LA HERRADURA ORE DEPOSIT: AN OROGENIC GOLD DEPOSIT IN
NORTHWESTERN MEXICO. by
Francisco Javier Quintanar Ruiz
________________________________________
Copyright Francisco Javier Quintanar Ruiz 2008
A Thesis Submitted to the Faculty of the
DEPARTMENT OF GEOSCIENCES
In Partial Fulfillment of the Requirements for the Degree of
MASTER OF SCIENCE
In the Graduate College
THE UNIVERSITY OF ARIZONA
2008
2
STATEMENT BY THE AUTHOR
This thesis has been submitted in partial fulfillment of requirements for the Master of
Science degree at The University of Arizona and is deposited in the Antevs Reading
Room to be made available to borrowers, as are copies of regular theses and dissertations.
Brief quotations from this manuscript are allowable without special permission, provided that accurate acknowledgment of the source is made. Requests for permission for extended quotation from or reproduction of this manuscript in whole or in part may be granted by the Department of Geosciences when the proposed use of the material is in the interests of scholarship. In all other instances, however, permission must be obtained from the author.
Francisco Javier Quintanar Ruiz signature)
APPROVAL BY RESEARCH COMMITTEE
As members of the Research Committee, we recommend that this thesis be accepted as fulfilling the research requirement for the degree of Master of Science.
Joaquin Ruiz
Major Advisor (type (signature)
Eric Seedorff
Lucas Ochoa
Christopher Eastoe
3
ACKNOWLEDGMENTS
I am thankful to Joaquin Ruiz, my advisor, for his assistance in all aspects during this study, particularly for his time spent in the development of my research project and the improvements of the final manuscript. I also would like to thank my committee thesis members. Eric Seedorff for his help and comments during the preparation of this manuscript. Lucas Ochoa for his help and comments during field work and preparation of this manuscript. Chris Eastoe, for guiding me into stable isotope studies, especially for his wise comments on this work.
I am so grateful to Servicios Industriales Peñoles for the financial support for this research, especially to Engineers Jaime Lomelín, Octavio Alvidrez, David Giles,
Victor de la Garza, Luis Novelo and Benito Noguez, for trusting in me. I would also like to thank Engineers Carlos Díaz de León, Martín López, Ramses Tarazón, José de la Torre, Enrique García, Juan Romero and Mr. Jesús Murrieta, for the logistic support and sharing experience during field work. Thanks to Francisca López and
Hector Mendívil for the drawing of some figures.
Thanks to Rafael Del Rio, Victor Valencia, Fernando Barra, Marty Grove, and many others that assisted me during my graduate work. Special thanks to Robert
Kamilli for the help provided in the study of fluid inclusions. Also, Thanks to David
Dettman, Richard Goldfarb and Lukas Zurcher by helping me in the laboratory work and the improvement of this manuscript. Special thanks to Geosciences staff.
Lastly, I am also thankful to my wife Leticia, my son Francisco, and my daughters Eva and Sarah. You are my inspiration! Thanks for your time and your patience. The dedication of this study is for them!
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TABLE OF CONTENTS
LIST OF FIGURES………………………………………….…….………….……….7
LIST OF TABLES………………………………………………………….….……...9
ABSTRACT……………………………………………………………………….…10
CHAPTER 1: INTRODUCTION……………………………………………..……..12
1.1. Introduction and Previous Work ……………………………………….......12
1.2. Mining and Exploration History……………….…..……………..………..…13
CHAPTER 2: GEOLOGIC AND TECTONIC SETTING………….……………….14
2.1. Regional Geologic and Tectonic Setting…………….………………………..14
2.1.1. Pre-Cretaceous Lithologies and Evolution: The Mojave-Sonora
Megashear Hypothesis…………………....………………………………….14
2.1.2. Cretaceous and Younger Events and Lithologies………..………..……..18
2.2. The Geologic Setting of La Herradura…........………………............………..20
2.2.1. Precambrian Lithologies……………………………...……................…20
2.2.2. Paleozoic Units……………………………………...…………………...24
2.2.3. Jurassic Units…………………………………………….....…….……...24
2.2.4. Tertiary and Quaternary Units…...……………………….……...........…25
2.3. The Structural Setting of La Herradura………..…………...……………….....25
2.4. Alteration of La Herradura…………...…………..……………………...…….26
CHAPTER 3: U-PB AND RE-OS GEOCHRONOLOGY FROM LA
HERRADURA GOLD DEPOSITS……………...….……….….………..….30
3.1. Zircon U-Pb Dating……………………..……………….………………….....30
3.1.1. Sampling…………………………….……………….…………………..30
3.1.2. Preparation of Samples……………………………………......................30
3.1.3. Analytical procedures………………………………...………………….30
5
TABLE OF CONTENTS – continued
3.1.4. Results……………………………………………………………...……31
3.2. Pyrite-Magnetite Re-Os Dating…………………………………………..……37
3.2.1. Sampling………………………………………...……………………….37
3.2.2. Analytical Methods…………………………………...……………...….37
3.2.3. Results…………………………………………………………...………38
CHAPTER 4: STABLE ISOTOPES…………………...……………………….……40
4.1. Introduction……...………………………………………………………….…40
4.2. Oxygen and Hydrogen Isotopes……………...………………………….…….41
4.2.1. Sampling…………………...………………………………………….....41
4.2.2. Analytical Methods………………………………………………...……45
4.2.3. Analytical Results………………………………………...……………..46
4.3. Sulfur isotopes……...……………………………………………………….…47
4.3.1. Sampling……………………………………….…………………...……47
4.3.2. Analytical Methods…………………………………………………...…49
4.3.3. Analytical Results………………………………………….....................50
4.3.4 Sulfur Isotope Geothermometry……………………………….............…50
4.4. Carbon Isotopes…………………………………………………………….….53
4.4.2. Analytical Methods…………………………………………………....54
4.4.3. Analytical Results……………………………..…………………...….55
4.5. Interpretation and Discussion………………………………….……………..57
CHAPTER 5: FLUID INCLUSIONS………………………………………………..59
6
TABLE OF CONTENTS – continued
5.1. Introduction………………………………...……………………………………59
5.2. Sampling……………………………………………………………………….60
5.3. Analytical Methods…..…………………………………………………….….61
5.4. Petrographic Characteristics of Fluid Inclusions………………………………65
