero Ferrífero. Openpit iron ore mining-operations have exposed sections of jacutinga mineralization. Gold is currently an intermittent by-product of iron ore mining at Gongo Soco (several tens of kg Au per year) and Itabira, where gold production amounted to about 600 kg Au per year in 2000. Close 822 R.L. Romer · V. Lüders · D.A. Banks · J. Schneider the Gongo Soco mine as well as from barren veins show narrow ranges of salinity between 7.2–11.7 wt.% NaCl equiv. and homogenization temperatures between 148 and 229°C (Fig. 2). Fluid inclusions in specular hematite from the Itabira area are comparatively more complicated. The ice melting temperatures of multiphase aqueous inclusions cover a wide range between -26.1 and -10.7°C (Fig. 2). The majority of the homogenization temperatures of multiphase aqueous inclusions range between 317 and 365°C (Fig. 2). In contrast, aqueous carbonic inclusions have considerably higher total homogenization temperatures when compared with multiphase aqueous inclusions and higher ice melting temperatures (Fig. 2). Crush-leach analyses on samples of quartz and hematite show that Cl and SO4 are the major anions in the fluid inclusions. The fluids are dominated by Na and show significant but variable amounts of K and Ca, and lesser amounts of Mg and Li. The low Cl/Br and Na/Br ratios of the analyzed inclusions are indicative of halite dissolution and reprecipitation by a halite saturated fluid. During dissolution and reprecipitation, Br is excluded from halite and enriched in the fluid, just as during halite precipitation from seawater. The salinity of the fluid inclusions, however, is below halite saturation and indicates dilution after they have gained Br by interaction with halite. The Na/K ratios of the analysed fluids fall into the narrow range (mean 4.5±2.2). The Na/K ratios in brines are likely to be controlled by equilibrium reactions with alkali feldspars and muscovite. Therefore, the elevated K and Li concentration in the fluids are likely to derive from water-rock interaction between the ore-forming fluids and granites and/ or gneisses of the crystalline basement. 3 U-Pb systematics of hematite and gold 3.1 Hematite The Pb isotope data of the hematite samples scatter widely in the 206Pb/204Pb – 207Pb/204Pb, 206Pb/204Pb–208Pb/204Pb, and 206Pb/204Pb–238U/204Pb diagrams (Fig. 3a-c). The data do not define isochrons. Although the scatter among samples from individual deposits is smaller than for the entire data set, there is significant excess scatter, which may originate from (i) initial isotopic heterogeneity within single deposits and contrasting Pb composition in different deposits, (ii) addition of isotopically distinct Pb at some time after formation of the deposits, and (iii) fractionation between U and Pb (modification of the 238U/ 204Pb ratio) during a later event. Furthermore, there may have been some redistribution of radiogenic Pb between hematite host and fluid inclusions by recoil. These potential non-idealities make the derivation of a precise age impossible. Nonetheless, the Pb isotope systematics of the fluid-free hematite samples imposes several constraints on the evolution of the hematite deposits. (1) The data fall in a triangular area in the 206Pb/204Pb–207Pb/204Pb diagram (shaded area, Fig. 3a), which may reflect a heterogeneous source or a poly-stage evolution of the hematite veins. The steepest 207Pb/206Pb trend corresponds to a mixing line of Pb that evolved from ca. 2.7 Ga to 1.9-2.0 Ga. Since the sampled jacutinga–style veins are hosted by Palaeoproterozoic itabirite-type iron deposits, variations along the 2.7-1.9 Ga trend possibly reflects derivation of Pb from an isotopically heterogeneous source during the Palaeoproterozoic formation of the iron deposits. (2) In the 206Pb/ 204Pb– 238U/ 204Pb isochron diagram (Fig. 3c), most data scatter about a linear trend, whose slope corresponds to an age of c. 635 Ma. This age has no strict geochronological meaning as the requirements for an isochron (common initial, single stage evolution) are not met. There are numerous samples that fall above this Palaeozoic reference line, which either implies that these samples had a more radiogenic initial Pb isotopic composition (dashed line, Fig. 3c) or that they record an older age. (3) Hematite from each deposit shows a relatively narrow range in 208Pb/204Pb, but shows distinct differences between deposits (Fig. 3b). (4) The initial Pb isotopic composition of all deposits is characterized by 207Pb/204Pb values, which implies that the initial Pb of the hematite deposits was dominantly derived from an old crust. 3.2 Gold The Pb isotopic composition of gold flitters from jacutinga veins at Gongo Socco align along the steep trend in the 206 Pb/204Pb–207Pb/204Pb diagram (Fig. 3a) with some samples being displaced to the right of this trend. In situ Pb growth (shift to the right) was insignificant for most Close Chapter 7-26 · U-Pb data of Au-Pd-Pt-bearing quartz-hematite veins, Quadrilátero Ferrífero, Minas Gerais, Brazil 823 samples. The Pb from the gold samples is distinctive by its higher 207Pb/204Pb and lower 208Pb/204Pb values (at comparable 206Pb/204Pb) than the hematite samples (Figs. 3a and 3b), the itabirites, or the wall-rocks. This implies that trace Pb in gold may have been derived from a different source than the iron. Hematite from the barren deposit Córrego do Feijão is in its 208Pb/204Pb signature closest to the host-rocks and the itabirite deposits, whereas hematite from the Au-bearing jacutinga-style veins have 208Pb/ 204 Pb values that are closer to the signature of Au. 4 Discussion Specular hematite ores from barren veins and Au-Pd-Ptbearing jacutinga–style mineralization at Gongo Soco were deposited from fluids that show narrow ranges of salinity and homogenization temperatures. This may be due to similar formation conditions or fluid origin from a common source, although the barren veins do not contain Au, Pd, and Pd. Crush-leach analyses demonstrate Cl and SO4 to be the major anions in the ore-forming fluids. The high sulfate concentrations of the analyzed fluids may also be derived by leaching of evaporites (gypsum). The formation of schistose high-grade specular hematite veins at Itabira can be related to acid Cl-SO4-CO2 retrograde metamorphism fluids that interacted intensively with crystalline rocks. The absence of CO2 in hematite-hosted inclusions from veins in the low-strain domain may be attributed to carbonate precipitation or conversion of CO2 to bicarbonate due to cooling during fluid migration from the highto low-strain domain. A Brasiliano age can be derived from the 238U/204Pb–206Pb/204Pb diagram (Fig. 3c) where specular hematite samples from the Itabira district and fluid inclusions therein fairly plot on or close to the reference line for 635 Ma. The least radiogenic Pb isotopic composition from the investigated region was measured on galena from stratiform gold deposits in the Archaean Rio das Velhas Supergroup. Starting from such a composition and lasting until the Transamazonian orogeny in situ Pb growth would yield values that fall on the red array in Fig. 3. Samples with low µ values would have evolved less from their starting composition, whereas samples with high µ values would have evolved to more radiogenic composition. There may be a lithologic control on the µ values, which higher values in more evolved felsic units than in mafic units. Depending on source regions for the itabirite-type iron deposits in the Palaeoproterozoic clastic-chemical sediments of the Minas Supergroup, different deposits may have a constrasting Pb isotopic composition. Undisturbed in situ Pb growth in itabitirite-type iron deposits until the present would result in Pb isotopic compositions that fall between the 1.83 Ga reference line of Olivo et al. (1996) and the Archaean-to-Transamazonian Pb trend (Fig. 3). As the Pb isotopic composition of most samples falls to the right of Close 824 R.L. Romer · V. Lüders · D.A. Banks · J. Schneider the 1.83 Ga reference line, lead evolution to highly radiogenic compositions occurred mainly after the Braziliano orogeny (see also Fig. 3c). The scatter of the data in the 206Pb/204Pb vs. 238U/204Pb diagram either may reflect several events, most prominantly a Braziliano and a Transamazonian event (Fig. 3c) or it may reflect that the initial Pb isotopic compositions of some deposits was highly radiogenic at the time of the Braziliano orogeny (dashed line in Fig. 3c). The Pb isotopic composition of trace Pb in gold generally has lower 208Pb/204Pb values than the hematite samples. Furthermore, this trace Pb plots above the 1.83 Ga reference line and above the hematite field (Fig. 3). The contrasting Pb isotopic composition between hematite and gold in the jacutinga-style veins possibly suggests that hematite incorporated significant amount of locally derived material and that the veins in part even may contain hematite grains originating from the older wallrock. The relation of the trace Pb from gold is compatible with a derivation from an Archaean source rock that is characterized by high 238U/204Pb values and relatively low 232Th/204Pb values. In this context, Archaean source does not only refer to the Archaean basement, but also to its cover of Palaeoproterozoic clastic sediments that were derived from the Archaean basement. The relation of the trace Pb from gold is incompatible with a derivation from the same source as the Pb in the itabirites or from the itabirites itself. If the Archaean felsic basement is the source of the trace Pb in gold, the same source could also be the source of U, which eventually gave rise to radiogenic Pb isotopic compositions in hematite. This source may also have had controlling influence on the homoge- neous Na/K ratios in hematite-hosted fluid inclusions. A felsic Archean basement, however, could not provide Au and Pd. Instead, these two elements may be derived from the Archaean supracrustal rocks that include voluminous units of mafic volcanic rocks. Since the Pb contents in felsic rocks are much higher than in mafic and ultramafic rocks, the Pb isotopic composition reflects the signature of the felsic basement rather than the mafic units. Thus, the fluid that transported Au and Pb into the jacutinga–style veins may carry the Pb isotopic signature of a source rock that does not correspond to the source of Au and Pd. This explanation allows the fluid to acquire its Pb isotopic signature either in the felsic basement below the greenstone unit or in the Palaeoproterozoic clastic sediments between the Archaean basement and the units hosting the itabirite-type iron deposits. The occurrence of Au (and Pd), however, is controlled by the distribution of Au-bearing mafic to ultramafic supracrustal rocks in the Archaean basement. Thus, there may be a spatial correspondance between stratiform Archaean and jacutinga-type Braziliano gold deposits. Au in both deposits would have been mobilized from the same source rocks. The formation of the jacutinga–style veins during the Brazilian orogenic cycle explains both the homogeneous nature of the fluids with respect to dissolved major components, e.g., Na/K, Cl/Br ratios, high-SO4 content, and the heterogeneous character of the fluids with respect to CO2 content and trace (Au, Pd, Pb, and U) constituents, as differences in proportions of major components reflect contrasting evolution histories of the fluid in terms of unmixing and cooling. Close Chapter 7-27 7-27 Constraints on the source and evolution of mineralising fluids in the Norrbotten Fe oxide-Cu-Au province, Sweden Martin Smith School of the Environment, University of Brighton, Brighton, BN2 4GJ, U.K. Sarah A. Gleeson University of Alberta, Edmonton T6G 2E, Canada Abstract. Norrbotten County, Sweden, is well known for the iron oxide-apatite deposits of the Kiruna and Malmberget areas. These are spatially associated with iron oxide Cu (± Au) deposits and a genetic link between the two has been suggested as a part of the IOCG spectrum of deposits. Here, we report the results of a fluid inclusion microthermometry and bulk crush leach halogen and chlorine stable isotope study, carried out to test that hypothesis. Quartz veins from late stage veins from Fe oxide-apatite deposits and Cu-(Au) deposits contain hypersaline brine inclusions, with a salinity range of 32 to 38wt. % NaCl eq. in Fe-oxide bodies, and of 38 to 47wt % NaCl eq. in Cu-Au deposits. In Cu-(Au) deposits these are sometimes accompanied by CO2-rich inclusions. The Cl/Br ratio of the fluid inclusion leachates is consistent with magmatic fluid compositions, and ranges between 859 and 9597, with no distinction between the Fe-oxide samples and the Cu-mineralizing brines. δ37Cl(SMOW) values range from –0.99 to –5.63‰. The data are far removed from both mantle (δ37Cl = +4.7‰) and crustal (δ37Cl = 0‰) values and must represent fractionation of the isotopes during the mineralizing process. We suggest this fractionation occurred during the formation of Cl-rich mineral phases commonly found associated with the deposits e.g. scapolite, biotite and amphibole. Keywords. Fluid inclusions, halogens, IOCG, chlorine isotopes 1 Introduction The original classification of iron oxide-copper-gold type deposits by Hitzman et al. (1992) postulated a link between Fe oxide-apatite deposits (‘Kiruna-type’) and the IOCG deposits themselves. Northern Norrbotten County, Sweden, is well known for the Kirunavaara deposit, and also hosts several Cu-(Au) deposits (Bergman et al., 2001). However, magnetite-apatite bodies and epigenetic Cu-Au bodies formed in the range 1900-1860Ma (Romer et al., 1994; Billstrom and Martinsson, 2000), but with the CuAu systems potentially post-dating the Fe oxide-apatite bodies. Younger deposits still (~1800-1750Ma) are associated with regional scale shear zones. All these deposits show similar alteration types and association with regional sodic alteration (Frietsch, 1997), and have been suggested to belong to the IOCG group. A knowledge of fluid source in all three deposit types is therefore of value for metallogenetic models, and will help to define any common mineralising processes related to episodic metamorphism or magmatism. As a part of the EU-RDF Georange program we have investigated the fluid sources for quartz veins from the late stage of Fe oxide-apatite ore forma- tion and from a range of Cu-(Au) deposits and prospects using a bulk crush leach technique to analyse for cation, anion, and chlorine isotope composition within the inclusion fluids. 2 Sample sites The geology of the Norrbotten area consists of a Palaeoproterozoic supracrustal sequence overlying Archaean basement, which was deformed and intruded by grantoids during the Svecofennian orogeny (1.96-1.85Ga). The Palaeoproterozoic sequence within the area studied is broadly separated into the Greenstone Group metabasic rocks, and the overlying Porphyry Group, which consists of intermediate to acid volcanics and intercalated sediments. Within Fe oxide-apatite bodies, quartz veins cross-cut both the ore itself, and altered footwall rocks. Samples of this kind were collected from the magnetite-hematite-apatite bodies of the Kiruna area and from the Valkommen deposit, which forms a part of Malmberget Fe oxide-apatite body. Samples from Cu-(Au) deposits where collected from sites hosted in the Greenstone and Porphyry Group volcanics at Pahtohavare (Lindblom et al. 1996), Kallosalmi and Gruvberget, and from younger deposits associated with the Nautanen Deformation Zone (Fig. 1). Close 826 Martin Smith · Sarah A. Gleeson 3 Techniques Samples were initially characterised petrographically and microthermometrically using a Linkam TMS600 heatingfreezing stage at the University of Brighton. Samples were then crushed and hand picked to provide approximately 5g of pure quartz for crush leach analysis. Samples were electrolytically cleaned prior to crushing, and the leachates analysed for Na, Li and K using atomic absorption spectroscopy, for other cations using ICP-MS, and for halogens, sulphate and phosphate using ion chromatography at the University of Alberta. Chlorine isotope analyses were carried out on the leachates using gas source mass spectrometry at Environment Canada, Saskatoon. 4 Results 4.1 Microthermometry Late stage quartz veins cutting Fe-oxide apatite bodies or their wall rocks contain a consistent fluid population across the area (salinity 30-40 wt. % NaCl eq.; Th=100150°C). Fluids associated with quartz veins from Cu-(Au) deposits and prospects, range from much higher salinities (around 50-60 wt % NaCl eq.) to those comparable with the late stage veins associated with the Fe-oxide bodies. Two veins from the Gruvberget body contain lower salinity, Ca-rich inclusions, which probably represent a post-ore fluid. The inclusion assemblage from deposits associated with the NDZ is more complex, with coexisting Lw+Sh+V, Lw+Lc+V and Lc+V inclusions. In some instances these are preserved along the same secondary fluid inclusion trails. Lw+Sh+V inclusions from the Valkommen body, and from some veins at Nautanen show similar salinities and homogenisation temperatures to those from the Feoxide and Cu-Au deposits already discussed. At Nautanen complex inclusion assemblages are hosted on secondary trails. These are indicative of phase separation. Salinities vary from ~12-18 wt. % NaCl eq. for Lw+Lc+V inclusions to ~29wt % NaCl eq. for halite bearing inclusions. Total homogenisation temperatures for Lw+Lc+V inclusions are typically around 250-300°C, whilst partial L-V homogenisation for halite bearing inclusions is around 100-120°C. At both Nautanen and Ferrum a further assemblage of Ca-rich brines is observed similar to those observed in some veins at Gruvberget. Many of the observations made here are in agreement with previous work by Broman and Martinsson (2000). 4.2 Halogen chemistry Log Br/Cl ratios within leachates from these fluids (Fig. 2) range from approximately –2.5 to -3.7, with two exceptional analyses at –2.3 and –4.4. The majority of analyses fall in the range –2.8 to –3.5 with no distinction between Fe-oxide related and Cu-related brines. These data are compared with a selection of previous data from Yardley et al. (2000) in Figure 2. They are most comparable to S.W. England granite related fluids, and are clearly distinct from fluids associated with the Capitan Pluton, New Mexico and Columbian Emerald deposits. This is significant as these are both interpreted as deriving their salinity either from magmatic interaction with evaporites, or from metamorphism of evaporites. Our data are therefore consistent with magmatic sources for mineralising fluids in Norrbotten, and not with a meta-evaporitic source. The more Br enriched samples are lower salinity fluids from the NDZ, and possibly indicate interaction of a magmatic fluid with the surrounding metasediments. 