5.5. Analytical Results……………………………………………………….…….67
5.6. Interpretation and Discussion……………………………………………….…72
CHAPTER 6: DISCUSSION AND CONCLUSIONS………………………………74
6.1. Discussion………………..………………………………………….……….74
6.2. Conclusions…………………………………………………………………....85
REFERENCES
7
LIST OF FIGURES
Figure 2.1. Regional geological map of the La Herradura area…..…………...…….17
Figure 2.2. La Herradura geological map and cross section…..…………….……....22
Figure 2.3. Photomicrographs of representative rocks………………......……...........23
Figure 2.4. Photograph of Victoria shear zone separating Proterozoic gneiss from
Jurassic volcanic rocks…………………………………...........................24
Figure 3.1. Map showing location of samples for U-Pb ages…………………..........35
Figure 3.2. U-Pb ages of zircons..................................................................................36
Figure 3.3. Map of La Herradura mine showing locations of samples used for
Re-Os isotopes…………...………………………………………...……..38
Figure 3.4. Re-Os isochron for La Herradura gold deposit…………………………..39
Figure 4.1. Map of La Herradura mine showing locations of samples used for
oxygen and hydrogen isotopes……..………………………………........42
Figure 4.2. Photographs of representative samples used for stable isotope studies…….……44
Figure 4.3. Map of La Herradura mine, showing location of samples used for
sulfur isotopes……… ………………………………………………………….48
Figure 4.4. Reflected light microphotography showing pyrite with strong fracturing
and later gold mineralization in the fractures……...……………………...……..49
Figure 4.5. Plot of δ 34 S versus elevation .……………………………………………………53
Figure 4.6 Map of La Herradura mine, showing location of samples used for
carbon isotopes……….
…………………………………………….…………..54
Figure 4.7 P lot of δ
13 C versus 1/concentration of C…………………………...……..56
Figure 4.8.
Plot of δ D and δ 18 O of water coexisting with gangue minerals at 330°C…........58
Figure 5.1. Map of La Herradura mine showing locations of samples used for fluid
inclusions petrography and microthermometry studies……………….......62
Figure 5.2. Photograph showing shear veins and associated flat extension veins…...63
8
LIST OF FIGURES -Continued
Figure 5.3. Photograph showing extensional quartz vein with sericite-pyrite
envelope ………………………………………………………………....64
Figure 5.4. Photomicrograph of extensional quartz veins………………..…….…….64
Figure 5.5.
Microphotograph showing quartz vein with carbonate and Fe oxides
as a selvage ……..… ………………………………………………...….......65
Figure 5.6. Photomicrograph showing fluid inclusions…………………...…………66
Figure 5.7. Clathrate melting temperatures for all samples……………….......70
Figure 5.8. Temperatures of homogenization of CO
2
(to liquid) for all samples….70
Figure 5.9. Final homogenization temperatures for all samples…………………..…71
Figure 5.10. Plot of maximum and minimum isochors for fluid inclusions…............71
Figure 6.1. Plot of δ D Vs δ
18 O of water coexisting with gangue minerals…..……..84
9
LIST OF TABLES
Table 2.1. Tectonic and deformation history from La Herradura gold deposit........…28
Table 2.2. Paragenetic sequence of ore and gangue minerals from La Herradura
gold deposit………...……………………………...……………………...29
Table 3.1. U-Pb ages from La Herradura gold deposit………………………………35
Table 3.2. Results of analysis from Re-Os isotopes………...………………………..39
Table 4.1. Description of samples for oxygen and hydrogen isotopes………...……..43
Table 4.2. Oxygen and Hydrogen isotope data…………………………...………….47
Table 4.3. S isotope database and calculated temperatures for deposition of
sulfides…………………………………………………………………….52
Table 4.4. Carbon content and δ
13 C values of fluid inclusion-bearing quartz
and ankerite……………………...………………………………………..54
Table 5.1. Description of samples used for fluid inclusion petrography-
Microthermometry………………………………………….……..........................63
Table 5.2. Microthermometry summary………………………………………..……72
Table 6.1. Oxygen and Hydrogen compositions of quartz-carbonate veins in the
western North American Cordillera and counterparts worldwide……...…83
Table 6.2. Comparison of fluid inclusions results from La Herradura with OGD
located in the circum-Pacific rim of North and South America…………..84
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ABSTRACT
The production plus reserves of La Herradura mine is 5.4 million ounces of gold. The deposit occurs within a northwest trending belt of metamorphic rocks of greenschist and amphibolite facies and granitoids of Proterozoic age. The ore deposit is hosted mainly in a 1.75 Ga quartz-feldspathic gneiss and strikes northwest. The orebody is bordered to the east by the Victoria shear zone, separating Jurassic clastic rocks and subvolcanic intrusions. To the west the orebody is bordered by the Ocotillo shear zone, separating Upper Paleozoic limestone.
Most of the gold mineralization occurs within thin quartz-sulfide veins that follow en echelon tensional swarms. These veins dip at low angles (<30°) and are interconnected to a thicker set of fault-fill higher-grade quartz vein systems. These higher-grade quartz vein systems are believed to be the feeders for gold mineralization in the deposit.
Oxygen isotopes of several quartz veins show consistent δ
18 O values between +14 and +16 ‰. The calculated δ 18 O values for the waters in equilibrium at 330°C for these quartz veins range between +8 to +10 ‰. These values are similar to those of metamorphic waters. Carbon isotopes from fluids inclusions-bearing quartz veins and ankerite, suggest that there are two sources of C, one associated with carbonate minerals, δ
13 C=0 to -6 ‰, and other associated only with fluid inclusions, δ
13 C < -
18 ‰. The low δ
13 C carbon source is organic C. Sulfur isotopes of sulfides in quartzpyrite-galena-sphalerite veins from the Centauro pit have δ
34 S values from +3.1 to
+6.6 ‰. Geothermometry studies using pyrite-galena pairs show equilibrium temperatures on the order of 330 ±20°C for the quartz-sulfide-gold-bearing veins.
11
Fluid inclusion studies from these same veins show that the ore fluids are CO
2
-rich, are low in salinity, have homogenization temperatures between 285-295 °C, and have calculated trapping pressures between 1.6 and 2.7 kbar. The fluids responsible for the mineralization are interpreted to have a metamorphic origin generated during the
Laramide orogeny, as is consistent with isotopic measurements of Re-Os from pyrite and magnetite that accompany gold mineralization which is dated at 61.0 ± 2.1 Ma.
The style and geometry of mineralization, stable isotopes and fluid inclusions studies, show that La Herradura gold deposit can be classified as an orogenic gold-type deposit, the largest and the first orogenic gold-type deposit described in Mexico.
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CHAPTER 1: INTRODUCTION
1.1. INTRODUCTION AND PREVIOUS WORK
The northwestern part of Mexico has similar geology to the southwestern
United States. The most outstanding geologic feature in Mexico, however, is the postulated Mojave-Sonora megashear, which is suggested to have occurred during
Late Jurassic time and separates two Proterozoic blocks of difference ages (Silver and Anderson, 1974). Nourse et al. (2005) alternatively suggest that the two different sequences of Proterozoic rocks in the region resulted from Paleoproterozoic accretion. Iriondo (2001) indicates that juxtaposition of Paleoproterozoic blocks in the Quitovac area represents a Laramide thrust zone and not the original Proterozoic suture between the basement rocks. Regardless of the precise reason, a large-scale structure occurs with the distribution of gold mineralization in northwest of Sonora.
Consequently, previous works on gold occurrences in Sonora emphasize the relationship between gold mineralization and this large-scale structure (Silberman and Giles, 1988).
For La Herradura gold deposit, several internal studies from mining companies focus on the geology of the deposit in order to understand the genesis of the mineralization (Altamirano and Carreón, 1995; López and Díaz de León, 1995;
Salvatierra and Novelo, 1995, de la Garza et al., 1998). Later, during the development of the mine, new studies are dealing with the structural framework and the geology of the deposit (Caddey, 2002; Caddey and García, 2003; de la Torre, 2004; Rhys, 2005; and Romero, 2005).
This study mainly addresses the geochemistry and origin of the ore fluids involved in the formation of the La Herradura gold deposit; in order to explain the geochemistry of the ore bearing fluids and to compare this deposit with orogenic gold deposits located in the Circum-Pacific rim, especially those in North America and Peru.
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1.2. MINING AND EXPLORATION HISTORY
The La Herradura mine contains 5.4 million ounces of contained gold in production plus reserves. The deposit is owned by Minera Penmont, a Joint
Venture between Peñoles and Newmont. As a result of an aggressive grassroot exploration program in northwestern Mexico that started in 1987, the first economic drill intersection in La Herradura came in 1991 (100m @ 0.85 g/t Au).
Subsequent and continuous drilling campaigns resulted in the definition of an orebody containing 1.7 M oz by May 1998, when mine operations started. To date,
2 M oz of gold have been produced. Present reserves are 3.4 M oz of gold in ore with an average grade of 1 g/t, using a cut-off of 0.35 g/t Au. The mine produces
210,000 ounces of gold per year ( Jose de la Torre, pers. commun., 2008).
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CHAPTER 2: GEOLOGIC AND TECTONIC SETTING
2.1. Regional Geologic and Tectonic Setting
La Herradura mine is located in northwestern Sonora, Mexico. This deposit occurs within a northwest trending belt that consists of metamorphic rocks of greenschist and amphibolite facies and granitoids of Proterozoic age (Nourse et al.,
2005). These rocks are intruded by a series of Triassic and Middle Jurassic granitoids and are overlain by younger sedimentary and volcanic rocks of Middle to Late
Jurassic age (Figure 2.1). All these units are intruded by Late Cretaceous to early
Tertiary granitoids related to the Laramide orogeny and are overlain by Miocene rhyolites, andesites, and basalts and Quaternary basalts. Basin and Range tectonics affect this area, as they do much of Sonora and adjacent Arizona. Basin and Range faulting occurred in the mid to late Tertiary. Faulting resulted in the formation of
NW-trending linear ranges of crystalline rock, separated by deep basins filled with sand and gravel derived from the ranges (Figure 2.1). Correlation is difficult between ranges.
2.1.1. Pre-Cretaceous lithologies and evolution: The Sonora-Mojave megashear hypothesis
The interpretation of the pre-Cretaceous geological and tectonic evolution of the region is highly controversial and focuses on the possible existence of the Sonora-
Mojave megashear, which is believed to have an important impact on the distribution of gold mineralization within the region. Many of the gold prospects in Sonora occur within or adjacent to the southwestern boundary of this regional fault that occurs
15 within Precambrian, Mesozoic, and Tertiary rocks (Silberman and Giles, 1988).
Evidence for the Mojave-Sonora megashear is based mainly on geochronological studies of the Proterozoic basement that indicate two different basement blocks with slightly different ages and interpreted differences in Paleozoic to Jurassic cover sequences across the proposed northwest-trending shear trace (Silver and Anderson, 1974). The trace of the shear zone is interpreted to pass north of the town of Caborca and to the west of Quitovac and Sonoyta before extending into southern California. The Caborca block to the west consists predominately of amphibolite and greenschist grade siliciclastic paragneiss and orthogneiss with ages ranging from 1.8 to 1.7 Ga. The North America block to the east consists predominately of orthogneiss and volcanosedimentary paragneiss with ages varying from 1.7 to 1.6 Ga old. La Herradura gold deposit is located in the Caborca block.
The Caborca block, in addition to containing the older Proterozoic basement, is also distinguished by the local presence of Neoproterozoic and Paleozoic strata, including carbonate sequences, that occur west of Caborca and near the La Herradura mine. Such strata are absent, or have non-correlative sequences northeast of the proposed trace of the megashear and east of the region extending from Sonoyta to southeast of Caborca. Pre-Jurassic lithologies are not exposed on the North America block in an area termed the Papago terrane (Haxel et al., 1984; Calmus and Sosson,
1995). Other sequences potentially unique to the Caborca block include Lower to
Middle Jurassic clastic, volcanic, and plutonic rocks, which differ from the predominantly conglomeratic Upper Jurassic to lowermost Cretaceous sedimentary rocks, and rarity of older Jurassic units, northeast of the proposed Megashear trace
(Anderson et al., 2005). Some of these Jurassic to Lower Cretaceous sequences are
16 proposed to have been deposited in pull-apart basins during active displacement along the Sonora-Mojave Megashear (Anderson and Nourse, 2005).