4.3 Chlorine isotopes The chorine isotopic composition of leachates from vein quartz samples from Fe oxide-apatite bodies, and from epigenetic Cu-Au deposits ranges in δ37Cl relative to standard mean ocean chlorine (SMOC) from -5.63 to -0.99‰. These data are compared with previous data from inclu- Close Chapter 7-27 · Constraints on the source and evolution of mineralising fluids in the Norrbotten Fe oxide-Cu-Au province, Sweden sion fluids, natural porewaters and rocks and minerals in Figure 3. Norrbotten inclusion fluids are consistently enriched in 35Cl relative to all previously analysed fluid inclusions, most rocks and minerals and most natural porewater samples. The only comparable data are from subduction zone porewaters sampled in the Barbados and Nankai accretionary prisms (Ransom et al. 1995). Luders et al. (2002) showed that submarine hydrothermal fluids could be enriched in 37Cl by extraction of 35Cl into a vapour phase during boiling, and consequently a condensate from a low density fluid or vapour could show low δ37Cl values. However, the high salinity of these fluids would seem to preclude their origin as a condensate. Equally 35Cl enriched fluids can be formed by the evapo-concentration of seawater and precipitation of halite (Eastoe et al. 1998), but such fluid have not yet been reported with the low δ37Cl values seen here. The most likely explanation for the Cl isotope data is the preferential extraction of 37Cl into silicate mineral phases (in this case scapolite, biotite 827 and amphibole) results in a passive enrichment of hydrothermal fluids in 35Cl. Chlorine isotope analyses of silicate minerals are relatively limited at the present time, but those available from biotites in the Stillwater complex (Boudreau et al. 1997), Porphyry Cu related biotites (Arcuri and Brimhall 2003) show uniformly positive δ37Cl values. Experimental data from. Pan and Dong (2003) show that Br/Cl ratios of marialitic scapolite closely reflect the halogen composition of co-existing fluids, and hence this process would not be expected to affect the Br/Cl signature of hydrothermal fluids. 5 Discussion and conclusions The data presented here are consistent with a magmatic fluid source for Porphyry and Greenstone Group hosted Cu-(Au) mineralization in Norrbotten, and for late stage fluids associated with Fe oxide-apatite bodies. The microthermometric data do not, however, indicate that directly comparable fluids were involved in the formation of the Fe oxide- apatite bodies and the Cu-(Au) mineralization. The displacement of δ37Cl values to lower values in the epigenetic Cu-(Au) mineralising fluids may reflect extensive water rock interaction and Na-Cl metasomatism during this stage of the regions evolution. Fluids associated with younger, shear zone hosted deposits are also potentially magmatic, although the inclusion of several fluid inclusion populations reflects the modification over an extended period and possibly the input of metamorphic fluids. Temporal constraints indicate that the highly saline ore fluids present in all deposits must have been generated during several magmatic events, with the additional input of non-magmatic fluids into the younger, shear zone hosted deposits at Nautanen. Previous workers have suggested that meta-evaporites may have played a role in generating the highly saline brines and regional sodic alteration in Norrbotten (Frietsch et al. 1997). We find no evidence to support this idea. Halite typically shows heavy δ37Cl values relative to the fluid from which it precipitates, so halite dissolution is unlikely to form strongly 37Cl depleted fluids. We have not yet, however, analysed samples containing a significant proportion of the Ca-rich brine, and this may preserve such a signature (Wanhainen et al. 2003). References Arcuri T, Brimhall G (2003) The chloride source for atacamite mineralization at the Radomiro Tomic porphyry copper deposit, Northern Chile. Econ Geol 98:1667-1681 Banks DA, Gleeson SA, Green R (2000) Determination of the origin of salinity in granite-related fluids: evidence from chlorine isotopes in fluid inclusions. J Geochem Expl 69-70: 309-312 Banks DA, Green R, Cliff R, Yardley BWD (2000) Chlorine isotopes in fluid inclusions: Determination of the origins of salinity in magmatic fluids. Geochim Cosmochim Acta 64:1785-1789 Close 828 Martin Smith · Sarah A. Gleeson Bergman S, Kübler L, Martinsson O (2001) Description of regional geological and geophysical maps of northern Norrbotten county (east of the Caledonian orogen). Sver Geol Unders Ba 56. Billstrom K, Martinsson O (2000) Links between epigenetic Cu-Au mineralisations and magmatism/deformation in the Norrbotten county, Sweden. In: LuT research report 2000:06. 2nd GEODE Fennoscandian Shield field workshop on Palaeoproterozoic and Archaen greenstone belts and VMS districts in the Fennoscandian Shield. Boudreau AE, Stewart MA, Spivack AJ (1997) Stable Cl isotopes and origin of high-Cl magmas of the Stillwater Complex, Montana. Geology 25 791-794 Broman C, Martinsson O (2000) Fluid inclusions in epigenetic FeCu-Au ores in northern Norrbotten. In: L..T research report 2000:06. 2nd GEODE Fennoscandian Shield field workshop on Palaeoproterozoic and Archaen greenstone belts and VMS districts in the Fennoscandian Shield. Eastoe CJ, Long A, Kinaith LP (1998) Stable chlorine isotopes in the Palo Duro Basin, Texas: Evidence for preservation of Permian evporite brines. Geochim Cosmochim Acta 63: 1375-1382 Frietsch R, Tuisku P, Martinsson O, Perdahl JA (1997) Early proterozoic Cu-(Au) and Fe ore deposits associated with regional Na-Cl metasomatism in northern Fennoscandia. Ore Geol Rev 12: 1-34 Hitzman MW, Oreskes N, Einaudi MT (1992) Geological characteristics and tectonic setting of proterozoic iron-oxide (Cu-U-AuREE) deposits. Precambr Res 58: 241-287 Lindblom S, Broman C, Martinsson O (1996) Magmatic-hydrothermal fluids in the Pahtohavare Cu-Au deposit in greenstone at Kiruna, Sweden. Mineralium Depos 31: 307-318 Luders V, Banks DA, Halbach P (2002) Extreme Cl/Br and δ37Cl isotope fractionation in fluids of modern submarine hydrothermal systems. Mineralium Depos 37: 765-771 Pan Y, Dong P (2003) Bromine in scapolite-group minerals and sodalite: XRF microprobe analysis, exchange experiments, and application to skarn deposits. Can Mineral 41: 529-540 Ransom B, Spivack AJ, Kastner M (1995) Stable Cl isotopes in subduction-zone pore waters - implications for fluid-rock reactions and the cycling of chlorine. Geology 23:715-718 Romer RL, Martinsson O, Perdahl JA (1994) Geochronology of the Kiruna iron ores and hydrothermal alterations. Econ Geol, 89:1249-1261 Yardley BWD, Banks DA, Barnicoat AC (2000) The chemistry of crustal brines: tracking their origins. In: TM Porter (ed) Hydrothermal iron oxide copper-gold and related deposits: A global perspective. Austral Min Found, Adelaide, pp. 61-70. Close Chapter 7-28 7-28 LA-ICPMS U-Pb dating of titanite: New constraints on multistage geological evolution of the Norrbotten mining district, Sweden Martin Smith, Craig Storey School of the Environment, University of Brighton, Brighton, BN2 4GJ, U.K. Teresa Jeffries Department of Mineralogy, The Natural History Museum, London, SW7 5BD, U.K Abstract. Established techniques for the laser ablation ICP-MS UPb analysis of zircon have been developed for application to common Pb bearing phases, including titanite and allanite. A novel common Pb correction procedure has been developed for deriving mineral ages, and has been tested using well characterised samples. This technique has been applied to samples from the mining district of Norrbotten, Sweden, with the aim of constraining the timing of iron oxide-copper-gold (IOCG) mineralization in relation to the formation of Fe-oxide-apatite deposits and the regional geological evolution. Titanites from three of the Fe oxide apatite deposits studied show complex multistage growth textures implying a prolonged metasomatic history. Cores from these samples show ages in the range 2070 to 2000 Ma before present, indicating that the age of the host supracrustal sequence in Norrbotten may be significantly older than previously thought. The rims of these crystals, which show distinct trace element signatures to the cores, as well as unequivocally metasomatic titanites and allanites from other areas give ages in the range ~1875-1820Ma. These ages probably indicate the time of primary mineralization of both the late stages of Fe oxide and Cu-Au types. Younger ages in the range ~1790-1700Ma are interpreted to relate to subsequent metamorphism of the deposits, and remobilisation of sulphide mineralization along long lived, regional scale structures. 2 Technique In this study we have extended established U-Pb techniques by LA-ICPMS (quadrupole) to titanite and allanite. Titanite and other common U hosting minerals readily incorporate up to ppm levels of (common)Pb into their lattice alongside U and Th during crystallisation, making the necessity for common Pb correction paramount. In this study we have used both a mathematical based 207Pb-correction, and the far more robust TIMS-style correction. The TIMS-style correction is based upon measurement of the stable 204Pb isotope to assess the amount of common Pb in the analysis. This requires an independent measurement or estimate of the common Pb composition to be corrected for. We have made measurements of common Pb composition by utilising in line gold traps to reduce interferances on the 204Pb peak from mercury stable isotopes. In samples with low analytical signal intensity we combine this approach with a novel appraoch based on 3 dimensional U-Pb concrodia. 3 Sites investigated Keywords. U-Pb, geochronology, titanite, Norrbotten, Kiruna, IOCG 1 Introduction Northern Norrbotten County, Sweden, is well known as a region of Fe oxide-apatite mineralization, and also hosts a range of copper-gold deposits (Bergman et al. 2001). These deposits have been proposed to be related as a part of the iron oxide-copper-gold (IOCG) spectrum of deposits. A more detailed understanding of this relationship will be of great use to defining ore genetic and exploration models in terms of both the relationship of CuAu mineralization to Fe oxide mineralization, and the relationship of both mineralization types to the regional geological evolution. As a part of the EU-RDF Georange program we have investigated this relationship via the development of a novel U-Pb geochronological technique, which allows the use of in situ laser ablation ICP-MS for analysis of titanite and other common lead-bearing phases within polished thick sections. The geology of the Norrbotten area consists of a Palaeoproterozoic supracrustal sequence overlying Archaean basement, which has subsequently been deformed and intruded by grantoids during the Svecofennian orogeny (1.96-1.85Ga). The Palaeoproterozoic sequence within the area studied is broadly separated into the Greenstone Group metabasic rocks, and the overlying Porphyry Group, which consists of intermediate to acid volcanics and intercalated sediments. For the purpose of this study we have examined material from both Fe oxide-apatite and copper deposits (Bergman et al. 2001) including titanite intergrown with magnetite from deformed vesicle fills within the sodically altered footwall trachyandesites at Luossavaara, and titanite hosted in quartz-carbonate veins cutting magnetite cemented brecciated metavolcanics in the footwall of the Kirunavaara magnetite-apatite body. Within the Kiruna area samples were also analysed from Cu-(Au) deposits and prospects at Rakkurijarvi (Porphyry Group hosted) and Kallosalmi (Greenstone Group hosted). We Close 830 Martin Smith · Craig Storey · Teresa Jeffries have also analysed samples from the Gruvberget Cu deposit, developed in the footwall to a magnetite-hematiteapatite body, again hosted by intermediate metavolcanics. The third area studied was around Malmberget to the south of Kiruna. The Malmberget body itself is an Fe oxideapatite body exposed in a large fold structure. It is interpreted to be a metamorphosed Kiruna type deposit. Samples where taken from the hanging wall of the Valkommen ore body. To the east of the Malmberget body both the supracrustal sequences and the Svecofennian granitoids are cut by a regional scale shear system (the Nautanen Deformation Zone). This hosts the working Cu-(Au) mine at Aitik, and a historically worked prospect at Nautanen. 4 Results of geochronological studies A number of samples show complex multistage growth (Fig. 1). Samples from Luossavaara, Gruvberget, and Malmberget show core ages in the range 2073-2028 Ma. All these bodies are Fe-oxide (and sometimes copper) deposits hosted in Porphyry group metavolcanics, supposedly of Svecofennian age. The BSE light rims of most of these Close Chapter 7-28 · LA-ICPMS U-Pb dating of titanite: New constraints on multistage geological evolution of the Norrbotten mining district, Sweden titanites give ages in the range 1920 to 1826 Ma. LA-ICPMS trace element analyses from corresponding sites in the same grains show a clear distinction between core and rim analyses (Fig. 2). The younger, rim zones are strongly LREE enriched relative to the core zones. These patterns are comparable to the composition of unequivocally metasomatic titanites from other deposits. The rim zones are volumetrically the most significant parts of the crystals. The ages obtained from these zones are reflected in previous TIMS data from Norbotten titanite which analysed bulk crystals. The range of ages from the alteration surrounding Fe-oxide and Cu-deposits is previously unreported from the Porphyry Group and the deposits which it hosts. These data suggest a minimum age of the Porphyry group of between ~2070-2028 Ma, significantly older than currently thought. Analyses of titanites from regional alteration (Nunasvaara) and the alteration surrounding Fe-oxide and Cu-Au deposits hosted by the Porphyry Group range from 1902+/-8 Ma (Nunasvaara) to 1758+/-18 Ma (Tjarrajäkka). The data in the range of 1920-1826 Ma correspond to the time range of the Svecofennian metamorphism, and the main intrusive activity in the area. Our data are consistent with 831 either metamorphic growth of titanite during this period or metasomatic growth of titanite during hydrothermal activity. The youngest ages so far encountered are from the Valkommen body, with titanite at 1708±20 Ma, and apatite at 1584±12 Ma. The very young age recorded in apatite from Valkommen is related to the lower closure temperature of apatite relative to either titanite or zircon. We suggest that these ages record subsequent metamorphism of the deposits in question. Data from deposits hosted by, or associated with, the NDZ range from 1826+/-15 Ma to 1756+/-20 Ma. Two samples from the Nautanen deposit gave ages of 1810+/21 Ma and 1756+/-20 Ma respectively. These data indicate a prolonged history of deformation and fluid flow along the NDZ, probably involving multiple episodes of ore deposition and remobilisation. The REE patterns of these titanites are LREE depleted; indicating different chemical conditions of titanite formation in the NDZ compared to other Cu-(Au) deposits. This may be related to contrasting fluid chemistry, or may reflect ore-forming processes, particularly the co-precipitation of allanite and LREE enriched epidote. Close 832 Martin Smith · Craig Storey · Teresa Jeffries 5 Discussion and conclusions The data presented here are generally in agreement with previous data on mineral deposits within the Norrbotten region. The Kirunavaara and Luossavaara mineralization has previously been dated at 1888+/-6 Ma between 1876+/ -9 Ma by Billstrom and Martinsson (2000), who reported U-Pb titanite ages for Cu-Au mineralization in the ranges 1880-1860Ma and 1800-1750Ma. These ages are also in broad agreement with our data; however, a number of deposits in the younger group in their study gave ages in the older group in this study. This is likely to represent a difference in the scale of sampling, and suggests that the age heterogeneity seen in these deposits is the result of metamorphic remobilisation of ore in the period 1800-1750Ma. In complex zoned grains we interpret the data from the cores as indicating the timing of initial metamorphism (and a minimum age for magmatism), and data from the rims as indicating the timing of metasomatic fluid flow associated with mineralization. Previous constraints on the age of the Porphyry group come from U-Pb dating of zircon (Welin 1987; Skiöld and Cliff 1984). Our new data now suggest these ages may represent recrystallisation of zircon during a later metamorphic/metasomatic event. In summary, the data from titanite cores suggest that Porphyry and Porphyrite group volcanism occurred significantly earlier than previously thought. This has significant implications for the timing of rifting and subduction during the early tectonic evolution of the Fennoscandian shield. It may also have implications for correlation of Norrbotten stratigraphy with that of the Skellefte district (Bergman et al. 2001). The timing of Fe oxide and Cu-Au deposit formation corresponds to that of the Svecofennian metamorphism, and the intrusion of the Haparanda and Perthite-monzonite suite granitoids. A second stage of mineralisation, or metamorphism of previously formed deposits occurred in association with the younger stage of metamorphism. This possibly accompanied movements on the Nautanen Deformation Zone. References Bergman S, Kübler L, Martinsson O (2001) Description of regional geological and geophysical maps of northern Norrbotten county (east of the Caledonian orogen). Sveriges geologiska undersökning Ba 56 Billstrom K, Martinsson O (2000) Links between epigenetic Cu-Au mineralisations and magmatism/deformation in the Norrbotten county, Sweden. In L.U. T. research report 2000:06. 2nd GEODE Fennoscandian Shield field workshop on Palaeoproterozoic and Archaen greenstone belts and VMS districts in the Fennoscandian Shield Romer RL (1996) What is the significance of lead isotope data from stilbite, a low temperature natural ion exchanger? The 22nd Nordic Geological Winter Meeting, Turku, Åbo, Abstracts, 172 Romer RL, Martinsson O, Perdahl JA (1994) Geochronology of the Kiruna iron ores and hydrothermal alterations. Economic Geology 89: 1249-1261 Skiöld T, Cliff RA (1984) Sm-Nd and U-Pb dating of Early Protoerozoic mafic-felsic volcanism in northernmost Sweden. Precambrian Research 26: 1-1 Welin E (1987) The depositional evolution of the Svecofennian supracrustal sequence in Finland and Sweden. Precambrian Research 35: 95-113 Close Chapter 7-29 7-29 Metamorphic to magmatic transition captured at the Myszków Mo-W deposit, southern Poland H.J. Stein AIRIE Program, Department of Geosciences, Colorado State University, USA, and Norges Geologiske Undersøkelse, Trondheim, Norway M. Markowiak, S.Z. Mikulski Polish Geological Institute, Sosnowiec and Warszawa, Poland Abstract. Millimetre scale drilling of paragenetic ally-specific sulphide occurrences represented by ten Myszków molybdenite samples provides a temporal framework for this Mo-W deposit, associated with the transcontinental Hamburg-Kraków tectonic zone. With replicates (second mineral separates) for two samples, a total of twelve Re-Os model ages pin high temperature molybdenite-scheelite(chalcopyrite) mineralization to a narrow time window, from 300 ± 1 to 296 ± 1 Ma (2-sigma). Published 40Ar/39Ar ages (305-290 Ma) for potassium feldspar, white mica, and biotite do not precisely pin the timing of mineralization, but provide information on the regional cooling history. Alteration is characterized by local metasomatism of hosting Vendian to Cambrian metamorphic rocks, and spatial patterns for Mo-W-(Cu) mineralization support a relationship between metasomatism and mineralization. Dehydration melting of middle crust was followed by local intrusion of magmas along structurally vulnerable zones. Melting of hosting metaclastic sequences influenced local metallic assemblages and provided the magmatic apophyses and crustal enclaves associated with much of the Myszków mineralization. Even though local stockwork may be found, the overall architecture of the Myszków deposit does not support a calc-alkaline porphyry-style deposit, and this interpretation should be reconsidered. We attribute Myszków mineralization to unroofing of the Variscan orogen, rapid late Variscan uplift, and exhumation melting. Keywords. Re-Os, molybdenite, Mo-W deposit, metasomatism, Myszków, Poland 1 Introduction Late Variscan (~300 Ma) Mo-W mineralization at Myszków has been classified as a calc-alkaline porphyrytype deposit situated in a poorly defined belt of magmatic rocks in south-central Poland (Podemski et al. 2004; Markowiak et al. 2001). Features defining of calc-alkaline porphyry-style mineralization, however, are conspicuously absent, not the least an intrusion centered brittle-planar stockwork and attendant alteration types. Re-Os data for molybdenites have provided key information on the timing and genesis of a broad spectrum of deposits, in particular, metamorphically-derived deposits versus classic Cu-Mo-Au porphyry-style mineralization (e.g. Stein, in press). The former tend to be small in size, of erratic but locally high-grade, and display widely dispersed rather than focussed ore zones. They are associated with moderate-low ppm to sub-ppm levels of Re. In contrast, true porphyry systems have high to very high Re contents (hundreds to thousands of ppm) associated with main stage molybdenites, and are the product of a vertically and laterally communicative magmatic-hydrothermal system that moved from deep to shallow crustal levels, over a period of several million years, importantly, without venting. With these characteristics in mind, we apply Re-Os dating of molybdenite through the paragenetic history of Myszków to document the timing and duration for its formation and to improve our understanding of this unusual deposit. 