Based on the differences in Proterozoic and Phanerozoic sequences across the proposed trace of the megashear and the general age and lithological similarities of the rocks to the northeast of the megashear in California, several authors (e.g.,
Anderson and Silver, 2005; Stewart, 2005) propose approximately 800-1000 km of left-lateral displacement along the structure. The timing of the displacement suggested by Anderson and Silver (2005) is constrained to Late Jurassic by the youngest affected rocks (mid-Jurassic) and oldest unaffected and overlapping lithologies (Cretaceous). This time corresponds to the initial opening of the Gulf of
Mexico. Alternative hypotheses which also invoke similar large scale displacements include the California-Coahuila transform, involving a major Late Paleozoic to
Triassic left-lateral translation and juxtaposition of the Caborca block in a manner comparable to that of the Jurassic megashear hypothesis (Dickinson, 2000). An alternative to the megashear hypothesis is proposed by Nourse et al. (2005). They suggest that the two packages of Proterozoic rocks in the region are the result of
Paleoproterozoic accretion.
Exposures of northwest trending mylonitic rocks 13 km southwest of the town of Sonoyta near the U.S. – Mexico border (Figure 2.1) have been interpreted by
Campbell and Anderson (1998, 2003) to be the exposed fault rocks of the Sonora-
Mojave megashear. Mylonites in this location affect rocks interpreted to be as young as Lower Jurassic age but are overprinted by Late Cretaceous granite, suggesting that the mylonites formed between these two times. The mylonites contain both sinistral kinematic indicators and locally shallow thrusts associated with down-dip
17
Gold occurrences
Figure 2.1. Regional Geological Map of the La Herradura area. Modified from
Iriondo et al. (2005). Notice the location of Figure 2.2
.
MSM refers to the proposed locations of the Mojave-Sonora Megashear from Anderson and Silver
(2005). MSM (alt) is the alternative position of this possible structure from
Nourse et al. (2005).
18 plunging lineation indicating reverse shear, which collectively are interpreted as sinistral transpression by Campbell and Anderson (2003). However, it is also possible that these mylonites represent the effects of Laramide deformation in the area as documented by Iriondo et al. (2005) in Quitovac 40 km to the southeast, and thus postdate the proposed megashear. Elsewhere, the potential trace of the megashear is hidden under Tertiary and Quaternary rocks or is overprinted by Late Cretaceous plutons and the effects of Laramide deformation and mid-Tertiary Basin and Range extension. Further age dating, mapping, and structural studies are necessary to place the trace of the MSM into a more detailed context.
The presence of large-scale structures is a characteristic widely documented at
OGD worldwide. For example, these regional structures are observed in the early-
Eocene orogenic gold deposits in the Juneau gold belt, Alaska (Goldfarb, 1988), the late-Jurassic and Early Cretaceous Mother Lode in California (Böhlke and Kistler,
1986; Elder and Cashman, 1992), the Carboniferous orogenic gold deposits in Peru
(Haeberlin, 2002), the Archean deposits in the Superior and Yilgarn cratons in Canada and Australia, respectively (Robert et al., 2005). Consequently, large-scale structure, related either to MSM or Paleoproterozoic accretion, is a positive factor in the exploration for OGD in northwestern Sonora, where several gold occurrences exist, and can be related at least in space to the same reservoir.
2.1.2. Cretaceous and younger events and lithologies
The Upper Cretaceous intrusions and all pre-Cretaceous units have been affected by regional Late Cretaceous to early Tertiary Laramide deformation, which is constrained in the Quitovac region, 40 km northeast of La Herradura, by the age of
19 the affected Cretaceous intrusions, 40 Ar39 Ar studies of metamorphic rocks in associated thrusts, and post-Laramide volcanosedimentary sequences range between
75 and 39 Ma (Iriondo et al., 2005). Laramide deformation in the area is associated with development of mainly northeast vergent folds and thrusts, inhomogeneous eastwest to northwest trending foliation in lower greenschist grade rocks, and generally steeply plunging elongation lineation which formed in response to regional northeastsouthwest to north-south directed shortening (e.g., Nourse, 2001; Iriondo et al., 2005).
Post-Laramide tectonic events in the region are dominated by extensional and transtensional faults that affect rocks as young as the Miocene calc-alkaline volcanic rocks of the El Pilar sequence, which occurs east of the La Herradura deposit (Iriondo et al., 2005). Mid-Tertiary, Basin and Range extension in the region is widespread. It is characterized by local development of metamorphic core complexes and shallow dipping foliations and by northeast- and southwest-dipping normal and detachment faults that locally remobilize Laramide thrust surfaces. These latter structures are probably largely responsible for the current topography, which is dominated by north to northwest trending outcrop ridges and intervening covered valley areas. In La
Herradura district, these faults affect both Precambrian and Jurassic blocks and displace the orebody (See section in Figure 2.2). A second set of northeast trending dextral faults identified by Iriondo et al. (2005) in the Quitovac area overprint the northwest trending extensional structures. Late Miocene to Recent tectonics in the region is dominated by dextral activity of the northwest trending San Andreas and subsidiary fault systems associated with opening of the Gulf of California.
The youngest rocks in the area are basaltic lava flows associated with Cerro
Pinacate, approximately 80 km north of La Herradura. A series of probable coeval
20 isolated minor eruptive centers, dikes, and erosional basalt flow remnants that occur along valleys in the region are potentially related to volcanism along dextral transform faults related to the San Andreas Fault system.
2.2. The Geologic Setting of La Herradura
La Herradura mine occurs within a northwest trending belt of Proterozoic rocks consisting of greenschist and amphibolite grade metamorphic rocks and granitoids. The deposit is hosted in biotite-quartz-feldspar and quartz-feldspathic gneisses that are bordered to the east by Jurassic clastic rocks and subvolcanic intrusions and to the west by upper Paleozoic limestone. Isolated outcrops of fresh andesite, trachyte, and basalt occur locally northeast of the mine.
2.2.1. Precambrian lithologies
The belt of Precambrian rocks that are the host rocks for La Herradura mine is part of the Caborca block as described by Silver and Anderson (1974). These rocks have also been described at Sierra Pinta (Araux-Sánchez, 2000) located 20 km to the north of La Herradura and to the southeast near the town of Caborca (Anderson and
Silver, 2005; Nourse et al., 2005). This Proterozoic block comprises a northwest elongate, 2-km wide, Proterozoic structural block (de la Torre, 2004) that is bordered by two large shear zones. The eastern Victoria shear zone separates Precambrian rocks from Jurassic rocks (Figure 2.2 and 2.5), and the western Ocotillo shear zone separates Proterozoic rocks from Paleozoic rocks. The age for the gneiss ranges between 1.7 to 1.8 Ga (Silver and Anderson, 1974) and are coincident with new
21 isotopic U-Pb ages from zircons obtained in this study. These host rocks are composed principally of biotite-quartz-feldspar and biotite-poor quartz-feldspathic paragneiss. The protolith represents a metamorphosed clastic sequence of impuresandstone-siltstone, and arkosic sandstone to quartzite. Pegmatite dikes and segregations dominated by K-feldspar-quartz also are common within this unit.
Gradational contacts of the pegmatites with surroundings lithologies and common occurrences of coarse aggregates of anatectic K-feldspar + quartz + biotite segregations in the gneiss sequence suggest that the pegmatites formed by partial melting of the gneiss sequence at or near peak metamorphic conditions. Locally, coarser grained bodies of probable tonalite and granite composition are present to the northwest of Centauro Pit. The paragneisses are weakly foliated, internally massive to crudely banded biotite-poor quartz-feldspathic gneiss, forming several lenses up to
300 m thick. These rocks normally exhibit strong fracturing and are crosscut by numerous quartz veins. In thin section, the quartz feldspar gneiss is composed primarily of quartz and K-feldspar. Secondary minerals, in the core of the mineralized zone, are mainly albite and sericite replacing feldspars (Figure 2.3A), and relicts of fresh and/or oxidized pyrite and hematite after pyrite. In the periphery of the mineralized zone, the plagioclase and biotite of the quartz-feldspar-biotite gneiss have been replaced partially by chlorite and epidote.
22
Oc otill o S hea r Z one
Paleozoic
Limestone
Projected
Megapit cto ria S hea r Z on e
Jurassic
Ms-Mv
Yaqui
Pit
Centauro
Pit
O co lo til h
S r Z ea on e
O co lo til h
S r Z ea on e
Paleozoic
Limestone
Proterozoic
Gneiss
Vic tor ia S he ar
Jurassic
Ms-Mv
Zo ne
Figure 2.2. La Herradura geologic map and cross section. Modified from de la Torre
(2004).
A
23
Sericite
K-Feldspar
0.2 mm
B
Chlorite + epidote
0.2 mm
Figure 2.3. Photomicrographs. A is showing quartz-feldspar gneiss under microscope. Note the abundant sericite that is interpreted to have been derived mainly from metamorphic reactions and to a lesser extent by hydrothermal replacement of feldspar. Polarized light. B is showing andesite under microscope. Note strong chlorite-epidote replacing previous ferromagnesian minerals. Polarized light.
QFG
1737 +-20 Ma
RHYOLITE
168 +-3.5 Ma
ANDESITE
159 +-3.5 Ma
24
Figure 2.4. Photograph of Victoria shear zone separating Proterozoic gneiss from
Jurassic volcanic rocks. New ages from this study by using U-Pb isotopes are indicated.
2.2.2. Paleozoic units
The oldest Phanerozoic lithologies in the area are Paleozoic limestone with subordinate quartzite and chert that lie to the west and northwest of La Herradura mine (Figure 2.2). Although these lithologies are frequently recrystallized to marble and highly strained, they still contain recognizable conodonts that range in age from
Mississippian to Permian (Poole et al., 2004). This unit is separated from the mineralized Proterozoic gneiss block by the Ocotillo shear zone and does not host gold mineralization.
2.2.3. Jurassic units
To the east and northeast of the Proterozoic gneiss belt, and separated by the
Victoria Shear zone, lies a Jurassic unit, composed of a diverse assemblage of clastic sedimentary rocks, rhyolitic sills and/or extrusive equivalents and andesitic
25 flows/dikes (Figure 2.2). These units are comparable to those units described previously in the Caborca block (Anderson and Silver, 2005). Under the microscope, the rhyolite exhibits a primary mineralogy dominated by quartz and feldspar. The secondary minerals are epidote, sphene, chlorite, sericite and calcite. This rock is weakly metamorphosed or contains only lower greenschist grade assemblages. The andesite shows a strong propylitic alteration where ferromagnesian minerals have been replaced by chlorite, epidote, and sphene (Figure 2.3B). In general, this rock is not deformed or metamorphosed. These Jurassic units are not affected by the gold mineralization in La Herradura mine.
2.2.4. Tertiary and Quaternary Units
Tertiary rocks are andesites and trachytes. These rocks outcrop to the northeast of La Herradura district and generally trend northwesterly. Younger basalts outcropping northeast of Centauro pit are associated with the Pinacate volcanic field, located 80 km north of the La Herradura. Outcrops of Quaternary basalts also have a general northwest trend.
2.3. The Structural Setting of La Herradura
As is published by de la Torre (2004) and Romero (2005), the orebody of La
Herradura is hosted within shear zones in the more competent quartz-feldspar gneiss.
Gold mineralization is bounded to the east and west by the Victoria and Ocotillo shear zones, respectively. Shear zones exhibit a northwest trend and are controlled by premineral reverse faults that appear to have been reactivated during Laramide time.