2 Geologic setting The Myszków deposit is situated along the NE margin of the NW-trending Kraków-Lubliniec tectonic zone, a segment of the transcontinental Hamburg-Kraków tectonic zone. In southern Poland, the tectonic history of this zone is poorly known but strike-slip movement appears to be an important component. Mafic to felsic magmatism with granodiorite prevailing is common along the 15 km segment of the Kraków-Lubliniec tectonic zone that includes the Myszków Mo-W region. Magmatic rocks are hosted by intensely folded, predominantly fine-grained Vendian to Cambrian clastic units at regional greenschist facies. Upper amphibolite-granulite facies (metasomatic) is locally present in the vicinity of magmatic rocks. A NW-trending granodiorite body with subvolcanic dacite and rhyolite porphyry dikes intruded the metasedimentary rocks, and contact relations vary from sharp to ill-defined. The overall character of the Myszków granodiorite is one of a moderately flattop intrusion extending over tens of kilometres, and dissected by normal faults (Fig. 1). Interfingering and foliation parallel magmatic units intersected in drill holes in the vicinity of the granodiorite are interpreted as apophyses to the granodiorite body (Podemski et al. 2001). Associated alteration is described both as metasomatic and hydrothermal vein type, with significant K-feldspar, silica, sericite, and carbonate. While potassic alteration is prevalent, secondary biotite, magnetite, and significant pyrite are conspicuously sparse. Some alteration assemblages have been described as greisen-like at Myszków. Close 834 H.J. Stein · M. Markowiak · S.Z. Mikulski Three periods of mineralization are defined at Myszków: Early Skarn (Period I), Main Hydrothermal (Period II), and Late Post-Ore (Period III). The first two are molybdenite-bearing. Within Period I, early skarn consists of magnetite-sulfide mineralization. Within Period II, different stages of ore deposition are proposed (Stage 1, feldspar-molybdenite veins with biotite; Stage 2, quartz-feldspar pegmatite veins; Stage 3, quartz-molybdenite stockwork with scheelite; Stage 4, black quartz veins with microsulfide; Stage 5, quartz polymetallic veins without molybdenite and late brecciated quartz veins with sulfide. The Period-Stage classification (Þlósarz 1985, 1993) was used for our molybdenite samples (Table 1), and is summarized in Podemski et al. (2001). 4 The Myszków deposit, outlined by 35 boreholes from 1985 to 1993, is estimated to contain 800 million tons of ore at 0.15% Cu, 0.05% Mo, and 0.04% W and continues to at least 1250m depth (Podemski et al. 2001). Several similar deposits were also discovered in this region. Significantly, Cu mineralization (chalcopyrite) bears little spatial relation to W and Mo mineralization (scheelite and molybdenite). And, W and Mo also exhibit differences. In general, W (and Mo) are associated with magmatic rocks, whereas Cu and to some extent Mo, are associated with contact regions between granodiorite and metaclastic host units. Molybdenite is generally associated with quartz veins and patches in pink (potassic) granodiorite, but these ill-defined and scattered veins do not constitute stockwork in the classical sense. Also, the richest ore body is contained in an enclave of metaclastic host rock within the upper portion of the granodiorite (Chaffee et al. 1997), rather than exhibiting an intrusion-wide association to the granodiorite. Myszków mineralization and paragenesis have been described in detail by Piekarski (1982, 1995) and Þlósarz (1985, 1993), including vein, pegmatitic, metasomatic, disseminated, and skarn varieties (see Podemski et al. 2001). 3 Molybdenite samples dated This Re-Os study utilizes different ore occurrences to determine the relative timing of ore-forming environments at Myszków. Even at the hand-specimen scale, molybdenite was drilled from occurrence-specific sites, a critical step for successful age determinations in complex metamorphic settings (Stein in press). Replicate ages for two samples were acquired from new mineral separates exploiting the same occurrence. This is an indisputable test for age accuracy. Re-Os analytical results Twelve Re-Os ages representing paragenetically defined Myszków molybdenites provide a remarkably narrow age range, 300 ± 1 to 296 ± 1 Ma (2-sigma). Re concentrations are moderate, ranging from an about 40 to 74 ppm. The lower value (40 ppm) is an estimate of the true Re concentration as up to 95% dilution of the molybdenite separate by quartz was unavoidable during drilling of some samples. Such samples consist of very fine-grained grey streaks of molybdenite in quartz (see footnote, Table 1). This does not affect the age calculation, as diluting quartz contains essentially no Re and Os. Four samples with abundant and coarser crystalline molybdenite suggest that ~70 ppm Re was common to the fluids forming quartz-molybdenite veins. Notably, the Re values reported in Podemski et al. (2001), 0.07 to 0.17% (700 to 1700 ppm), bear no resemblance to our Re values determined by isotope dilution. It is highly unlikely that both data sets can be correct for a single deposit. 5 Discussion and conclusions The moderate and fairly consistent Re levels (about 40 to 75 ppm) for Myszków molybdenites do not support a subduction-related porphyry-style origin (Stein et al. 2001). A better fit would be a moderately local derivation utilizing a crustal reservoir with fairly consistent Re, rather than one dependent on batch additions of material from different reservoirs, mixing, and system wide fluid separation (porphyry model). At Myszków, development of local veins, stockwork, and pegmatite likely depended on local separation and volatile enhancement of hydrothermal fluids that were not far-travelled. Re-Os ages have a very tight range (300-296 Ma) and 40Ar/39Ar ages (305-290 Ma) overlap the molybdenite age range but should be interpreted as recording the cooling history at the sampled localities for the minerals dated Close Chapter 7-29 · Metamorphic to magmatic transition captured at the Myszków Mo-W deposit, southern Poland (potassium feldspar, biotite, white mica). Argon geochronology should not be used to define ages of high temperature Mo-W-Cu mineralization (Stein et al. 2001). General agreement between Re-Os and 40Ar/39Ar ages suggests that the region cooled very quickly, and has not seen any further thermal activity. Mineralogy (e.g. lack of abundant chalcopyritee, fluorite, and Au), lack of an intrusion-centered relationship for mineralization, lack of correlation between Cu and Mo, the abundance of W, lack of planar-brittle vein styles, and lack of classic porphyry-style alteration collectively do not support a Mo-W calc alkaline intrusion-related, porphyry model (Podemski et al. 2001). Re-Os ages and the preserved regional greenschist facies character of host rocks with local high temperature contact metamorphism suggest rapid uplift with structurally favourable but localized discontinuities serving as focussing sites for intrusion. This was accompanied by local and brief in situ melting and metasomatism. As a result, erratic mineralization of variable grade covers a large region. This includes the Myszków deposit and other prospects in the Kraków-Lubliniec tectonic zone. Small perturbations in pressure permitted local formation of thick (cm scale) “stockwork” veins but true and abundant stockwork never formed system wide as defines classic Cu-Mo-Au-W porphyry-style mineralization. Furthermore, there is no evidence for a regional tectonic envi- 835 ronment conducive to classic porphyry-style mineralization, as at ~300 Ma the Variscan orogeny is not characterized by subduction. We suggest that the Myszków Mo-W deposit is the product of exhumation melting associated with rapid unroofing of the Variscan orogen. Acknowledgements Re-Os analytical work was carried out by AIRIE graduate students A Zimmerman and N Loeppke, and supported by NSF EAR-0087483. Salary support for HJS was provided by Edward Warner. References Chaffee MA, Eppinger RG, Lasón K, Mlósarz J, Podemski M (1999) A geological, alteration, and geochemical model of the Myszków porphyry Cu-Mo deposit, southern Poland, in Papunen (ed). Mineral Deposits, Balkema, Rotterdam, 851-854 Markey RJ, Hannah JL, Morgan JW, Stein HJ (2003) A double spike for osmium analysis of highly radiogenic samples. Chemical Geology 200: 395-406 Markowiak M, Þlósarz J, Lasón K, Podemski M, Karwowski L, Chaffee MA (2001) Palaeozoic porphyry molybdenum-tungsten mineralization in the Myszków area, southern Poland, in Piestrzynski et al. (eds). Mineral Deposits at the Beginning of the 21st Century, Swets & Zeitlinger Publishers Lisse, 445-448 Piekarski K (1982) Molybdenum schists in the vicinities of Myszków (Eng Sum). Prz Geol 30(7): 335-340 Close 836 H.J. Stein · M. Markowiak · S.Z. Mikulski Piekarski K (1995) Geologic setting and ore mineralisation characteristics of the Myszków area (Poland). Geol Quart 39(1): 31-42 Podemski M (editor), BuÝa Z, Chaffee MA, Cießla E, Eppinger R, Habryn R, Karwowski L, Lason K, Markiewicz J, Markowiak M, Snee LW, Þlósarz J, Truszel M, Wybraniec S, Zaba J (2001) Palaeozoic porphyry molybdenum-tungsten deposit in the Myszków area, southern Poland. Polish Geological Institute Special Papers 6: 1-87 Þlósarz J (1985) Stages and zonality of ore mineralization in Palaeozoic rocks of the environs of Myszków. Ann Soc Geol Pol 53(1-4): 267-288 Þlósarz J (1993) The main paragenetic stages for molybdenum mineralisation in the Palaeozoic rocks of the Myszków area and their importance to the formation of the ore deposits of that area (Eng Sum). Pol Tow Mineral Pr Spec 3: 123-128 Stein HJ (in press) Low-rhenium molybdenite by metamorphism in northern Sweden: recognition, genesis, and global implications. Lithos. Stein HJ, Markey RJ, Morgan JW, Hannah JL, Scherstén A (2001) The remarkable Re-Os chronometer in molybdenite: how and why it works. Terra Nova 13(6): 479-486 Close Chapter 7-30 7-30 New K-Ar, 87Sr/86Sr, REE, and XRF data for Tertiary volcanic rocks in the Sasa-Toranica ore district, Macedonia G. Tasev, T. Serafimovski, P. Lazarov Department of Mineral Deposits, Faculty of Mining and Geology, Goce Delcev 89, 2000 Stip, Macedonina Abstract. The latest K-Ar, 87Sr/86Sr, and REE data for samples from Sasa-Toranica ore district are presented. Whole rock XRF analyses confirm host rock composition as dacites, quartz-latites, trachyandesites and rhyolites. K-Ar absolute ages range from 31 to 14 Ma confirming Oligocene-Miocene age as previously determined by relative methods. 87Sr/86Sr ratios (0.70954 to 0.71126) suggest material is sourced from the contact zone between the lower crust and upper mantle where contamination of primary melt occured. New REE data including negative Eu anomalies along with previously determined La/Yb ratios ranging from 13.3 to 43.0 (Serafimovski 1990) confirm inferred material source. These new data reconfirm previous results, provide insight into the Tertiary magmatic history of the district, and suggest the exact origin of the material that produced the Tertiary magmatic rocks. Keywords. Sasa, Toranica, volcanic rocks, age, origin, contamination, Tertiary 1 Introduction Tertiary volcanic rocks in the Osogovo-Besna Kobila (SasaToranica ore district) area regionally strike NW-SE for 100 km on both sides of Macedonia-Bulgaria border. Volcanic rocks in the area occur as ~50 m thick elongate dykes oriented roughly east-west (260o). From the Osogovo Mountain to the Besna Kobila Mountain (Osogovo-LukeKaramanica), volcanic rocks are present as pyroclastics (Deve Bair), volcanic domes, dykes, necks and veins. Volcanic rocks at the Osogovo-Besna Kobila mountains cut the Paleozoic and Riphean-Cambrian metamorphic and igneous rocks and overlie Upper Eocene sedimentary sequences. The volcanics are mainly dacitic tuffs (Deve Bair), dacites, quartzlatites, rhyolites, trachyandezites, andesitelatites and occasionally lamprophyre veins (Sasa and Toranica localities). 2 Methodology After detailed sampling and preparation at the Faculty of Mining and Geology in Stip, samples were sent to the Geological Department, University of Padova, Italy for whole rock XRF analysis, Actlabs in Canada for ICP-MS and INAA REE analysis, the Geology Department, Royal Holloway University of London, U.K. for TIMS 87Sr/86Sr ratios, and the Geological Institute in Budapest, Hungary for K-Ar dating. 3 Results and discussion The new K-Ar, Sr isotope, REE, and whole rock XRF data from Sasa-Toranica host rocks provide insight into the composition, timing, and sources of volcanic activity in the region. Dacites in the Luke-Kiselica area occur from the Karamanica mountain to the southeast at the Osogovo mountain (Serafimovski and Alexandrov 1995). The dacites contain plagioclase (37% An), small amount of orthoclase, quartz, biotite and amphibole phenocrysts. Their matrix is holocrystaline to hypocrystaline with glassy domains. Apatite, sphene and zircon were identified as accessory minerals; while sericite, chlorite, kaolinite, carbonate and metallic minerals are present as secondary minerals. Quartzlatites are found near the springs of Lucka River and Kuprina Padina as dykes and at Samar and Karamanica as dykes and volcanic flows (Samar and Crcorija) over the volcano-sedimentary rocks. They are characterized by a porphyritic coarse grained texture with sanidine and plagioclase (35-40% An) phenocrysts, with secondary amphibole and augite phenocrysts. Sphene and zircon are accessory minerals. These rocks also contain metallic secondary minerals. Hialoandesites appear as necks and lava flows over the Upper Pliocene sediments at Gradeska Mountain. These rocks are porphyry-vitrophyric with phenocrysts of plagioclase (37% An), biotite, amphibole and augite; apatite and zircon occur as accessory minerals. Hypoabyssal and subvolcanic dacites and quartzlatites dominate the Sasa-Toranica zone (Osogovo). All the dacites and quartzlatites in the Sasa-Toranica zone experienced hydrothermal alteration. Dacites are holocrystalline with ~ 30% phenocrystals of andesine (5-16%), quartz (2-3%) and smal amount of orthoclase and coloured minerals (13-20%), mainly replaced by epidote, chlorite and carbonates. Hydrothermal alteration of andesites result in various new mineral assemblages. Illitization, seritization and propylitization dominante andesite alteration. Apatite, zircon, sphene and magnetite are present as accesory minerals, while pyrite, chalcopyrite, sphalerite and galena represent economic mineralization. Close 838 G. Tasev · T. Serafimovski · P. Lazarov Quartzlaties are the most common rocks in the zone mentioned above. They occur as elongated dykes a few kilometers in length. These rocks are characterized by large phenocrysts of sanidine, andezine and femic minerals biotite, amphibole and rarely augite. Sanidine crystals are fresh and quite large (up to 5-6 cm). Quartzlatites were intensively hydrothermaly altered. Transition rocks from quartzlatites to rhyolites are found at a few locations at Osogovo Mountain. Rocks with increased SiO2 content occur near the Sekirica Tower close to the Macedonian-Bulgarian state border. These rocks were intensly propylitized and hydrothermaly altered. The volcanic rocks from the Kozja River and Svinja River (Sasa Mine area) are dominantly dacites and quartzlatites. The volcanic rocks from this area are intensly propylitized and hydrothermaly altered. In addtion to previously mentioned secondary minerals, these rocks also contain ore minerals including pyrite, galena, sphalerite, sometimes chalcopyrite and occasionally traces of ceruzite, anglezite and malachite.Trachyandesites occur as small bodies at subvolcanic-volcanic levels in the SasaToranica zone and its western borders. They are characterized by porphyry structure (fine grained porphyry) and crystalized microlitic or microtrachytic matrix. Phenocrystals of large, around 2 to 3 mm, andezine, sanidine, biotite, augite and hornblende are present. Apatite, sphene, and zircon occurs as accessory minerals. In comparison to the quartzlatites, the trachyandesites are characterized by lower SiO2 concentrations. Similar rocks were identified in Pecovska Maala on the Osogovo Mountain on the Bulgarian side of the Bulgaria-Macedonian border. Lamprophyres occur as small dykes near Sredno Brdo and Toranica. They are dark grey to brown rocks with a fine-grained porphyrtic texture and glassy matrix. Pyroxene, amphibole and biotite pheocrysts are identified. Accessory minerals are apatite, sphene and zircon. Data obtained after geochemical analyses were entered into the computer software IGPET 2000 and Microsoft Excel; results are displayed in Table 1. Use of IGPET 2000 software facilitated determination of rock types by the Total Alkali Silica (TAS) classification scheme, their classification under the calk-alkaline or tholeiitic series of rocks (Fig. 1, 2), and subsequent interpretations based on the classifications. Graphical view of those determinations is presented in Figure 1. TAS classification indicate that the rocks of interest mostly plot in the areas that define dacites, trachydacites, trachyandesites and rhyolites. All analyzed rocks plot in the area of calk-alkali series. Selected samples were analyzed for rare earth element (REE) concentrations. The analyses were performed at the Active Labs, Canada. REE concentration data for four samples are presented in Table 2 and plotted in a chondrite-normalized spider diagram in Figure 2. From the spider diagram (Fig. 2) it can be seen that the rare earth elements in the Sasa-Toranica ore region have a decreasing trend. Comparing the left and right side of the diagram suggests there is a decrease in heavy rare earth elements, HREE with an atomic number higher than 63 (Eu), in comparison with light rare earth elements, LREE with an atomic number lower than 63 (Eu). The trend is typical as the product of fractionation of light Close Chapter 7-30 · New K-Ar, 87Sr/86Sr, REE, and XRF data for Tertiary volcanic rocks in the Sasa-Toranica ore district, Macedonia rare earth elements and their increase in comparison to the chondritic values. Fractionation occurred as a direct consequence of partial melting, which according to the angle of the line in the diagram was not of high intensity. Looking at the middle part of the diagram the value of Eu is slightly and negatively displaced from the “ideal” linear line between Sm and Gd defining a distinct negative Eu anomaly. A chondrite normalized, geometric mean calculation of the Eu anomaly is shown in Table 3. From the table it can be seen that Eu anomaly values are in range from 0.727669702 up to 0.828905716, and all are less than 1, which implies a negative Eu anomaly (Rollinson 1992). Eu anomalies are controled by presence 839 of feldspars. Eu2+ is compatible in plagioclase and K-feldspar, in contrast to the Eu3+ which is incompatible. Thus the removal of feldspar from a felsic melt by crystal fractionation or the partial melting of a rock in which feldspar is retained in the source will result in a negative Eu anomaly in the melt. Accordingly, the data for Eu in analyzed samples and its negative anomaly it can be concluded that Eu has been removed from the melt as a compatible Eu2+, by the processes of crystal fractionation or partial melting. With the analyses of strontium isotopes (Table 4) was performed to construct a general model of formation for rock complexes at the Osogovo Mountain (Sasa-Toranica ore field). Strontium isotope analyses of rock samples from the volcanic rocks from the Sasa-Toranica ore field results in strontium ratios that range from 0.70954 up to 0.71125. The results suggest the magma forming Neogene magmatic complexes at the Osogovo Mountain is a product of primary magmatic melt originating from the border zone between upper mantle and continental crust where mixing and contamination of primary magma occurred. The new data complies with previous 87Sr/86Sr data for Upper Tertiary calk-alkaline complexes formed in the Serb-Macedonian metallogenic province. 