Most of the gold mineralization occurs within thin quartz-sulfide (leached in outcrop)
26 veins that follow en echelon tensional swarms. These veins are dip at low angles
(<30°) and are interconnected to a thicker set of fault-fill higher-grade quartz vein systems. These higher-grade quartz vein systems are believed to be the feeders for gold mineralization in the deposit. At depth, these veins may be coalescing into one single large shear fault system that served as a channel for the ascending of ore fluids.
In La Herradura mine, there is a strong correlation between the grade of gold in the thin extensional quartz veins and the proximity to fault-fill higher-grade quartz vein systems. Robert and Poulsen (2001) noted that extensional veins and vein arrays are generally of lower economic significance, but they can be important ore hosts in competent rocks or in areas adjacent to the fault-fill vein systems.
Based on structural mapping in the La Herradura mine area, it is possible to identify at least five tectonics events superimposed on all stratigraphic units outcropping in this area (de la Torre, 2004; Romero 2005, Table 2.1). These observations indicate that gold mineralization is associated with the third tectonic event, and they also tend to constrain the age of this mineralization to between 80 and
45 Ma.
2.4. Alteration of La Herradura
Reported alterations assemblages of this deposit (de la Torre, 2004; Romero,
2005) are quartz-sericite-albite in the core of the deposit and selectively follow the quartz-feldspar gneiss bands in the outer zones of the deposit. Iron-carbonates
(ankerite-siderite) are widespread within the deposit, mainly restricted to haloes adjacent to quartz-sulfide veins within the core of the orebody. Iron carbonates also are found in the outer alteration aureoles of the deposits. Propylitic alteration is
27 located in the outermost portions of the deposit, and it occurs mainly in the biotitebearing gneiss and in Jurassic rhyolitic and andesitic volcanic rocks.
The paragenesis for La Herradura gold deposit comprises seven different mineralogical associations; three of them are related to the gold mineralization (Table
2.2). Gold mineralization is mainly associated to quartz- galena-sphalerite and quartzhematite veins (2 d and 3 rd stages), however milky quartz veins are also carrying some gold (4 th stage).
28
Table 2.1. Tectonic and Deformation History from La Herradura Gold Deposit. Modified from de la Torre (2004) and Romero (2005).
Relative
Age
Geological Age
Quaternary 1 Ma
Tectonic environment
Tectonic
Major Event
Tectonic
Secondary event
Strain type σ 1 Orientation
Volcanic fissural rocks related to San Andrés Fault System (El Pinacate Complex). Rocks outcropping near the La Herradura mine.
Middle Miocene Brittle Depth<
20-12 Ma 10 km
D5
D4
NW 56_47 SE
NE 25_18 SW
Laramide D3
Pulse 5
D3e
Sense of Displacement
Right lateral
Normal Oblique
Left-lateral Reverse-oblique
Right lateral
Left-lateral Reverse-oblique
D3d; Step 3 Brown color quartz, calcite, ± goethite; barren to weak gold-bearing
Upper
Cretaceous to
Lower Tertiary
80-45 Ma
D3c; Step 2 Quartz-hematite-gold ± wulfenite ± galena. Main gold mineralization
Laramide
Brittle-Ductile 12 -
10 km depth
D3
D3
Pulse 2,3,4
Pulse 1
D3a
5 compressive pulses
D3b; Step 1 Quartz-goethite; barren to weak gold-bearing
Horizontal compression and vertical extension
NE 44_35 SW
NE 44_41 SW
NE 80 SW
Inverted section and thrust faults
Left-lateral Reverse-oblique
Intense horizontal compression and vertical extension
Middle Jurassic
187-163 Ma
Brittle-Ductile 15 -
13 km depth
D2 Compression and extension
NE 51 SW
Mohave Sonora Megashear
Reverse
Lower Jurassic
208-187 Ma
Paleozoic
315-286 Ma
Precambrian
Metasediments and metavolcanics, magmatic arc affinity. Greenschist metamorphic facies
Calcareous rocks: Limestones and dolomites with intense shearing, no foliation, no metamorphism. Corals and Brachiopods from
Carboniferous
D1b
Younger events have rotated their original positions
Extension
Ductile, depth >
15 km
D1
D1a
Intense
Compression
NE SW Left-lateral Reverse-oblique
Greenschist to amphibolite metamorphism grade on sedimentary rocks (1750 Ma). Sediments being deposited
29
Table 2.2. Paragenetic sequence of ore and gangue minerals from La Herradura gold deposit (modified from Altamirano and Carreón, 1995).
Event
5
6
7
3
4
1
2
Mineralogical association
Quartz-pyrite
*Quartz-galena-sphalerite
*Quartz-hematite
*Quartz (milky)
Quartz-siderite-ankerite
Siderite-ankerite
Calcite
The precipitation of gold from hydrothermal ore-forming fluids, in order to form the orebody, is produced by changes in the fluid chemistry that remove gold from solution by destabilizing aqueous Au-S complexes. This destabilization could be accomplished by cooling, oxidation, reduction, decreasing of pH or lowering S of the fluids. This modification of fluids chemistry, can be achieved by any of the following: (1) large-scale pressure and temperature gradients along the fluid plumbing system; (2) reaction of the fluid with the wall rocks surrounding the conduit; (3) transient pressure fluctuations inducing phase immiscibility in the fluid; (4) fluid mixing; or (5) chemisorption (Kerrich et al., 2000).
30
CHAPTER 3: U-PB ZIRCON GEOCHRONOLOGY FROM LA HERRADURA
GOLD DEPOSIT.
3.1 Zircon U-Pb Dating
3.1.1 Sampling
Six samples from outcrops of different rock units were collected for dating by
U-Pb isotopes (Figure 3.1, Table 3.1). The main purpose of this study was to obtain the age of the Precambrian rocks that host gold mineralization in the La Herradura gold deposit and of Jurassic rocks exposed to the east of the orebody. These ages are also crucial for an understanding of the tectonic history of the area.
3.1.2 Preparation of Samples
Zircon crystals were separated from the rocks by traditional crushing, followed by magnetic, and by gravimetric separation techniques. Heavy mineral concentrates of the <350 micron fraction were separated magnetically. Inclusion-free zircons from the non-magnetic fraction were then handpicked under a binocular microscope. At least fifty zircons from each sample were mounted in epoxy and polished for laser ablation analyses. Before the isotopic analysis, the zircons were studied by Scanning Electron Microscopy (SEM) and cathodoluminiscence in order to determine the presence of inherited cores or any other complexity.