87Sr/86Sr ratios Close 840 G. Tasev · T. Serafimovski · P. Lazarov tration distribution of elements show that the magmatic rocks originated from one magmatic chamber but during different time intervals producing different rock types. K-Ar isotopic age data give Tertiary magmatic ages in the study area. Results of this study are shown in Table 5. The range of ages (Oligocene-Miocene) confirms the age determined by the relative methods. 4 Conclusion This study of the volcanic rocks in the Sasa-Toranica ore region identified the distinct and uniform chemical composition of these rocks. The rocks are characterized as dacites, trachydacites, trachyandesites and rhyolites based on the TAS scheme. New K-Ar ages range from 31.16 ± 1.40 to 14.0 ± 3.0 Ma confirming Oligocene-Miocene ages. Strontium isotope ratios and REE analyses identify magmatic material originated from the contact zone between the upper mantle and lower continental crust where certain contamination of primary melts occurred. References of samples from Kozuf Mountain range from 0.7088 to 0.7090 and those for volcanic rocks from the Rogozna range between 0.7074 and 0.7085 (Serafimovski 1990). Osogovo Tertiary igneous rocks are characterized by interesting distributions of Pb, Ba, Sr, Rb, Li, Cs and Be. Compared to Clark standard values Pb, Ba, Sr and Be are enriched while Li, Rb and Cs are similar to Clark standard values. Also, in magmatic processes it was noticed trend of increasing Li, Pb, Cs, Be, Rb and Ba concentrations going from fine-grained porphyry quartzlatites to coarse-grained porphyry quartzlatites (Serafimovski 1993a; Serafimovski et al. 2003). Tendencies in concen- Rollinson H (1992) Using Geochemistry Data: evaluation, presentation, interpretation. pp. 352. Prentice Hall, an imprint of Pearson Education, Harlow, England. Serafimovski T (1990) Metallogeny of the Lece-Halkidiki zone. Doctoral thesis, Faculty of Mining and Geology, Stip, p. 390 (in Macedonian) Serafimovski T (1993a) Structural - Metalogenic features of the LeceHalkidiki zone: Types of Mineral Deposit and Distribution. Faculty of Mining and Geology. Stip, Special Issue N. 2, 325 p, Stip. Serafimovski T, Aleksandrov M (1995) Lead-zinc deposits and occurrences in the Republic of Macedonia. Faculty of Mining and Geology, Stip, Special Issue 4, p. 387 (in Macedonian) Serafimovski T, Jelenkovic R, Tasev G (2003) Geodynamic Evolution and Metallogeny in the Southern Parts of the Balkan Peninsula. Geodynamics and Ore Deposit Evolution of the Alpine-BalkanCarpathian-Dinaride Province. Final GEODE-ABCD Workshop. Programme and Abstracts. pp. 50. Seggauberg, Austria. Serafimovski T, Jelenkovic R, Tasev G, Lazarov P (2003) Mineral Deposits Related to Tertiary Magmatism in the Southern Part of the Balkan Peninsula. Geologica Macedonica, Volume 17, pp. 19-23, Stip. Tasev G (2003) Polymetalic mineralizations related to the Tertiary magmatism in the Republic of Macedonia. Faculty of Mining and Geology, Stip. Master thesis, p. 176. (in Macedonian) Close Chapter 7-31 7-31 Sources of rhenium and osmium enrichment in fumaroles, sulphide sublimates and volcanic rocks from the Kudriavy volcano Svetlana G. Tessalina, Françoise Capmas, Jean-Louis Birck, Claude-Jean Allègre Laboratoire de Geochimie et Cosmochimie, Institute de Physique du Globe, 4 pl. Jussieu, 75252 Paris, France Marina A. Yudovskaya, Vadim V. Distler, Ilya V. Chaplygin Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM), RAS, Moscow, Russia Abstract. Rhenium loss through magma degassing could be partly balanced by rhenium enrichment in fumarolic magmatic gases and Re-bearing precipitates, as may be the case for the Kudriavy volcano associated with an active subduction zone. The relatively unradiogenic 187Os/188Os isotope ratios (0.122 up to 0.152) and high Os contents (averaging 0.6 ppb) of fumarolic gas condensates imply that significant Re and Os are remobilised from depleted MORB mantle. Involvement of a Re-rich component is evident from high Re concentrations in high-temperature gas condensates, ranging from 7 to 200 ppb. Indeed, Re-rich Os-poor components such as organic-rich subducted sediments and volcanic rocks do not significantly shift the isotopic composition of fumarolic products. The relatively radiogenic composition of the dacite-andesite-basaltic arc volcanics (187Os/188Os ratio up to 0.58), however, could result from significant Os (and Re) input from subducted sediments. Keywords. Re-Os, subduction zone, rheniite, Kurile Islands, Kudriavy loor sediments are almost completely subducted beneath Kurile Island arc (Von Huene and Scholl 1991). The lower part of the sedimentary section consists of the Cretaceous chert (120 to 92 Ma) of carbonate composition with abundant siliceous organisms. The radiolarian and diatom ooze accumulated during the middle to late Miocene (14 to 5 Ma) represents the upper part of the sedimentary section (Bailey 1993). The Kudriavy volcano has been passively degassing at 500-940° C, as recorded in fumarole activity for the last 100 years. The unique occurrence of rhenium disulphide (rheniite ReS2) has been discovered around high-temperature fumaroles on the Kudriavy volcano, together with elevated PGE contents. 3 1 Subduction zones are major sites of continental crust formation and elemental recycling between the mantle and crust. The great difference between Re contents in degassed subaerially deposited arc volcanics (~0.19 ppt, Lassiter 2003) and in melt inclusions from undegassed primary arc volcanics (~2 ppb, Sun et al. 2003) requires Re loss during magma degassing. Substantial Re loss from arcs can be partly balanced by high Re contents in magmatic gases and the presence of pure Re sublimates in arc systems (Korzhinsky et al. 1994), as reported for the Kudriavy volcano, above an active subduction zone in the Kurile Islands. The Re-Os systematics should provide important information on the source of Re-rich magmatic volatiles and sulphide precipitates with regard to contributions from the mantle, crust, subducting slab, and seawater, because of compatible Os and slightly incompatible Re behaviour. 2 Sample description and analytical methods Introduction Tectonic setting of the Kudriavy volcano The Kurile Islands are the result of Pacific plate subduction beneath the Eurasian plate. Subducted Pacific plate comprises oceanic crust (MORB), oceanic lithospheric mantle and associated sediments. The 400 m-thick seaf- In order to understand mechanisms for rhenium and osmium enrichment, we undertook integrated studies of fumarolic gases, sulphide sublimates and volcanic rocks at Kudriavy. The sulphide sublimates are represented by molybdenite (MoS2), rheniite (ReS2) and Pb-Bi sulphosalt. The suite of volcanic rocks ranges from basaltic to dacitic in composition. Two fractions of fumarolic gas condensates were analysed: = 0.2 mm (Fraction 1) and bulk fumaroles condensates (Fraction 2). Re and Os concentrations and Os isotopic compositions was determined by negative thermal ionisation mass spectrometry (NTIMS) on a Finnigan MAT 262 at the IPGP. Analytical procedure has been described previously (Birck et al. 1997). 4 Re-Os isotope systematics The Re contents in Kudriavy volcano rocks range from 3.5 to 17 ppb (Fig. 1) averaging 7 ppb, which is about 20 times higher than the estimated average Re abundance for arc lavas (0.3 ppb) and 3 times higher than for melt inclusions from primitive arc lavas, southern Pacific (Sun et al. 2003). The Os contents (ave. 11 ppt.) are similar to those of MORB (Roy-Barman and Allègre 1994). The 187Os/ 188Os ratios vary from 0.205 in basalt to 0.588 in dacite with an average of 0.385. This range of Os isotopic com- Close 842 Svetlana G. Tessalina · Françoise Capmas · Jean-Louis Birck · Claude-Jean Allègre · Marina A. Yudovskaya · Vadim V. Distler · Ilya V. Chaplygin position in volcanic rocks could be explained by mixing of an unradiogenic MORB-type reservoir with more radiogenic components. Our mass balance calculations are based on the following parameters (Table 1). The unradiogenic MORB-type component could represent Os-poor oceanic crust. The Os contribution from high-Os depleted mantle is limited to 10% in basalts and almost negligible in felsic volcanic rocks formation. Fluid– saturated sedimentary slab from the subduction zone can be considered as the more radiogenic end-member. Thus, the relatively radiogenic Os signatures for Kudriavy volcanic rocks could be explained by significant Os and Re input (up to 50 %) from slab-derived fluids and melts contaminated by more radiogenic (0.29 to 0.64 for 187Os/188Os) organic-rich sediments from the subducting Pacific plate (Peucker-Ehrenbrink et al. 1995) (Fig. 2) . Previous studies of fumarolic gases using H, He and C isotopic systematics (Taran et al. 1995; Fischer et al. 1998) showed that the subducted slab and mantle wedge were the main sources for fluids in the Kudriavy volcanic system. The Re-Os contents and isotope composition of gas condensates vary significantly depending on the method of analytical sampling. Fractions = 0.2 mm (Fraction 1) are characterised by high Re and Os contents (average values are 85 ppb and 0.6 ppb, respectively) and unradiogenic 187Os/ 188Os compositions (0.122 to 0.152). In contrast, bulk condensates (Fraction 2) are characterised by lower Re and Os concentrations (~0.4 ppb Re and 2-37 ppt Os) and slightly more radiogenic Os isotope compositions (0.12 to 0.45), similar to those of the hosting volcanic rocks. This difference can be explained by chemical procedure (incomplete digestion of Fraction 2 due to the absorption of Re and Os complexes by coarse sulphur particles coagulated during acid decomposition), or by the presence of rocks particles in a Fraction 2. Thus, the data obtained for Fraction 1 can be considered as representative of bulk gas condensate composition. The relatively unradiogenic 187Os/188Os ratios (0.122 to 0.152) and high Os contents (averaging 0.6 ppb) for fumarolic gas condensates imply that a significant part of Re and Os was remobilised from depleted MORB mantle (Table 1). Involvement of a Rerich component is evident from high Re concentrations in gas condensates, ranging from 7 to 200 ppb. But this radiogenic, Re-rich and Os-poor component, possibly organic-rich subducted sediments (up to 20%) and volcanic rocks (up to 20%), does not significantly shift the Os isotopic composition of fumarolic products. Rheniite is highly radiogenic due to its high Re content (74.5 wt.% Re). Repeated analyses of two rheniite samples provide model ages of 79±11 yr, which agree with the known 100 year period of fumarolic activity. The initial 187Os/188Os ratio is not well defined (0.32±0.15), but appears to be higher than ratios associated with gas condensates. The Pb-Bi sulphosalts have much lower Re contents (~250 ppb) and relatively unradiogenic osmium isotopic compositions (0.125 to 0.176), similar to that of gas condensates. 5 Conditions of Re enrichment Experimental work has shown that rhenium can be mobilized by high-temperature, saline, and sulphide-poor hydrothermal solutions (Xiong and Wood 1999). According to these experimental data, Re concentrations at 510°C in 0.5 m KCl solution are about 8 x 10-6moles/kg H2O (~1 ppm). Thus, Re could be easily remobilised from the host rocks and sediments by high temperature (700-940°C) Close Chapter 7-31 · Sources of rhenium and osmium enrichment in fumaroles, sulphide sublimates and volcanic rocks from the Kudriavy volcano fumarolic gases with 0.5 mol% of Cl (Taran et al. 1995). On the other hand, Re and Os enrichment in fumarolic gases could depend on melt-vapor fractionation processes. Deposition of Re-bearing sulphide could be induced by subaerial conditions, which exclude the possibility for dissolution of Re-complexes in water. 6 Importance for Re resources Until now, molybdenite-bearing Cu-porphyry deposits have been the primary source of Re. High Re concentrations in molybdenite from Cu-porphyry environments have been attributed to mantle involvement in a subduction setting (Stein et al. 2003; Zimmerman et al. 2003) The occurrence of high levels of rhenium in gases and sulphides from the Kudriavy volcano may represent a new and unexplored resource for Re. The Re resources of Kudriavy volcano are still under considerations. References Bailey JC (1993) Geochemical history of sediments in the northwestern Pacific Ocean. Geochem. J 27: 71-92 Birk JL, Roy-Barman M, Capmas F (1997) Re-Os isotopic measurements at the femtomole level in natural samples. Geostandards newsletter 20: 19-27 Fischer TP, Giggenbach WF, Sano Y, Williams SN (1998) Fluxes and sources of volatiles discharged from Kudriavy, a subduction zone volcano, Kurile Islands. Earth Planet Sci Lett 160: 81-96 Korzhinsky MA, Tkachenko SI, Shmulovich KI, Taran YA, Steinberg GS (1994) Discovery of a pure rhenium mineral at Kudriavy Volcano. Nature 369: 51-52 843 Lassiter JC (2003) Rhenium volatility in subaeral lavas: constraints from subaeral and submarine portions of the HSDP-2 Mauna Kea drillcore. Earth Planet. Sci. Lett. 214: 311-325 Peucker-Ehrenbrink B, Ravizza G, Hofmann AW (1995) The marine 187Os/188Os record of the past 80 million years. Earth Planet Sci Lett 130: 155-167 Roy-Barman M, Allègre CJ (1994) 187Os/186Os ratios of mid-ocean ridge basalts and abyssal peridotites. Geochim Cosmochim Acta 58: 5043-5054 Stein H, Scherstén A, Hannah J, Markey R (2003) Sub-grain scale decoupling of Re and 187Os and assessment of laser ablation ICPMS spot dating in molybdenite Geochim Cosmochim Acta 67: 3673-3686 Sun W, Benett VC, Eggins S, Kamenetsky VS, Arculus R (2003) Enhanced mantle-to-crust rhenium transfer in undegassed arc magmas. Nature 422: 294-297 Taran YuA, Hedenquist JW, Korzhinsky MA, Tkachenko SI, Shmulovich KI (1995) Geochemistry of magmatic gases from Kudriavy volcano, Iturup, Kuril Islands. Geochim Cosmochim Acta 59: 1749-1761 Von Huene R, Scholl DW (1991) Observations at convergent margins concerning sediment subduction, subduction erosion, and the growth of continental crust. Reviews in Geophysics 29: 279316 Widom E, Kepezhinskas P, Defant M (2003) The nature of metasomatism in the sub-arc mantle wedge: evidence from Re-Os isotopes in Kamchatka peridotite xenoliths. Chemical Geology 196: 283-306 Xiong Y, Wood SA (1999) Experimental determination of the solubility of ReO2 and the dominant oxidation state of rhenium in hydrothermal solutions. Chem Geol 158: 245-256 Zimmerman A, Stein H, Markey R, Fanger L, Heinrich C, von Quadt A, Peytcheva I (2003) Re-Os ages for the Elatsite Cu-Au deposit, Srednogorie zone, Bulgaria: in Eliopoulos, D.G. et al. (eds), Mineral Exploration and Sustainable Development, Millpress, Rotterdam: 1253-1256 Close Close Chapter 7-32 7-32 Muluozhai REE deposit in Sichuan Province, China: Stable isotope data and their implications on the dynamics of mineralization Shihong Tian, Zengqian Hou, Tiping Ding Institute of Mineral Resources, Chinese Academy of Geological Sciences, Beijing 100037, China, and Key Laboratory on Isotope Geology, Ministry of Land and Resources, Beijing 100037, China Yuling Xie Civil & Environmental Engineering School, Beijing University of Science and Technology, Beijing 100083, China Zhongxin Yuan, Ge Bai, Tianren Zou Institute of Mineral Resources, Chinese Academy of Geological Sciences, Beijing 100037, China Abstract. The Muluozhai REE deposit, located about 60 km to the southwest of the Mianning County, Sichuan Province, is the third largest light REE deposit in Sichuan. The Muluozhai REE deposit is tectonically located on the northern Jinpingshan Mountains, a Cenozoic intracontinental orogenic belt in southwestern China. The authors analyzed the essential ores from two tunnels for their carbon, hydrogen, oxygen, and sulfur isotopic compositions of the mineralizing fluid. The δ13CV-PDB values of fluid from fluid inclusions of the quartz and fluorite vary from - 2.5 to - 9.0 per mil, which show characteristics of mantle-derived carbon. The δDV-SMOW values of fluid from fluid inclusions of the calcite, quartz, fluorite, and bastnaesite range from - 63 to - 87 per mil, which are characteristics of mantlederived hydrogen. The δ34SV-CDT values of barite and galena vary in a narrow range of + 0.1 to + 2.2 per mil and - 8.6 to - 9.3 per mil, respectively, showing the isotopic characteristics of mantle-derived sulfur. The δ13CV-PDB values and the δ18OV-SMOW values of calcite range from - 6.6 to - 6.8 per mil and from + 8.4 to + 9.1 per mil, respectively, which are fallen into the range of the “primary carbonatites”, showing the carbon and oxygen in the ores of the Muluozhai ore veins were mainly derived from depths. The stable isotopic data suggest a mantle source for the rare earth elements mineralization and a dynamic process involving mantle materials and tectonics. Keywords. Rare earth element deposit, stable isotopes, mantle source, mineralization dynamics, Muluozhai in Sichuan Province 1 Introduction The Muluozhai REE deposit (28°22’ N Lat. and 101°50’ E Long.), located about 60 km to the southwest of the Mianning County, Sichuan Province, is the third largest light REE deposit in Sichuan. Along with other REE deposits in the Panzhihua-Xichang area, it forms one of the three major REE deposit producing regions in China. Although known since the 1960s, it has not attracted nearly as much interest as the Maoniuping and the Daluchao REE-deposits in the Panxi REE ore belt, and, therefore, only little research has been performed concerning its geological characteristics, geochemistry, isotopic geochemistry, mineralogy, and fluid inclusions. Because it is an important part of the Panxi REE ore-forming belt and is situated at the eastern margin of the Tibetan Plateau, it is necessary to understand regional metallogenic rules and the collision between the Indian plate and the Eurasia plate. In this paper, we present systematic studies on the characteristics of S, C, O, and H isotopes of the ores to ascertain the sources of the mineralizing fluids and the dynamic process related to the mineralization. 2 Geologic setting and REE mineralization The Muluozhai REE deposit is tectonically located on the northwest margin of the Panxi (Panzhihua-Xichang) rift zone at the western side of the Yangtze Platform (Fig. 1). According to Luo et al. (1985), the Panxi rift zone formed on the Yangtze platform starting in the early Paleozoic. Deposition continued during the late Paleozoic into the Mesozoic and ended in the early Cenozoic with the beginning of the Himalayan Orogeny. The Panxi rift was bordered by the Ganluo-Xiaojiang Fault to the east and Qinghe-Chenghai Fault to the west. It extends north-south for over 300 km and reaches a width of about 100 km. Large amounts of alkali-rich ultramafic, basic, and intermediate-acid rocks with a great deal of REE were intruded or erupted in the Panxi rift zone and its neighboring areas. In the region, the Devonian, Permian, Triassic and Jurassic strata are distributed scatteredly because of the destruction of the developed igneous rocks. The latter are distributed extensively in the region and the main rocks are Indosinian quartz diorite, granite, and Yanshanian alkali-feldspar granite. On the basis of orebody distribution, three kinds of ores have been identified: (i) massive fluorite-bastnaesite, (ii) impregnated, and (iii) banded. The ore minerals are mainly bastnaesite, whereas the gangue minerals include fluorite, barite, calcite, feldspar, quartz, mica and aegirineaugite. The textures and structures are allotriomorphic inequigranular, tabular, subhedral, and massive, banded, respectively. The wall-rock alteration is characterized by Close 846 Shihong Tian · Zengqian Hou · Tiping Ding · Yuling Xie · Zhongxin Yuan · Ge Bai · Tianren Zou clusions in quartz and fluorite was released by the decrepitation method and collected in sample tube at liquid N2 temperature. All SO2, CO2, and H2 were analyzed using a Finnigan MAT 251 mass spectrometer at the Key Laboratory on Isotope Geology, Ministry of Land and Resources. Analytical reproducibility in this study is ± 0.2 per mil for C, O, and S isotopes, and ± 2 per mil for H isotope. 3.2 Results contact metamorphism and hydrothermal alteration, which includes sericitization, pyritization, baritization, and carbonatization. 3 Stable isotope analysis 3.1 Experiments Sulfur, carbon, oxygen, and hydrogen isotopes of mineral separates from the Muluozhai deposit have been analyzed. SO2 was prepared from the samples for sulfur isotope analysis with the method of Robinson and Kusakabe (1975). For oxygen and carbon isotope analysis, calcite was reacted with phosphoric acid at 25° (McCrea 1950) to release CO2. The δ18OV-PDB values of calcite samples were directly obtained from the δ18O values of their CO2 against the CO2 of PDB. For converting the δ18OV-PDB to δ18OV-SMOW, the equation by Friedman and O’Neil (1977) was used, δ18OV-SMOW = 1.03086 · δ18OV-PDB + 30.86. For analysis of hydrogen isotopes, the water in fluid inclusion was released by the decrepitation method. Then, the water was reacted with Zn at 400° to produce H2 (Coleman et al. 1982), which was collected in a sample tube with activated charcoal at liquid N2 temperature. For the analysis of carbon isotopes from the fluid, the CO2 in fluid in- Sulfur isotope analyses have been done on 3 barite and 3 galena samples. The δ34SV-CDT values vary in a narrow range of + 0.1 to + 2.2 per mil with an average of + 0.8 per mil for the barite, and - 8.6 to - 9.3 per mil with an average of - 9.0 per mil for the galena, respectively. According to the theory by Ohmoto (1972), the δ34SV-CDT values of ore-forming fluid in the Muluozhai deposit vary from - 9.0 to + 0.8. On account of barite more than galena, the δ34SV-CDT values of ore-forming fluid is more than 0 per mil, but less than + 2.2 per mil, which shows the isotopic characteristics of mantle-derived sulfur (Lu 1986). Five calcite samples were analyzed for their carbon and oxygen isotopes. The δ13CV-PDB values and the δ18OV-SMOW values range from - 6.6 to - 6.8 per mil with an average of - 6.7 per mil and from + 8.4 to + 9.1 per mil with an average of + 8.7 per mil, respectively. These values fall into the range of “primary carbonatites”, showing that carbon and oxygen in the ores of the Muluozhai deposit were mainly derived from the mantle (Keller and Hoefs 1995). Carbon isotope analyses of fluid from fluid inclusions were made on 2 quartz and 5 fluorite samples. The δ13CVPDB values range from - 2.5 to - 3.6 per mil for quartz with an average of - 3.1 per mil and - 5.5 to - 9.0 per mil for fluorite with an average of - 7.1 per mil. Quartz and fluorite samples show narrow ranges in δ13CV-PDB values, which are close to the estimated value of mantle carbon (Pineau and Methez 1990). Hydrogen isotope analyses of fluid from fluid inclusions have been done on 2 quartz, 5 fluorite, 5 calcite, and 5 bastnaesite samples. The δDV-SMOW values range from 69 to - 76 per mil for the quartz with an average of - 73 per mil, - 73 to - 87 per mil for the fluorite with an average of - 81 per mil, - 70 to - 82 per mil for the calcite with an average of - 76, and - 63 to - 86 per mil for the bastnaesite with an average of - 71 per mil. All minerals show a narrow range in δDV-SMOW values that fall close to the estimated value (-60 to -80 per mil) of mantle hydrogen (Mao and Li 2004). 4 Discussion and conclusions REE mineralizations in rift belts are characterized by multiphase and multistage processes. Mineralizing types Close Chapter 7-32 · Muluozhai REE deposit in Sichuan Province, China: Stable isotope data and their implications on the dynamics of mineralization vary through time. Correspondingly, geological, mineralogical, petrological, and geochemical features differ also. For example, in the Liaodong rift belt, REE mineralizations in pegmatites and migmatites formed during an early stage of rift formation, REE-Fe-rich formation of metamorphism volcano-sedimentary rocks during the midstage of rift formation, and REE-U-rich aegirine and aegirine-nepheline syenites are related to the postrift evolution (Chen 1984). In the Bayan Obo rift belt, Inner Mongolia, the famous Bayan Obo Fe-Nb-REE ore deposit formed during the Proterozoic, in the evolved rift (Bai 1996) and REE-rich hydrothermal vein and skarn deposits formed during the Caledonian and Hercynian. These late mineralizations reworked the Proterozoic mineralizations (Yuan et al. 1992). The REE mineralizations of the Panxi rift belt are also characterized by multiphase and multistage processes. REE-rich nordmarkites, alkali granites, syenite porphyries, and albitites. formed during the Hercynian-Indosinian epoch in the developed stage of the Panxi rift, which were mostly associated with alkaline and basic bedded rocks in the region. Affected by the collision between the Indian plate and the Eurasia plate, the rift closed during the Himalayan epoch and changed into an intracontinental orogenic belt, i.e. the Jinpingshan Orogen (Fig. 1), which was formed during Cenozoic and became the eastern margin of the Tibetan Plateau (Burchfiel et al. 1995). The Muluozhai REE deposit is located in the transitional zone between the Panxi rift and the LongmenshanJinpingshan orogenic zone, where the Yangtze plate penetrated as a wedge into the crust at Longmenshan, resulting in a Moho dislocation, thereby inducing partial melting of the mantle materials (Xu et al. 1999). This tectonic environment may have caused intensive faulting and magmatism, possible metamorphic dehydration and upwelling of mantle fluids along the deep faults in the western margin of the Yangtze. The fluids that were responsible for the formation of the Muluozhai REE deposit have S, C, O, and H isotopes similar to mantle or mantle-derived rocks. Acknowledgements This work was supported by grants from the State Science and Technology Commission (contract No. 2002CG412610 and G1999043211) and China Natural Sciences Foundation (Grant No. 40425014). We thank Luo Yaonan of Sichuan Bureau of Geology and Mineral Resources and Pu Guangping, Yu Bo and other engineers of the No. 109 Geological Team during our field investigation. We are grateful to Professor Wang Denghong and 847 Professor Chen Wenming at the Institute of Mineral Resources, CAGS, for their constructive suggestion. We also thank Professor Wan Defang, Senior Engineer Li Jincheng, Senior Engineer Bai Ruimei, and Engineer Luo Xurong at the Key Laboratory on Isotope Geology, Ministry of Land and Resources, for their performance of analyses. References Bai G, Yuan ZX, Wu CY (1996) Geotectonic setting of the Bayan Obo deposit, Inner Mongolia. Acta Geosci Sinica 17 (supl): 1-8 (in Chinese with English abstract) Burchfiel BC, Chen, ZL, Liu, YP, Royden LN (1995) Tectonics of the Longmen Shan and adjacent regions, central China. Intern Geol Rev 37: 661-735 Chen RD (1984) A Proterozoic rift basin-Liaodong rift. Liaoding Dizhi 2: 125-133 (in Chinese with English abstract) Coleman ML, Sheppard TJ, Durham JJ, Rouse JE, Moore GR (1982) Reduction of water with zinc for hydrogen isotope analysis. Anal Chem 54: 993-995 Friedman I, O’Neil JR (1977) Compilation of stable isotope fractionation fraction factors of geochemical interest. In: Fleischer M (ed) Data of geochemistry. Sixth Edition. Geol Surv Profl Pap US P. 117 Keller J, Hoefs J (1995) Stable isotope characteristics of recent natrocarbonatites from Oldoinyo Lengai. In: Bell K (ed) Carbonatites volcanism: Oldoinyo Lengai and Petrogenesis of Natrocarbonatites. LAVCEI Proceeding in Volcanology. LAVCEI, 113-123 Lu CW (1986) Stable Isotopic geochemistry. Chengdu Univ Technol, Publ House, Chengdu, pp. 40-43 (in Chinese) Luo YN (1985) Panzhihua-Xichang paleo-rift zone, Southwest of Sichuan. In: Zhang YX (ed) Contribution to Panzhihua-Xichang rift, China. Geol Publ House, Beijing, pp. 1-25 (in Chinese with English abstract) Mao JW, Li XF (2004) Mantle-derived fluids in relation to ore-forming and oil-forming process. Mineral Deposits 23: 520-532 (in Chinese with English abstract) McCrea JM (1950) On the isotope chemistry of carbonates and a paleotemperature scale. J Chem Phys 18: 849-857 Ohmoto H (1972) Systematics of sulfur and carbon isotopes in hydrothermal ore deposits. Econ Geol 67: 551-578 Pineau F, Methez EA (1990) Carbon isotopes in xenoliths from the Hualalai volcano, Hawaii, and the generation of isotopic variability. Geochim Cosmochim Acta 54: 2117-2127 Robinson BW, Kusakabe M (1975) Quantitative preparation of sulphur dioxide for 34S/32S analyses from sulphides by combustion with cuprous oxide. Anal Chem 47: 1179 Wang DH, Yang JM, Yan SH, Xu J, Chen YC, Pu GP, Luo YN (2001) A special orogenic-type rare earth element deposit in Maoniuping, Sichuan, China: Geology and Geochemistry. Resource Geol 15: 177-188 Xu ZQ, Yang JS, Jiang M, et al., (1999) Continental subduction and uplifting of the orogenic belts at the margin of the Qinghai-Tibet Plateau. Earth Sci Front 6: 139-150 (in Chinese with English abstract) Yuan ZX, Bai G, Wu CY, Zhang ZQ, Ye XJ (1992) Geological features and genesis of the Bayan Obo REE ore deposit, Inner Mongolia, China. Appl Geochem 7: 429-442 Close Close Chapter 7-33 7-33 Stable isotope composition of the Dalucao rare earth deposit in western Sichuan Wan Defang, Tian Sihong Institute of Mineral Resources, Chinese Academy of Geological Sciences, Beijing 100037, China Luo Mei Chengdu University of Technology, Chengdu 610059, Sichun China Jiang Shaoyong Department of Earth Sciences, Nanjing University, Nanjing 210093, Jiangsu, China Abstract. Ore-forming solutions and the origin of mineralizing material in the Dalucao rare earth deposit were studied by means of H, O, C, and Si isotope analyses. The δ13C of the bastnasite range narrowly from -8.1‰ to-8.0‰, while the δD values range from -89‰ to -79‰. The quartz δ30Si of the orebody is -0.3‰, and the δD and δ18O of the quartz-fluid inclusion range from -87‰ to +6.0‰, respectively. The δD and δ18O values of the fluorite-fluid inclusion in the ore body are -99‰ to -11.6‰, respectively. The study shows that the compositions of hydrogen and oxygen isotopes in oreforming fluid of Dalucao rare earth deposit lie in the region between magmatic water and meteoric water. Therefore the ore-forming fluid was mixed from magmatic and meteoric water. The carbon isotopic features suggest that carbon of the bastnasite was from the mantle, carbon of fluorite-fluid inclusions in the ore body was from a mixture carbon source, and carbon of quartz-fluid inclusions was from the mantle. Keywords. Stable isotope composition, quartz-fluid inclusion, fluorite-fluid inclusion, rare earth deposit, Dalucao 1 Introduction The Dalucao rare earth ore deposit, one of the largest rare earth ore deposits of China, is located 20 km southwest from Dechang county town, Sichuan Province. It covers an area of about 3 km2. Tectonically, the deposit is situated in the middle part of the Panxi rift belt, a famous epicontinental rift in the western border of the Yangtze platform. Rare earth ore bodies of Dalucao rare earth ore deposit are mainly hosted in the aegirine-augite syenite, bordering to quartz diorite, and are related to hydrothermal activations associated with the quart diorite. Geological and geochemical features demonstrate that the deposit is a hydrothermal deposit that formed at medium to low temperature. Based on the C, H, O, and Si isotopes and in the context of the regional geology and tectonics of the Panxi rift, it is further suggested that the source rocks of the ore-bearing aegirine-augite syenite are probably early-formed alkali-rich rocks of the Hercynian epoch that are present at depth. The ore-bearing aegirineaugite syenite was mostly formed by remelting, ascend- ing, and emplacement of the source rocks under the activation of mantle plume and tectonic mobilization in the Himalaya period. 2 Geological survey of Dalucao rare earth deposit Dalucao rare earth ore deposit is located in the middle part of the Panxi rift belt, which is a famous epicontinental rift in the western border of the Yangtze platform. The distributive strata of the deposit are mainly Previndean system, Vindean-Cambrian system and Jurassic system (Fig. 1). Previndean strata are mainly composed of Yanbian formation strata of Huili group, Vindean-Cambrian strata are consisted of Guanyinyan formation and Dengying formation, and Jurassic system is made up of Baiguowan group and Yimen formation. The deposit is situated in part between Shuenhe syncline and Xincun syncline, located at intersections with the Dalucao (F1), Nanmuhe (F7)and Xincun syncline, located at intersections with the Dalucao (F1), Nanmuhe (F7) and Zhangmenzha (F6) faults. The regional structural framework was mainly made up of SN-striking, NW-striking and NE-striking faults. The ore body is cut through by Dalucao fault (F1), and affected by the fault. Outcropping magmatic rocks in the mineral district include quartz diorites of the Jinning epoch, alkali granites of the Indo-Chinese epoch, aegirine-augite syenites, and syenites of the Himalaya epoch. The Daluxiang quartz diorite (853Ma) is emplaced into the Presinian Huili group and is covered by the Jurassic Baiguowan formation. Rare earth ore bodies are hosted in the 64.9 Ma old aegirine-augite –syenite, which is emplaced in Daluxiang quartz diorite. The major ore body is lens-shaped and shows net-veining and mineralization of structural fissures in the aegirine-augite syenite. The major mineral assemblage in the ore is made up of bastnasite, celestobarite, barytocelestite, aegirine-augite, fluorite, calcite, quartz, mica, minor sulphide, and rare earth titanite. Close 850 Wan Defang · Tian Sihong · Luo Mei · Jiang Shaoyong 3 Geochemistry of stable isotopes 3.1 Signature of silicon and oxygen isotopic compositions We measured the silicon and oxygen isotope compositions of many wall rock and quartz samples from the rare earth ore body in order to elucidate the origin and the evolution of ore-forming fluid in the deposit. Table 1 shows the Si and O isotope compositions of the deposit. Quartz δ18O in quartz diorite has values around 9.1‰ to 9.3‰, and the quartz diorite δ18O is +7.1‰. It is suggested that the quartz diorite belongs the granitoid (Talor 1968). The quartz δ30Si in quartz diorite is 0.0‰, hornblende -0.2‰ and the quartz diorite δ30Si 0.1‰, which is close to the granitoid average. The δ18O and δ30Si of quartz in the ore body are respectively +10.1‰ and -0.3‰, the δ18OH2O of fluid inclusions in quartz is 6.0‰, and bastnasite δ18O is from +19.2‰ to +19.3‰. 3.2 Signature of H, O and C isotopic compositions Table 2 displays H, O, and C isotope compositions of mineral-hosted fluid inclusions in the REE deposit. The quartz δD in quartz diorite is -96‰ and the δ13CPDB of its CO2 is -11.9‰. δD and δ18OH2O of quartz in the ore body are respectively -87‰ and +6.0‰, the fluite inclusion δ13CPDB of quartz in the ore body is -8.4‰, which show the H, C and O isotope compositions of the magmatic water. Close Chapter 7-33 · Stable isotope composition of the Dalucao rare earth deposit in western Sichuan Fluorite δD of in the ore body range from -119‰ to 83‰, averaging around -99‰. Its δ18OH2O range from 13.6‰ to -9.6‰, with an average of -11.6‰, indicating that the ore-forming fluid is a mixed fluid of the magmatic water and the meteoric water. The fluid inclusion δD of the bastnasite range from 89‰ to -79‰, showing that the ore-forming fluid is a magmatic water. The bastnasite δ13CPDB is about -8.0‰, indicating the characteristic of mantle carbon. 851 fluorites in the ore body was from a mixed carbon source, and the fluid inclusion carbon of quartz was from mantle. The rare earth partitioning of the bastnasite, the ore and the alkali complex is all Ce>La>Nd, and Ce-rich, showing the mantle features of the metallogenetic material in the rare earth deposit. The 134Nd/144Nd of the rare earth deposit range from 0.512297 to 0.512313, indicating that the rare earth elements were mainly derived from the upper mantle. 