3.1.3 Analytical Procedures
Zircon crystals were analyzed in polished section with a Micromass Isoprobe multi-collector Inductively Coupled Plasma Mass Spectrometer equipped with nine
Faraday collectors, an axial Daly detector, and four ion-counting channels (Gehrels et al., 2008). The Isoprobe is equipped with an ArF Excimer laser, which has an emission wavelength of 193 nm. Analyses were conducted on 25- to 35-micron spots with output energy of ~80 mJ (at 23kV) and a repetition rate of 8 Hz. Each analysis consisted of one 20-second integration on peaks with no laser firing and twelve 1second integrations on peaks with the laser firing. The Hg contribution to the 204 Pb
31 mass position is accordingly removed by subtracting the on-peak background values.
The depth of each ablation pit was ~15 microns. The total measurement time was ~90 s per analysis.
The collectors were configured for simultaneous measurement of 204 Pb in an ion-counting channel while 206 Pb, 207 Pb, 208 Pb, 232 Th, and 238 U are measured with
Faraday detectors. All analyses were conducted in static mode. Inter-element fractionation was monitored by analyzing fragments of a large concordant zircon crystal from Sri Lanka with a known (ID-TIMS) age of 564 ± 4 Ma (2 σ ) (Gehrels et al., 2006). This reference zircon was analyzed once for every four unknown samples.
The reported ages for zircon grains are based on 206 Pb/ 238 U ratios because errors of the 207 Pb/ 235 U and 206 Pb/ 207 Pb ratios are significantly higher. This is due primarily to the low intensity (commonly <1 mV) of the 207 Pb signal from these young, low-U grains. The 206 Pb/ 238 U ratios are corrected for common Pb by using the measured 206 Pb/ 204 Pb, common Pb composition from Stacey and Kramers (1975), and respective uncertainties of 1.0 and 0.3 for 206 Pb/ 204 Pb and 207 Pb/ 204 Pb.
For each sample, the 206 Pb/ 238 U ages are plotted with two-sigma error bars that reflect only the error from determining 206 Pb/ 238 U and 206 Pb/ 204 Pb. The weighted mean of each sample was calculated using the Isoplot program (Ludwig, 2003). For the age of each sample, additional uncertainty from the calibration correction, decay constant, common lead composition and variation in measured 206 Pb/ 238 U and 206 Pb/ 207 Pb of the standard are considered. These systematic errors (1.0-1.7 %) were added quadratically to the measurement error (~1.1-1.2%). The reported ages are based primarily on
206 Pb/ 238 U ratios for <1000 Ma grains and 206 Pb/ 207 Pb for >1000 Ma grains. All reported ages and weighted mean ages have uncertainties at the two-sigma level.
3.1.4 Results
Sample LH-1
32
Fifty-six zircon grains were measured from the quartz-feldspar gneiss hosting the orebody, sample LH-1. The sample was collected to west of the Victoria shear zone. Zircons analyzed are clear reddish in color and range from 80 to 300 μ m in size. They are doubly-terminated prisms dominated by the [100] face (Pupin, 1980), with a 2-3:1 length to width ratio, which is typical morphologies of zircons in igneous rocks. Measurements were made at the center and tip of the zircons. Zircons from this sample have U concentrations that vary from 350 to180 ppm and U/Th ratios of
~2-3, characteristic of igneous zircons (Rubatto et al., 2002). These zircons yielded a weighted average 206 Pb/ 207 Pb age of 1737 ± 19.5 Ma (n=56, MSWD =0.22, Figure
3.2). In the fifty-six grains analyzed, an older component was not detected.
Sample LH-2
Twenty-five zircon grains were measured from volcanic rhyolite, sample LH-
2. The sample was collected lo to east of the Victoria shear zone. Zircons analyzed are clear, transparent to pinkish in color, and range from 120 to 300 μ m in size. They are doubly-terminated prisms dominated by the [100] face (Pupin, 1980), with a 3-5:1 length to width ratio, which is typical morphologies of zircons in igneous rocks.
Measurements were made at the center and tip of the zircons. Zircons from this sample have U concentrations that vary from ~600-~400 ppm and U/Th ratios of ~1-
2, characteristic of igneous zircons (Rubatto et al., 2002). These zircons yielded a weighted average 206 Pb/ 238 U age of 167.8 ± 3.5 Ma (n=22, MSWD =0.2; Figure 3.2).
In the twenty-five grains analyzed, Mesozoic (186, 214 Ma), Paleozoic (372 Ma) and mid-Proterozoic (1.4 Ga) components were detected.
33
Sample LH-3
Twenty-eight zircon grains were measured from tonalite, sample LH-3. This rock outcrops northwest of Centauro pit. Zircons analyzed are reddish in color, which is the product of the radiation damage, and range from 90 to 250 μ m in size. They are prisms dominated by the [100] face (Pupin, 1980), with a 2-4:1 length to width ratio, which is typical morphologies of zircons in igneous rocks. Measurements were made at the center and tip of the zircons. Zircons from this sample have U concentrations that vary from ~2800 to ~450 ppm and U/Th ratios of ~2-3, characteristic of igneous zircons (Rubatto et al., 2002). These zircons yielded a concordant age of 1651.9 ±
15.3 Ma (n=18; Figure 3.2). In the twenty-eight grains analyzed, an older component that is ~1716-1792 Ma in age was detected (n=8 cores).
Sample LH-4
Twenty-nine zircon grains were measured from granite, sample LH-4. This rock outcrops northwest of Centauro pit. Zircons analyzed are reddish in color, which is the product of the radiation damage, and range from 90 to 250 μ m in size. They are prisms dominated by the [100] face (Pupin, 1980), with a 2-4:1 length to width ratio, which is typical morphologies of zircons in igneous rocks. Measurements were made at the center and tip of the zircons. Zircons from this sample have U concentrations that vary from ~3000 to ~800 ppm and U/Th ratios of ~2-4, characteristic of igneous zircons (Rubatto et al., 2002). These zircons yielded a concordant age of 1756.3 ±
33.4 Ma (n=18; Figure 3.2). In the twenty-nine grains analyzed, a ~1786-1855 Ma older component was detected (n=10 cores).