4 Conclusions 3.3 Derivation of the metallogenetic material In the graph of δ18O vs δD for ore-forming fluids (Fig. 2), it is evident that the fluid-inclusion water in quartz belong to magmatic water, and the fluid-inclusion water in fluorite belong to meteoric water, indicating that the oreforming fluid was a mixed fluid of the magmatic water and the meteoric water. According to the Si isotope compositions of the ore body quartz and whole rock, it can help us infer that the Si may be from a deep magmatic source area. The carbon isotopic features suggest that carbon of the bastnasite was from mantle, the fluid inclusion carbon of The rare earth elements of Dalucao deposit are mainly from the mantle. Si may also be from a deep magmatic source. The ore-forming fluid was a mixture fluid of the magmatic water and the meteoric water. The carbon of bastnasite was deduced from the mantle and the carbon of the ore-forming fluid in bastnasites was from a mixture carbon source area. It is further suggested that the source rocks of the orebearing aegirine-augite syenite are probably early-formed alkali rich rocks in Triassic period or Carboniferous-Permian period. The ore-bearing aegirine-augite syenite was mostly formed by remelting, ascending and emplacement of the source rocks under the activation of mantle plume Close 852 Wan Defang · Tian Sihong · Luo Mei · Jiang Shaoyong References and tectonic mobilization in the Tertiary-Quaternary period. C, H, O, and Si isotope compositions of the deposit indicate that Dalucao rare earth deposit was a hydrothermal vein type deposit of the rich light rare earth element, which was formed in the Tertiary-Quaternary period. Clayton RN, O’Neil JR, Mayeda TK (1972) Oxygen isotope exchange between quartz and water. J Geophys Res 77: 3057-3059 Ding T (1994) Silicon isotope geochemistry. Geol Pub House, Beijing, 23-30 Matsuhisa Y, Goldsmith JR, Clayton RN (1979) Oxygen isotopic fractionation in the systemquartz-albite-water. Geochim. Cosmochim Acta 43: 1131-1140. O’Neil JR, Taylor HP (1967) The oxygen isotope and cation exchange chemistry of feldspars. Am Mineral 52: 1414-1418 Pu G (2001) REE mineralization evolution in Panxi rift and basic metallogenic feature in Himalaya age. Study on the endogenetic minerallization in Hymalaya age, China. China Seismol Press, Beijing, 104-113 (in Chinese) Shen W (1987) Geology of stable isotope. Atom Ener Pub House, Beijing: 123-125 (in Chinese) Tang L, Yang D, Liu S, Wang Z, Ye X, Chen Z (1985) The double structural feature of Panxi rift. The collected works of Panxi rift, China. Geol Pub House Beijing: 72-84 (in Chinese) Taylor HP (1968) 18O/16O ratios coexisting minerals in glancophanebearing metamorphic rock: Bull Geol Soc Am 79: 1727-1756 Yuan Z, Shi Z, Bai G, Wu C, Li X (1995) Mouniuping REE deposit, Mianning County, Sichuan Province. China Seismol Press, Beijing: 103-105 (in Chinese) Close Chapter 7-34 7-34 Preliminary study on the Chinese continental mineralization system Wang Denghong Institute of Mineral Resources, CAGS, Beijing, 100037, China Chen Yuchuan Chinese Academy of Geological Sciences (CAGS), Beijing, 100037, China Abstract. China is enriched in mineral resources. How to systematically deduce the regularity of mineralization in order to serve for prospecting is the main purpose of this paper. The Chinese continental mineralization system (CCMS) can be referred to as the whole group of mineral deposits located in the present continent of China and their genetically related geological factors. The CCMS consists of 214 minerogenic series of 11 geological periods from Early Archean to Cenozoic, including at least 978 patterns of representative mineral deposits.The CCMS is the final result of mineralization formed through the whole evolution history of Chinese continental crust. Keywords. Chinese continental mineralization system, minerogenic series, metallogenic prognosis, evolution regularity 1 Introduction After a long history of mining (at least 3000 years), especially large-scale geological exploration conducted since the founding of the People’s Republic of China (1949), 171 kinds of mineral resources have been discovered up to present. Among these, 156 commodities have explored reserves, including 9 types of energy resource, 54 metallic minerals, 90 industrial minerals, plus groundwater, mineral water, and carbon dioxide gas. The total value of potential reserves places China third in the world. Various deposits are among the richest in the world, including rare earths, W, Sn, Sb, Mo, Bi, Be, coal, magnesite, barite, fluorite, talc, graphite, bentonite, fireclay, asbestos, gypsum, wollastonite, diatomaceous earth, and building stone. On the other hand, the country is lacking oil, high-grade iron, Cr, Mn, Cu, PGE, potash salt, and diamond. By now, about 200,000 localities of ore deposits or mineral occurrences have been discovered. Among these, 20,000 ore deposits have been investigated in detail, including 90 super giant deposits (Fig. 1; Chen 1999). However, little geological work has been done in the vast western territory of China and for depths greater than 500 m, suggesting a great potential for further discoveries. Owing to the diversity of geological settings for mineralization in China, there is great potential for ore prospecting (Guo, 1987; Chen 1999). 2 Concept of Chinese continental mineralization system and related terms In this paper, we refer the Chinese continental mineralization system (CCMS) as the whole group of mineral deposits located in the present continental crust of China and their genetically related geological factors. All mineral deposits located in the present continental crust of China formed during the history of continent evolution. The concept of CCMS contrasts with the term Chinese oceanic mineralization system (COMS), both the CCMS and the COMS compose the Chinese Mineralization System (CMS), while the CMS is part of the global mineralization system (GMS). The global mineralization system can be divided into a series of sub-systems geographically. The GMS can be divided into sub-systems according to different classification systems, such as spatial subsystems, temporal sub-systems (Mesozoic mineralization system, Cenozoic mineralization system and so on), and genetically sub-systems (magmatic mineralization system, sedimentary mineralization system and metamorphic mineralization system). Thus, the CCMS is in fact a complex big system composed of different levels of sub-systems, which related to each other structurally, regularly, inevitably and recognizably. By the study of CCMS, the wholly, knowledge about mineralization can be concluded systematically and sequentially, instead of individually, fragmentally or randomly. In this paper, we will pay more attention to the CCMS, because it’s forming history shows an important aspect of the continental evolution history of China and provides valuable clues and indispensable examples for the understanding of global mineralization system. The relationships among different deposits and the relationships between mineralization and its geological history and tectonic setting are very important for the study of CCMS. The present Chinese continental crust includes relative stable regions (paleo-plates or massif) and active belts (suture zones and/or collision belts). There are three large landmass or plates and four active belts in China (Fig. 2). The three main landmass include: (1) the North China landmass, which were formed after the Lvliang Movement (1800 Ma) and includes a basement of Archean and/or Lower Proterozoic metamorphic rocks; (2) the Tarlimu landmass, formed after the Jinning Movement (1000 Ma) and has a basement of pre-Sinian metamorphic rocks; (3) the Yangtze landmass, also formed after the Jinning Movement and its basement consists mainly of Proterozoic metamorphic rocks. Close 854 Wang Denghong · Chen Yuchuan The main active belts include: (1) the Tianshan- Xing’an active belt, which consist with a series of fold belts and micro-plates and formed after the Caledonian- Hercynian movement; (2) the Kunlun-Qilianshan- Qinling active belt, located between North China and South China and activated at different epochs of Jinning, Caledonian, Hercynian, Indo-Chinese, Yanshanian and Himalayan; (3) the Sichuan-Yunnan-Qinghai-Tibet active belt, which is the most important active belt of Tethys- Himalayan in the southwestern China; and (4) the western circum-Pacific active belt, mainly overprinted on the Paleozoic and pre-Paleozoic tectonic belts in the eastern China and featured by strong activation of Mesozoic-Cenozoic volcanism-magmatism in East China, large-scale granitoid intrusion in the Nanling Region (Chen et al. 1989), NE-NNEtrending movement of blocks and rifting-magmatism in the margin area of paleo-landmass. 3 Manifestation of the CCMS Generally speaking, the CCMS is a natural system consisting of more than 200 thousand localities of ore deposits or mineral occurrences. Obviously, it is difficult to reveal the nature and complexity of CCMS by single deposits, deposit types, mineralized belts, host rocks, or other factors related to mineralization. In this paper, we apply the terminology of minerogenic series to describe the CCMS in brief. The concept of CCMS is different from that of minerogenic series presented by Cheng et al. (1979, 1983), which groups a series of mineral deposits related to each other genetically within a certain setting of geological environment and within a certain stage of geological history (Wang et al. 2002). However, because each minerogenic series bases on the four most important factors (ore-forming age, tectonic setting, geologic event and mineral assemblage and/or metal association), it is suitable to apply the nomenclature of minerogenic series to construct the framework of CCMS. Generally speaking, we have divided the CCMS into different sub-systems according to geological time, and each sub-system consist of secondly sub-system of mineralization based on geological setting of the same geological time. Given a certain geological setting of a certain geological time, each minerogenic series refers to a certain group of metals and/or mineral resources and/or energy resources related to a certain geologic process. Thus, minerogenic series is the preferred and integrant unit to make up of the CCMS. As a whole, the CCMS consists of 214 minerogenic series of 11 geological periods from Early Archean to Cenozoic, including at least 978 patterns of representative mineral deposits. Close Chapter 7-34 · Preliminary study on the Chinese continental mineralization system 4 Application significance of the CCMS Because the CCMS can be build up by basic unit of minerogenic series, minerogenic series and their relationship with the evolution history of China continental crust then become the most important aspect of our present research. As to each minerogenic series, all the mineral deposits are grouped together genetically rather than randomly. For example, the Triassic sedimento-minerogenic series of salt and coal deposits associated with marine carbonaceous rocks and paralic clastic rocks within the Sichuan basin, which is one of the above 214 minerogenic series of the CCMS, consists of a series mineral deposits including the gypsum deposits (named as Nongle-type) and the celestite deposits (named as Chongqing-type) hosted within the Jialingjiang Formation (T12j), including the polyhalite deposits (named as Quxian-type) within the Jialingjiang Formation and the Leikoupo Formation (T21l), including the halite deposits (named as Weixi-type) within the Leikoupo Formation, and including the coal deposits (named as Yongrong-type) within the Xujiahe Formation (T32-3x). The evolution trend of mineral deposits from salt to coal gradually is in accordance with the evolution history of the Sichuan basin changing from oceanic to terrestrial facies at its waning stage. Such trend 855 of mineralization evolution can thus be deduced as a piece of regularity for prospecting in the Sichuan basin and in other similar basins further. In a broad sense, in a geosyncline’s environment such as the Northern marginal belt of the North China Platform of Proterozoic, the Kunlun- Qilianshan-Qinling belt of Proterozoic-Paleozoic, the Altay tectonic belt of Paleozoic ,and the Tethys belt of Mesozoic, mineral deposits usually change from base metal deposits of VHMS-type formed at its early stage to rare metal deposits associated with magmatism at its folding or mountain building stage, and to gold deposits controlled by regional structures at its late stage of structural adjustment within an actually continental setting. Such trend is partly similar to that of an Wilson cycle, but each minerogenic series is different from each other because of its unique geological time of ore-forming, tectonic environment, special association of mineral resources and genetic relationship with other geologic process. Thus, the study of CCMS also can provide a new approach for deduction the evolution history of the Chinese continent crust. In addition, the study of CCMS can contribute to metallogenic prognosis. For instance, the number of minerogenic series become more and more from Archean to Proterozoic to Paleozoic to Mesozoic and to Cenozoic. Close 856 Wang Denghong · Chen Yuchuan However, the number of Yanshanian minerogenic series shows a negative anomaly calculated on the same scale of geological time, suggesting that there is still a good potential for prospecting Yanshanian minerogenic series in China. Recently, numerous new deposits of Mesozoic age have been discovered both in northwestern China (such as the Baishan Mo deposit in Xinjiang, dated at 229±3Ma by a Re-Os isochron on molybdenite) and in south-eastern China (such as the Taoxikeng wolframite deposit in south Jiangxi, the Baolun gold deposit in Hainan). Some important deposits discovered earlier have also been proved to be of Mesozoic age by systematic dating. For example, the famous rare metal deposit hosted within the No.3 pegmatite-vein in Keketuohai mine, North Xinjiang, yields 40Ar/39Ar isochron ages ranging from 177.9 Ma to 148 Ma (Wang et al. 2002). This deposit has been recognized as a Hercynian deposit for nearly a century. 5 Evolution of the CCMS In general, the concept of CCMS can also be summarized as the systematic combination of all the minerogenic series that formed during the whole evolution history of the present continental crust in China. So, the CCMS can be divided into Archean, Proterozoic, Paleozoic, Mesozoic, and Cenozoic sub-systems of mineralization as follows: 1. Archean sub-systems occurred in nucleus of the Chinese continental crust, dominated by BIF-type deposits, VHMS-type Fe, Cu, Pb, and Zn deposits, gold, graphite, and sillimanite deposits associated with metamorphic rocks; 2. Proterozoic sub-systems occurred in the marginal rift setting peripheral to the Archean Chinese continental shield, also dominated by Fe, Cu, Ni, REE, Pb, Zn deposits related to magmatism and sedimentary process and Au, B, P, magnesite, graphite, andalusite, and sillimanite deposits related to metamorphic process, and featured by massive Cu-Ni deposits related to maficultramafic rocks; 3. Paleozoic sub-systems occurred in the main orogenic belts around the Proterozoic Chinese continent, featured by more complex association of elements and/ or mineral resources than that of Proterozoic and by typical plate tectonic environment; 4. Mesozoic-Cenozoic sub-systems occurred both around and within the Paleozoic Chinese continent (Chen and Wang 2001), featured by porphyry-type copper deposits, skarn-type Fe-Cu deposits, granite-related W, Sn, Bi, Mo, REE, Rare metal, Pb, Zn, Sb, Ag, Au, Hg deposits, placer deposits, industrial mineral deposits formed within weathering crust, energy resources formed within continental basins and so on, with banded iron formation and mafic-ultramafic massive Cu-Ni deposits disappearing (Wang et al. 2000). Close Chapter 7-35 7-35 Origin and evolution of Sn- and Cu-rich fluids in the Dajing tin-polymetal deposit - evidence from LA-ICP-MS analysis of individual fluid inclusions Wang Lijuan, Wang Yuwang, Wang Jingbin Beijing Institute of Geology for Mineral Resources, Beijing 100012, and Key Laboratory of Mineral Resources Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, 100029, China Zhu Heping Key Laboratory of Mineral Resources Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, 100029, China Günther Detlef ETH, Swiss Federal Institute of Technology, 8092 Zürich, Switzerland Abstract. LA-ICP-MS analysis of the composition of individual fluid inclusions indicate that shallow-originated Sn-rich fluids and deeporiginated Cu-rich fluids mix at moderate to low temperature and low salinity, eventually resulting in the formation of Cu and Sn mineralization in the Dajing deposit. Keywords. Dajing, single inclusion, LA-ICP-MS anslysis, Cu-rich fluids, Sn-rich fluids The Dajing tin-polymetal deposit is located at the northern margin of North China Craton (Zhao and Zang 1997; Wang et al. 2001). Quartz and fluorite are intergrown with cassiterite and chalcopyrite. Chalcopyrite can be found included in fluorite. Abundant fluid inclusions were found in fluorite. They are large with a gas/liquid ratio of 10%. Chalcopyrite crystals can be found in some fluid inclusions. It is deduced that these fluid inclusions with chalcopyrite crystals are trapped from Cu-rich fluids. Cassiterite can be found included in quartz. Fluid inclusions in quartz are small in size and some are gas inclusions with high gas/liquid ratios. Microthermometric data show that the chalcopyrite-bearing fluid inclusions in chlorite have low to moderate temperature and low to moderate salinity whereas gas inclusions in quartz have moderate to high temperature and low salinity. Therefore, it is inferred that Cu-rich fluids are low to moderate temperature and low to moderate salinity whereas the Sn-rich fluids are moderate to high temperature and low salinity. The intergrowth of Sn and Cu probably resulted from mixing of Cu-rich fluids and Sn-rich fluids (Wang et al. 2000). To further ascertain the origin and evolution of the Sn-rich and Cu-rich fluids in the Dajing deposit, LA-ICPMS analyses on individual fluid inclusions with different temperature, salinity, and occurrence in quartz and fluorite from the Sn-Cu orebodies were carried out at Swiss Federal Institue of Technology, Switzerland in February, 2004. LA-ICP-MS is the most advanced analysis method for the composition of single fluid inclusions. Most of the reseach focused on fluids of high temperature and high salinity (Audeat et al. 1998; Günther et al. 1998; Günther and Heinrich 1999). Because some fluid inclusions in fluorite contain chalcopyrite crystals, we made LA-ICP-MS analysis of individual fluid inclusions on them and take their compositions as representative of the Curich fluids. Near the Dajing deposit, there is a tin deposit named Huanggangliang, which belongs to the same tinmineralization belt as the Dajing deposit. Both deposits have quite similar geological background (Li et al. 2001; Wang et al. 2001). We analyzed the fluid inclusions in quartz associated with cassiterite from the Dajing deposit and primary fluid inclusions in fluorite from the Huanggangliang deposit with LA-ICP-MS analysis. The Close 858 Wang Lijuan · Wang Yuwang · Wang Jingbin · Zhu Heping · Günther Detlef results are quite similar. Therefore, the LA-ICP-MS analytic results of individual fluid inclusions in quartz associated with cassiterite from the Dajing deposit were taken as representative of the Sn-rich fluids. Tables 1 and 2 are the LA-ICP-MS analytic results of individual Cu-rich and Sn-rich fluid inclusions, respectively. Table 1 shows that the Cu-rich fluids have higher Cu contents than Sn, have Sr contents one to several order of magnitude higher than Rb, and are relatively richer in Na than K. Table 2 shows that the Sn-rich fluids have higher Sn contents than Cu, have Rb contents one to several oder of mragnitude higher than Sr, and are relatively richer in K than Na. Based on the compositions of representative Cu-rich and Sn-rich fluids, we infer whether other fluid inclusions with different occurrence, temperature and salinity in quartz and fluorite belong to Cu-rich or Snrich fluids, and thereby trace the origin and evolution of these fluids. Cu-rich and Sn-rich fluid inclusions are listed in Tables 3 and 4, respectively. Figure 2 shows that both the Cu-rich and the Sn-rich fluids have a similar evolutionary trend from high to low temperature and the two kinds of fluids probably mix at moderate temperature, resulting in mineralization. The Sr and Rb concentrations in the fluids are important indicators for the fluid source. According to Zhao et Close Chapter 7-35 · Origin and evolution of Sn- and Cu-rich fluids in the Dajing tin-polymetal deposit - evidence from LA-ICP-MS analysis of individual fluid inclusions 859 shallow-originated Sn-rich fluids and the deep-originated Cu-rich fluids mix at the stage of moderate to low temperature and low salinity and result in the formation of Cu and Sn mineralization in the Dajing deposit. 4. To our knowledge, there have been no reports about LA-ICP-MS analysis on individual fluid inclusions with such low temperature, low salinity and small size as in the Dajing deposit. The results demonstrated that the LA-ICP-MS analysis of individual fluid inclusions has practical applications in studying ore-forming processes in polymetal ore deposits. References al (1997), Sr is enriched in the early stage of magma differentiation, whereas Rb is enriched in the late stage of magma differentiation. Therefore, the ratio of Rb/Sr increases with magma differentiation, from an average of about 0.5 at the early stage to above 10 at the late stage. The Cu-rich fluid in the Dajing deposit are highly enriched in Sr, indicating that the fluids are derived from the deep, whereas the Sn-rich fluids are enriched in Rb, reflecting their derivation from the shallow. Based on the analyses, several conclusions can be reached: 1. The Cu-rich fluids have higher Cu contents than Sn, higher Sr contents than Rb, and are relatively rich in Na. The fluids are derived from a deep source and are mainly trapped in fluorite. 2. The Sn-rich fluids have higher Sn contents than Cu, higher Rb contents than Sr, and are relatively rich in K. The fluids are shallowly derived and mainly trapped in quartz. 3. Both the Cu-rich and Sn-rich fluids have an evolutionary trend from high temperature to low temperature. The Audetat A, Günther D, Heinrich CA (1998) Formation of a magmatichydrothermal ore deposit: Insights with LA-ICP-MS analysis of fluid inclusions. Science 279: 2091-2094 Günther D, Heinrich CA (1999) Enhanced sensitivity in laser ablation-ICP mass spectrometry using helium-argon mixtures as aerosol carrier. J Anal Atom Spectrom 14: 1363-1368 Günther, D Audetat A, Frischknecht R, Heinrich CA (1998) Quantitative analysis of major, minor and trace elements in fluid inclusions using laser ablation-inductively couple plasma mass spectrometry. J Anal Atom Spectrom 13: 263-270 Li JW, Shimazaki H, Yoshihide S (2001) Skarns and genesis of the Huanggang Fe-Sn deposit, Inner Mongolia, China Resource Geol 51: 359-376 Wang L, Wang J, Wang Y, Shimazaki H (2001) Ore-forming fluid and metallization of the Huanggangliang skarn Fe-Sn deposit, Inner Mongolia. Sci China (Series D) 44: 735-747 Wang L, Wang Y, Wang J, Jin X, Zhu H (2000) Metallogenetic fluid study of tin and copper stage from Dajing deposit and its genetic significance. Acta Petrol Sinica 16: 609-615 (in Chinese with English abstract) Wang YW, Wang JB, Uemoto T, Wang LJ (2001) Geology and mineralization at Dajing tin-polymetallic ore deposit, Inner Mongolia, China. Resource Geol 51: 307-320 Zhao Y, Zhang D (1997) Metallogeny and prospective evaluation of copper-polymetallic deposits in the Da Hinggan Mountains and its adjecent regions Seismo Press, Beijing: 125-144 Zhao Z (1997) The principle of trace elements geochemistry. Science Press 1-153 (in Chinese) Close Close Chapter 7-36 7-36 Lead and zinc-rich fluid inclusions in Broken Hill-type deposits: Fractionates from sulphide-rich melts or consequences of exotic fluid infiltration? Patrick J. Williams, Dong Guoyi School of Earth Sciences and 1Predictive Mineral Discovery CRC, James Cook University, Townsville 4811, Australia Bruce Yardley School of Earth Sciences, University of Leeds, Leeds LS2 9JT, UK Thomas Ullrich Geology Department, The Australian National University, 0200 Canberra, Australia Chris Ryan CSIRO Exploration and Mining, School of Geosciences, Monash University, Melbourne 3168, Australia Terry Mernagh Geoscience Australia, GPO Box 378, Canberra 2601, Australia Abstract. High salinity fluid inclusions (Th = 200-550° C) from the Broken Hill and Cannington “Broken Hill-type” ore deposits in Australia have been analysed by PIXE and LA-ICP-MS. They have high Pb (>1%) and Zn (>1000 ppm) and Pb/Zn ratios much higher than those of the majority of crustal brines. Laser Raman studies reveal the presence of methane and PIXE images show that Pb and Zn are respectively concentrated in a Pb-K-Cl solid, and the liquid phase. This indicates that the inclusions have very low total sulphur contents. The Pb/Zn ratios are similar to those of eutectic melts in the Gn-Sp-Po system whereas Pb/Fe ratios are variable and lower than those of such melts. If these brines originated by fractionation from synmetamorphic sulphide-rich melts, then they must been greatly modified prior to entrapment. An alternative origin involving lateto post-metamorphic interaction of externally-derived brines with pre-existing sulphide accumulations should also be considered. In either case, the unique brine chemistry would appear to relate to the large amounts of sulphides in these systems. New South Wales (2 pyroxene granulite) and Cannington in NW Queensland (upper amphibolite). Along with just a few other ore deposits worldwide these are referred to as “Broken Hill-type” (BHt) deposits which are defined more by their high grade metamorphic settings than any consensus on their origin (e.g. Walters, 1998). It has recently emerged that very Pb- and Zn-rich aqueous fluid inclusions occur in both large Australian BHt deposits (Williams et al. 1999). In this paper we show that the chemistry of these brines is unlike any others previously known and discuss the possible processes by which they may have formed. Keywords. Lead, zinc, fluid inclusions, Broken Hill-type deposits, PIXE, LA-ICP-MS 1 Introduction Yardley et al. (2003) used compiled natural brine and fluid inclusion analyses to show that concentrations of many metals vary systematically with temperature and salinity. This was taken to indicate that rock buffering is a powerful control on other major chemical influences of solubility, such as pH, fO2 and sulphur abundance. Concentrations of elements such as Mn, Fe, Cu, Zn and Pb in natural fluids can be predicted within about an order of magnitude for known temperature and salinity and this can be viewed as a limiting chemical framework for hydrothermal ore-forming processes Large and very distinctive Pb-Zn-Ag ore deposits occur in partially melted metamorphic rocks at Broken Hill, Close 862 Patrick J. Williams · Dong Guoyi · Bruce Yardley · Thomas Ullrich · Chris Ryan · Terry Mernagh 2 Petrography and microthermometry A large variety of fluid inclusions have previously been observed in the Broken Hill ore deposit but this have received little attention in the literature (Wilkins 1977; Spry 1978). The current study used rocks displaying evidence of hydrothermal modification during the retrograde metamorphic history of the deposits. Sample 147001 from Broken Hill is a partly recrystallized quartz-rich rock from Western A lode in which older “blue quartz” is overprinted by late stage “white quartz” as described by Wilkins (1977). Fluid inclusions, predominantly less than 15 microns in diameter are very abundant as secondary trails in the older quartz and belong to the same fracture association that formed the white quartz. Sample 42170 from Cannington is an example of a quartz vein associated with a form of Fe- and Cl-rich hornblende alteration which is very common in the deposit (Chapman and Williams 1998). Fluid inclusions are again abundant in secondary trails (Fig. 1) and in this case can be very large (up to circa 100 microns). In both samples, the vast majority of inclusions at room temperature are composed of liquid, a small vapour bubble, and number of solids. The latter have been investigated by microprobe in opened inclusions, in PIXE images and (42170 only) by laser Raman probe and were consistently found to include halite, pyrosmalite, and a Pb-K chloride.Some inclusions additionally contain sylvite and/or a Mn-rich carbonate mineral. Vapour bubbles were investigated by laser Raman probe in 42170 only and were found to consist of methane. The inclusions in 147001 homogenise by vapour bubble disappearance at temperatures between 270 and 410° C and have NaCl equivalent salinities between 30 and 40 wt %. Those in 42170homogenise by pyrosmalite dissolution at 400-450° C and have NaCl equivalent salinities between 30 and 40 wt %. In both samples the Pb-K-Cl phase dissolves at temperatures 100-200° below those of total homogenisation. 3 lyzed by LA-ICP-MS owing to a lack of suitable external standards, and (c) able to image the distribution of elements between the phases present in the inclusions at room temperature. Coupled with microthermometric and laser Raman gas phase data, the images throw light on the likely abundance and speciation of the critical element sulphur which can not be determined at normal geological abundance by either microanalytical technique. PIXE analyses give a quantitative estimate of element abundances to an accuracy of ± circa 50 % though interelement ratios are determined to a much better level of accuracy as the main sources of error have similar effects on all elements. LA-ICP-MS data are determined as ratios and estimation of absolute concentrations depends on an independent internal standard such as the estimated abundance of a component by PIXE or microthermometric salinity estimates (Heinrich et al. 2003). PIXE analysis can only be undertaken of shallow inclusions (typically < 20 microns). Attempts to achieve controlled laserablation of shallow inclusions were generally unsuccessful and the analyses obtained by the two techniques were undertaken on different groups of inclusions. Pb and Zn data from the three different laboratories are very consistent (Fig. 2). The average concentrations estimated by PIXE are 3150 ppm Zn, 36500 ppm Pb in 147001 and 4950 ppm Zn, 30300 ppm Pb in 42170 (ex- Fluid inclusion geochemistry In situ microanalysis of fluid inclusions is a new and rapidly developing field and to date there has been a general lack of studies comparing results obtained using different techniques and in different laboratories. High salinity brine inclusions from Cannington and Broken Hill were investigated using both proton induced X-ray excitation (PIXE) analysis (method of Ryan et al. 2001), and laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) using Excimer laser ablation systems (cf. Heinrich et al. 2003) at the Australian National University and Leeds University. The PIXE method is (a) relatively insensitive to contamination from the host quartz and any solid inclusions it contains, (b) able to provide quantitative data for halogens (Cl, Br) that were not ana- Close Chapter 7-36 · Lead and zinc-rich fluid inclusions in Broken Hill-type deposits: Fractionates from sulphide-rich melts or consequences of exotic fluid infiltration? cluding one outlying analysis with lower concentrations - cf. Fig. 2). The PIXE images reveal that Zn is codistributed with Ca and Br in the liquid phase of the inclusions at room temperatures. Zn/Pb ratios determined by both techniques are all less than 1 and on average around an order of magnitude below those of high temperature and high salinity brines in the data set compiled by Yardley et al. (2003). This reflects much higher concentrations of Pb in the Broken Hill and Cannington inclusions than have been measured in other natural high salinity fluids excepting a single case where extreme Pb enrichment was deduced to occurred in a fluid involved in retrograde hydration of granulites (Svenson et al. 1999). Pb/Ag ratios measured by LA-ICP-MS are between 640 and 1470 in sample 147001 and between 200 and 800 in sample 42170. Br/Cl ratios determined by PIXE in sample 42170 are in the range 0.0003 to 0.0016 which is distinctly lower than seawater and magmatic brines as measured from porphyry copper deposits (cf. Kendrick et al. 2003). The PIXE investigation of sample 147001 was undertaken under conditions of comparatively poor instrumental performance and meaningful data were not obtained for Br in this case. 4 Discussion The studied fluid inclusions from Broken Hill and Cannington have much higher Pb concentrations and Pb/ Zn ratios than fluid inclusions with similar salinities from other geological settings suggesting that they result from some process which is specific to this sort of ore deposit. Mavrogenes et al. (2001) have shown that compositions in the FeS-ZnS-PbS-Ag2S system would have been partially-molten under peak metamorphic conditions at Broken Hill (though it is not clear that this would also have been the case at Cannington). One possible explanation for the unusual fluid inclusions is that they represent aqueous phases that equilibrated with sulphide melts. If this is the case then element abundances in the inclusions should reflect their activity ratios in the melt. The FeSZnS-PbS eutectic as determined by Mavrogenes et al. (2001) has Pb:Fe:Zn (by weight) approximating to 12:2.5:1 (Fig. 3) and all melts below 900° C have low ZnS compared to the other two components. High Pb/Zn ratios are therefore to be expected in fluids equilbrated with FeS-ZnS-PbS melts and the average ratios measured in the fluid inclusions from samples 147001 and 42170 are very similar to the ratio of the eutectic composition Furthermore, Mungall and Brenan (2003) established that Cl has an affinity for Fe-Cu-Ni-S melts (due to similarities with sulphur) and predicted that aqueous fluids evolved from such melts should have low Br/Cl ratios (cf. the fluid inclusions in 42170). This would be also expected to be a feature of other sulphide melt systems. However, it is not a diagnostic feature as low ratios could also reflect salin- 863 ity derived from evaporitic halite or its preserved signature in metamorphic rocks. Other features of the fluid inclusions are less easily reconciled with a relationship to sulphide melts. Thermometric results and paragenetic associations with retrograde hydrous and Cl-bearing silicates suggest the inclusions were trapped at temperatures several 100°s below those of the metamorphic peaks in the two systems. At Cannington, metamorphic hornblendes did not pass through their 40Ar-39Ar blocking temperatures until some 40 million years after the partial melting event recorded in the gneissic host rocks (Pollard et al. 1997; Giles and Nutman 2002). Aqueous fluids present at peak conditions would have somehow had to have avoided extraction by silicate melts and remained trapped in the system throughout this period to have been preserved in fluid inclusions. Fluids from both locations were evidently strongly undersaturated in Pb and Zn when trapped and must have very low reduced sulphur contents given the phase distribution of metals at room temperature. Large chemical variations are present including those of Pb/Fe (all lower than eutectic melt; Fig. 3) and Pb/Ag (different in the two samples) suggesting that the fluids were involved in chemical reactions at the time the inclusions were trapped. An alternative origin involving late- to postmetamorphic interaction of externallyderived brines with pre-existing sulphide accumulations should also be considered. In this case the high Pb/Zn ratio might reflect the higher solubility of galena compared to sphalerite in high temperature brines (Hemley et al. 1992). In either case the unique chemistry would appear to relate to the large concentrations of sulphides in these systems. Close 864 Patrick J. Williams · Dong Guoyi · Bruce Yardley · Thomas Ullrich · Chris Ryan · Terry Mernagh Acknowledgements This work was supported by AMIRA, the ARC and the Predictive Mineral Discovery CRC. 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Austr J Earth Sci 49: 455-465 Heinrich CA, Pettke T, Halter WE, Aigner-Torres M, Audétat A, Günther D, Hattendorf B, Bleiner D, Guillong M, Horn I (2003) Quantitative multi-element analysis of minerals, fluid and melt inclusions by laser-ablation inductively-coupled plasma massspectrometry: Geochim Cosmochim Acta 67: 3473-3496 Hemley JJ, Cygan GL, Fein JB, Robinson GR, D’Angelo WM (1992) Hydrothermal ore-forming processes in the light of studies in rock-buffered systems: I, iron-copper-zinc-lead sulfide solubility relations: Econ Geol 87: 1-22 Kendrick MA, Burgess R, Pattrick RAD, Turner G (2001) Fluid inclusion noble gas and halogen evidence on the origin of Cuporphyry mineralising fluids: Geochim Cosmochim Acta 65: 2651-2668 Mavrogenes JA, Macintosh JW, Ellis DJ (2001) Partial melting of the Broken Hill galena-sphalerite ore. Experimental studies in the system PbS-FeS-ZnS-(Ag2S). Econ Geol 96: 205-210 Mungall JE, Brenan JM, (2003) Experimental evidence for the chalcophile behavior of halogens. Can Mineral 41: 207-220 Pollard PJ, Perkins C (1997) 40Ar/39Ar geochronology of alteration and Cu-Au-Co mineralization in the Cloncurry district, Mount Isa Inlier. AMIRA P438 Cloncurry Base Metals and Gold Final Report, Section 3, 40pp Ryan CG, McInnes, BM, Williams PJ, Guoyi Dong, Tin Tin Win, Yeats CJ (2001) Imaging fluid inclusion content using the new CSIROGEMOC nuclear microprobe. Instr Meth Physics Res B 181: 570-577 Spry PG (1978) The geochemistry of garnet-rich lithologies associated with the Broken Hill orebody, N.S.W., Australia. Unpubl MSc thesis, University of Adelaide, 129pp Svenson H, Jamtveit B, Yardley B, Engvik AK, Austrheim H, Broman C (1999) Lead and bromine enrichment in eclogite-facies fluids: extreme fractionation during lower-crustal hydration. Geology 27: 467-470 Walters SG (1998) Broken Hill-type deposits. AGSO J Austr Geol Geophys 17: 229-237 Wilkins RWT (1977) Fluid inclusion assemblages of the stratiform Broken Hill ore deposit, New South Wales, Australia. Science 198: 185-187 Williams PJ, Dong Guoyi, Prendergast K, Pollard PJ, Ryan CG (1999) Metasomatism and metal mobility in Broken Hill-type deposits. In: Stanley CJ et al. (eds) Mineral Deposits: Processes to Processing. Balkema, Rotterdam, pp 999-1002 Yardley B, Bennett A, Banks D (2003) Controls on the chemical composition of crustal brines. J Geochem Expl 78/79: 133-135 Close Chapter 7-37 7-37 Isotopic composition and source of lead in the Jinding Zn-Pb Deposit, Yunnan, China Zeng Rong, Zhao Shihua, Gao Yongbao, Li Yongqiang Faculty of Earth Sciences and Territory Resources, Chang’an University, Xi’an, Shaanxi 710054, China Abstract. The Jinding Zn-Pb deposit is the largest Zn-Pb deposit so far discovered in China. To study the source of the mineralizing materials, we analyzed its lead isotopes. We found that the isotopic composition of lead in coarse-grained and fine-grained galenite crystals are very different. The ratio of lead isotopes in fine-grained galenite is higher, and lead isotopes are distributed over the lead development curve of the orogenic belt which is located in the range of upper crustal lead. All these indicate that the lead of fine-grained galenite comes mainly from stratigraphy. In contrast, the ratio of lead isotopes in coarse-grained galenite is lower and lead isotopes are distributed beneath the lead development curve of the orogenic belt, as well as in the upper mantle and lower crust. Keywords. Lead isotope, composition, source, Jinding Pb-Zn deposit, Yunnan, China 1 Previous research The Jinding Zn-Pb deposit is one of the seventeen giant Zn-Pb deposits in the world, with more than 10 million tons of Zn+Pb reserves. It is also the largest Zn-Pb deposit so far discovered in China. The Jinding Zn-Pb deposit is sediment-hosted, however its genetic origin differs from other sediment-hosted Zn-Pb deposits such as Mississippi Valley-type (MVT) deposits, Sedimentary exhalative (Sedex) deposits and Sandstone-type (SST) deposits. The Jinding Zn-Pb deposit may represent a new type of sediment-hosted deposit. Geologists have been studying the Jinding Zn-Pb deposit intensively since the 1980s, and during the twenty years of study there have been many different opinions about the genesis of the lead ores. Some think the lead in the ores comes mainly from the deep mantle, with minor input from the crust (Zhao 1989). Some argue that the lead in the ores is derived from the mantle, but has been hybridized by lead from the crust (Zhou and Zhou 1992). And others consider that the lead in the ores is derived from the lower crust and is related to the interaction between lead in the lower crust and in the sedimentary rocks (Zhang and Shao 2002). 2 Geologic characteristics of the ore zone The Jinding Zn-Pb deposit occurs in a Cenozoic dome structure whose center is eroded. There are six ore blocks (Beichang, Paomaping, Jiayashan, Xiponanchang, Baicaoping and Fengzishan) surrounding the dome. The slaty, veined, phacoidal and stratoid orebodies are dis- tributed around the center of dome and tilt in towards the deep dome. At the top of the dome the orebody is thicker. Two stratigraphic systems are present in the Jinding area, referred to as the autochthonous system and the allochthonous system. The former refers to strata of the Cretaceous Hutousi Formation (K2h) and the Paleocene Yunlong Formation (E1ya-E1yb). The allochthonous system includes the Lower Cretaceous Jingxing Formation (K1j), Mid-Jurassic Huakaizuo Formation (J2h), the Upper Triassic Maichuqing Formation (T3m) and the Sanhedong Formation (T3s). The Zn-Pb ores are hosted in the sandstones of the Lower Cretaceous Jingxing Formation (K1j) and the Upper Yunlong Formation (E1yb), which are separated by a thrust-nappe structure (F2). There are two distinct types of ores at the Jinding deposit, breccia-type ores and sandstone-type ores. The textures associated with the breccia-type ores include metasomatic and solutional texture, concentric zonal texture, massive structure, brecciated structure and reticular vein structure. These ores are hosted in the Upper Yunlong Formation (E1yb), east of ore district. The sandstone-type ores consist mainly of cementation texture and disseminated structure and are hosted in the middle and west of the ore district. 3 Isotopic composition and source of lead To study the source of the mineralizing materials of the Jinding Zn-Pb deposit, we choose the homogeneous galenite samples to do comparative study on lead isotopes (Table 1). We find that the composition of lead isotopes from coarse-grained and fine-grained galenite is different (Fig. 1): Fine-grained galenite 206Pb/204Pb 18.15~18.60, 207 Pb/ 204Pb 15.612~ 15.64, 208Pb/ 204Pb 38.287~ 38.66; Coarse- grained galenite 206Pb/204Pb 18.03~19.21, 207Pb/ 204Pb 15.252~15.55, 208Pb/204Pb 37.800~38.930. The ratio of lead isotopes in fine-grained galenite is higher, and lead isotopes are distributed over the lead development curve of the orogenic belt which is located in the range of upper crustal lead. All these indicate that the lead of finegrained galenite comes mainly from stratigraphy. In contrast, the ratio of lead isotopes in coarse-grained galenite is lower and lead isotopes are distributed beneath the lead development curve of the orogenic belt, as well as in the upper mantle and lower crust. The composition of lead isotopes in three plagioclases crystals and garnets Close 866 Zeng Rong · Zhao Shihua · Gao Yongbao · Li Yongqiang Close Chapter 7-37 · Isotopic composition and source of lead in the Jinding Zn-Pb Deposit, Yunnan, China 867 derived fluids rich in CO2 (jingdin and Chaoyang 1991). The isotopes of He, Ne, Xe also indicate that there are mantle components in the Jinding Zn-Pb deposit (Xue and Chen 2003). These data are consistent with the lead isotope data from coarse-grained galenite distributed in the upper mantle. According to the data, we may conclude that there are at least two metallogenic epochs in the Jinding Zn-Pb deposit: (1) The epoch of fine-grained galenite; (2) The epoch of coarse-grained galenite. The source of the mineralizing materials is different between the two epochs. The mineralizing materials of fine-grained galenite come mainly from stratigraphy, while mineralizing materials of coarse-grained galenite come mainly from the upper mantle and lower crust. The study on the controlling factors of evolution of the Lanping-Simao basin also indicates that the mineralization of the Jinding Zn-Pb deposit involves the interaction between crust and mantle (Yin and Fan 1990). All the data and analyses validate the theory of a multiperiod and multisource origin for the Jinding Zn-Pb deposit. References derived from the enclosures of the lower crust in alkalic rocks of western Yunnan is: 206Pb/204Pb 18.135~18.187, 207Pb/204Pb 15.335~15.388, 208Pb/204Pb 37.836~38.899. These values are identical to the coarse-grained galenite samples whose values are the lowest, so we can conclude that coarse-grained galenite come from the lower crust. The REE geochemical data indicate that the mineralizing materials of the Jinding Zn-Pb deposit are mainly mantle- Wang J, Li C (1991) REE geochemistry of the Jinding superlarge PbZn deposit Geochemica 19: 359~365 Xue C, Chen Y (2003) Geology and isotopic of Helium, Neon, Xeon and Metallogenic age of the Jinding and Baiyangping Ore Deposits Northwest Yunnan, china. Science in China, Ser. D, 46:789~800 Yin H, Fan W (1990) Deep processes and mantle-crust compound mineralization in the evolution of the Lanping-Simao MesozoicCenozoic Diwa Basin in Western Yunnan, China 4: 113~124 Zhang Q, Shao A (2002) Lead isotopic composition and lead soure of polymetallic deposits in the Large Ore Assembly District in the Langping Basin. Acta Mineralogica Sinica 22: 147~153 Zhao X (1989) stable isotope geochemistry of the Jinding lead-zinc ore deposit, Yunnan, Science in the Earth–The Journal of Geology University of China 14: 495~501 Zhou W, Zhou Q (1992) A study on the isotopic composition of Pb and Sinc in the Lanping Pb-Zn Deposit, Yunnan, Geochemica 2: 141~148 Close Close Chapter 7-38 7-38 Geology and geochemistry of the Furong Tin Deposit, Hunan Province, P. R. China Zhao Kuidong, Jiang Shaoyong, Jiang Yaohui State Key Laboratory for Mineral Deposits Research, Department of Earth Sciences, Nanjing University, Nanjing, China Abstract. Recently, a giant tin deposit, the Furong deposit, has been discovered in the Qitianling granitoid, Hunan, South China. The tin mineralization occurs as disseminated crystals or veins of cassiterite. The cassiderite is found in narrow envelopes of chlorite alteration within the granite. The Qitianling granite has distinctly different petrology and mineralogy from common S-type tin granites. The oxygen and hydrogen isotope data indicate a dominant influence of surface-derived meteoric water associated with chlorite alteration. Variations in δ18O of fresh and altered granites are due to continuous isotopic exchange reaction between hydrothermal fluids and granites at variable water/rock ratios. The sulfur isotope compositions of sulfides from the tin ores indicate that both the granite and the strata supported the sulfur for mineralization. The Pb isotopic compositions of sulfides are same as those of feldspars from the granite. Thus, Pb in the ores might come from the granite. Fractional crystallization of the magma and tin deposition directly from exsolved magmatic-hydrothermal fluids may not be the major mechanism for the tin mineralization in this deposit. Instead, we suggest that interactions between fluids of meteoric origin and the granite may contribute to the release and deposition of tin. Keywords. Geochemistry, Furong tin deposit, Qitianling granite, South China 1 Introduction The Furong deposit is a newly discovered giant tin deposit in Hunan Province, P. R. China (Fig. 1). The tin reserve in this deposit has been estimated to be about 600,000 tons (Wei et al. 2002). Tin orebodies mainly occur as veins in the Qitianling granite, which lies in the middle of the Nanling Granite Belt in South China. Previous workers mainly focused on the geology of this deposit (e.g. Wei et al. 2002; Huang et al. 2003; Wang et al. 2003; Mao et al. 2004). The main objectives of the present study are to investigate the source of the ore-forming materials, and to determine the origin and evolution of the hydrothermal fluids and its relationship with the Qitianling granite. We review the geology of the deposit and present the geochemical and isotopic data of the granites and the ores. These data provide important insights into the genetic model of this deposit. 2 Regional geology The Qitianling granite and the Furong tin deposit lie in the middle of the Nanling granitic magma intrusive belt, South China. The belt is an important granitic intrusion and metallic mineralization zone. The Nanling zone has been suggested as one of the domains of the transition from the Paleo-Asian to the Paleo-Pacific tectonic system (Shu and Zhou 2002). The Qitianling granite is ellipse shaped and is one of the largest stocks in the Nanling Granite Belt with a total outcrop area of 520km2. Coutry rocks intruded by the Qitianling granite are Permo-Carboniferous carbonates and Permo- Triassic sandy shales. 3 Geology of the Furong deposit Most of the cassiterite ores occur as veins hosted by altered granites. There are about 40 cassiterite-bearing veins, in which the No. 19 and the No. 10 veins contain 90% of the tin reserve in the deposit. The main granite alterations are chloritization, phyllic and potassic feldspar alteration, in which chloritization is mostly associated with tin mineralization. Cassiterite occurs as disseminated mineralization in the altered granites. There are minor skarntype tin orebodies, which forms at the contact between the granites and the country rocks. Other metallic minerals include scheelite, pyrite, chalcopyrite, sphalerite, arsenopyrite, and rutile. An interesting fact is that cassiterite is generally precipitated together with rutile as disseminations in chlorite. Chlorite has been used as a useful exploration guide for tin mineralization in the granites. 4 Petrology and mineralogy of the Qitianling Granite The Qitianling Granite is complex, with different intrusive phases (Zheng and Jia 2001). Tin mineralization mainly occurs in the Furong phase. Geochemical characteristics of the granite are distinctly different from common S-type tin granites. The Furong phase is composed of potassic feldspar (40%), plagioclase (24%), quartz (27%), biotite (7%) and minor amphibole (2%). Accessory minerals are mainly magnetite, ilmenite, zircon, fluorite, apatite, monazite, sphene. The granite is metaluminous with a ACNK ratio (molar ratio of Al2O3/(CaO+K2O+Na2O)) of 0.88~1.05, which is different from common strongly peraluminous tin granites. The granite is alkaline-enriched and shows low initial 87Sr/86Sr value (0.708), high εNd value (-5.1~-5.8) and young Nd model ages, which suggests contribution of mantle materials in granite genesis. Zircon SHRIMP U-Pb dating gave a crystallization age of 157.1±1.2Ma. Close 870 Zhao Kuidong · Jiang Shaoyong · Jiang Yaohui 5 Geochemical studies of the granite and the deposit 5.1 Mineral chemistry The main rock-forming minerals (amphibole, biotite, plagioclase and ore minerals such as cassiterite and rutile) were analysed for chemical composition by electron microprobe (Zhao et al., 2004). The biotite is Fe-rich annite, and has high Ti, Cl and Sn concentrations. The biotite has high Fe3+/(Fe2++Fe3+) ratios and the oxygen fugacity calculated by biotite compositions is above Ni-NiO (NNO), and near the Fe2O3-Fe3O4 (MH). The amphiboles are ferropargasite and ferro-edenite hornblende. The pressure of the granite, estimated by Al-in-hornblende barometer, is 3.6 ±0.9kbar. Amphibole- plagioclase thermometry and a semiquantitative hornblende thermometer yield a forming temperature of 750~820°C. The chlorite from the orebody has negligible K2O, Ti2O, F, and Cl, but shows similar Fe/(Fe+Mg) ratios with amphibole and biotite. Disseminated cassiterite is closely associated with rutile in chlorite alteration veins and envelopes. The oreforming temperature is estimated to be 290~405°C from chlorite geothermometry. The studied cassiterites are nearly pure SnO2 (>98%). The concentrations of Nb2O5 and Ta2O5 in cassiterite are very low and almost negligible (Nb2O5+Ta2O5<0.1%).These values are distinctly different from cassiterites found in granites or pegmatites, but similar to cassiterite from epithermal or hydrothermal ore deposits. 5.2 REE geochemistry REE contents of both fresh and altered granites are analyzed. Fresh granites show a LREE-enriched and large negative Eu anomaly REE pattern. Altered granites have a similar REE pattern to fresh granites. It suggested that REEs were immobile during hydrothermal alteration of granites in this case. Most sulfides have very low REE contents and show similar REE patterns with granites. Because REEs have distinctly different ionic radii from those of base metal elements, it is difficult for REEs to substitute into crystal lattices of sulfides. Thus, it may be assumed that a major part of REE content of sulfides comes from fluid inclusions in these minerals. REE patterns of sulfides may represent those of ore-forming fluids. Fluorites coexisting with sulfides have relatively high REE contents and show a different REE pattern. Fluorites show a HREE-enriched pattern. Marchand et al. (1976) studied the REE partition between fluorite and a solution of calcium chloride. The REE distribution coefficients strongly favor fluorite, and those for the HREE are greater than those for the LREE. 5.3 H-O isotopes Cassiterites have δ18O values from -4.8‰ to 1‰. Chlorites from the ores have δ18O values from 0.5‰ to 2.5‰, and δD values from -62‰ to -68‰. The estimated oxygen isotope compositions of the hydrothermal fluid from Close Chapter 7-38 · Geology and geochemistry of the Furong Tin Deposit, Hunan Province, P. R. China cassiterites and chlorites vary from -2.0‰ to +3.8‰. The values are lower than those of magmatic-hydrothermal fluids, and are higher than those of Mesozoic meteoric water (-8‰~-9‰) in the studied area. Involvement of surface water of meteoric origin during mineralization of the Qitianliang granite can be ascertained by the oxygen and hydrogen isotope data. Oxygen isotopic compositions of fresh and altered granites have also been measured. The fresh granite far away from tin mineralization has the highest oxygen isotopic composition (+10.5‰). The fresh and slightly altered granites near the tin veins have lower δ18O values from +6.0‰ to +10.0‰. The completely chloritized granites collected from the tin orebodies have the lowest oxygen isotopic composition (5.4‰~6.6‰). The oxygen isotopic variations of the whole rocks are the result of fluidrock interactions. The W/R ratios of completely chloritized granites are estimated to be 0.3~0.5. Pb diagram (Zartman et al. 1981). This suggests that Pb is of crustal origin. 5.4 Sulfur isotopic data Huang GF, Gong SQ, Jiang XW, Tan SX, Li CB, Liu DH (2003) Exploration on the ore-forming regularities of tin deposits in Qitianling area, southern Hunan. Geological Bulletin of China 22: 445-451 Mao JW, Li XF, Lehmann B, Chen W, Lan XM, Wei SL (2004) 40Ar39 Ar dating of tin ores and related granite and its geodynamic significance for rock and ore formation. Mineral Deposits 22: 164175 Marchand L, Joseph D, Touray JC, Treuil M (1976) Critères d’analyse géochimique des gisements de fluorine basés sur l’étude de la distribution des lanthanides- application au gîte de Maine (71Cordesse, France). Mineralium Deposita 11: 357-379 Shu LS, Zhou XM (2002) Late Mesozoic tectonism of Southeast China. Geological Review 48:249-260 Wang DH, Chen YC, Li HQ, Chen ZH, Yu JJ, Lu YF, Li JY (2003) Geochemical and geochemical features of the Furong tin deposit in Hunan and their significance for mineral prospecting. Geological Bulletin of China 22: 50-56 Wei SL, Zeng QW, Xu YM (2002) Characteristics and ore prospects of deposits in the Qitianling area, Hunan. Geology in China 29: 67-75 Zartman RE, Doe BR (1981) Plumbotectonics - the model. Tectonophysics 75: 135-162 Zhao KD, Jiang SY, Jiang YH, Wang RC (2004) Mineral chemistry of the Qitianling granitoid and the Furong tin ore deposit in Hunan Province, South China: Implication for the genesis of granite and related tin mineralization. Accepted by European Journal of Mineralogy Zheng JJ, Jia BH (2001) Geological characteristics and related tinpolymetallic mineralization of the Qitianling granite complex in southern Hunan Province. Geology and Mineral Resources of South China 4: 50-57 Sulfur isotopic compositions of twelve sulfides were analyzed. The δ34S values of sulfides vary from -20.4‰ to 3.2‰. The sulfur isotopic compositions were divided into two groups in the histogram plot. In one group, the sulfur isotopic compositions vary from -0.5‰ to +3.2‰. Sulfur in this group might come from the granite. In the other group, the sulfur isotopic compositions vary from 20.4‰ to -10‰. Sulfur in this group might come from sulfides in strata. 5.5 Lead isotopic data Thirteen sulfides from the ores and ten feldspars from the Qitianling granite were analyzed for Pb isotopic composition. The Pb isotopic composition of both sulfides and feldspars is relatively homogeneous. 206Pb/204Pb, 207Pb/204Pb and 208Pb/204Pb ratios of sulfides are 18.615~18.898, 15.726~15.766 and 38.893~39.077, respectively. The Pb isotopic ratios of feldspars are 18.682~18.970, 15.747~15.774 and 39.030~39.183, respectively. The similarity in Pb isotopic composition in sulfides and feldspars indicates that lead in sulfides might come from the Qitianling granite. The lead isotope data of both sulfides and feldspars were plotted on the upper crust Pb growth curve in a Zartman 6 871 Conclusions Tin mineralization in the Furong tin deposit is related to hydrothermal alteration of the Qitianling granite. The oreforming fluids might be derived from meteoric water. Both the granite and the strata supported the sulfur for mineralization. Water-rock interaction might have released tin and other metals (e.g. Pb and Ti) from the granite. Acknowledgements This work was supported by funding from China National Science Foundation (40221301). References Close Close