34
Sample LH-5
Twenty-two zircon grains were measured from quartz-feldspar gneiss, sample
LH-5. This sample was collected from outcrops in Yaqui pit. Zircons analyzed are reddish in color, which is the product of the radiation damage, and range from 90 to
300 μ m in size. They are prisms dominated by the [100] face (Pupin, 1980), with a 2-
4:1 length to width ratio, which is typical morphologies of zircons in igneous rocks.
Measurements were made at the center and tip of the zircons. Zircons from this sample have U concentrations that vary from ~850 to ~150 ppm and U/Th ratios of ~1 to 3, characteristic of igneous zircons (Rubatto et al., 2002). These zircons yielded a weighted average 206 Pb/ 207 Pb age of 1735 ± 21.8 Ma (n=22, MSWD =0.31, Figure
3.2). In the twenty-two grains analyzed, no older component was detected.
Sample LH6
Forty-two zircon grains were measured from metaandesite, sample LH-6. This rock outcrops east of the Victoria shear zone. Zircons analyzed are clear, transparent to pinkish in color, and range from 120 to 300 μ m in size. They are doubly-terminated prisms dominated by the [100] face (Pupin, 1980), with a 3-5:1 length to width ratio, which is typical morphologies of zircons in igneous rocks. Measurements were made at the center and tip of the zircons. Zircons from this sample have U concentrations that vary from ~3000-~200 ppm and U/Th ratios of ~0.5 to ~3, characteristic of igneous zircons (Rubatto et al., 2002). This sample yielded a 206 Pb/ 238 U age, calculated using the TuffZirc Algorithm (Ludwig, K.J., 2003), of 159.0 +3.5 -3.7 Ma
(n=23, Figure 3.2). In the forty-two grains analyzed, a ~1608-1785 Ma older component was detected (n=10 cores).
35
LH-3
LH-4
Vic tori a S hea r Z on e
LH-2
LH-1 LH-6
Jurassic
Ms-Mv
Projected
Megapit
Yaqui
Pit
LH-5
Oc otil lo S hea r Z on e
Paleozoic
Limestone
Proterozoic
Gneiss
Centauro
Pit
Figure 3.1. Map showing location of samples for U-Pb dating. Coordinate system
is UTM, NAD27.
Sample east north masl Rock type age (Ma)
LH-1
LH-2
LH-3
LH-4
321,830
321,826
320,493
320,430
322,661
3,448,829
3,448,936
3,448,943
3,448,835
3,447,941
200
226
231
204
98
Quartz-Feldspar gneiss
Metarhyolyte
Tonalite
Granite
1737 ± 19.5
167.8±3.5
1651.9 ± 15.3
1756.3 ±33.4
1735 ±21.8
LH-5 Quartz-Feldspar gneiss
LH-6 322,302 3,448,844 230 Metaandesite 159 +3.5, -3.7
Table 3.1. U-Pb ages from La Herradura Gold Deposit. Coordinates are UTM
NAD27.
Figure 3.2. U-Pb ages from zircons. box heights are 2 σ
TuffZirc Age = 158.97 +1.47 -1.91 Ma
TuffZirc age
36
37
3.2 PYRITE-MAGNETITE RE-OS DATING
3.2.1 Sampling
Five samples of quartz-pyrite and quartz-pyrite-magnetite veins from diamond drill cores were collected for dating by Re-Os isotopic analysis (Fig. 3.3). The main purpose of this study is to constrain the age of mineralization in the La Herradura gold deposit.
3.2.2 Analytical methods
The analytical procedure is the same as reported in Barra et al. (2003). Rock samples containing pyrite and magnetite were crushed, and mineral phases of interest were handpicked. About 0.8 g of sample was loaded in a Carius tube and dissolved in a 3:1 mixture of HNO
3
and HCl following the procedures described by Shirey and
Walker (1995). Hydrogen peroxide was added to ensure complete oxidation of the sample and spike equilibration (Frei et al., 1998). The carius tube was heated to ~220
° C overnight and the solution was later treated in a two-stage distillation process for
Os (Nägler and Frei, 1997). Re was extracted and purified through column chemistry
(Shirey and Walker, 1995). Os was loaded on platinum filaments, whereas Re was loaded on nickel filaments and later analyzed by negative thermal ion mass spectrometry (NTIMS) (Creaser et al., 1991).
Reported uncertainties listed in Table 1 for both the 187 Re/ 188 Os and
187 Os/ 188 Os ratios were calculated using error propagation. The isochron age was calculated using Isoplot (Ludwig, 2001).
38
Figure 3.3. Map of La Herradura mine showing locations of samples used for
Re-Os isotopes. Coordinate system is UTM, NAD27.
3.2.3 Results
The results for the analysis of three different pyrite samples and a magnetite sample (replicated) are shown in Table 3.2. The samples yielded a five-point isochron (Fig. 3.4) with an age of 61.0 ± 2.1 Ma and an initial 187 Os/ 188 Os ratio of
0.358 ± 0.009 (MSWD = 0.45). The concentrations of Re and Os range between 0.5-
3.0 ppb and 12-41 ppt, respectively.
39
Table 3.2. Results of analysis from Re-Os isotopes.
Sample
14-2
17-5
Mineral phase pyrite pyrite
17-6 pyrite
18-1-1 magnetite
18-1-2 magnetite
187
Os/
188
Os
0.7558
0.7374
0.6107
0.5241
0.5369
Error
0.004
0.010
0.006
0.006
0.005
187
Re/
188
Os Error Os (ppb) Re (ppb)
390.30
372.51
251.02
160.86
177.25
6.33
0.041
3.042
6.19
0.014
0.956
4.07
0.012
0.603
2.66
0.015
0.468
2.97
0.017
0.575
Figure 3.4. Re-Os isochron for La Herradura gold deposit.
40
CHAPTER 4: STABLE ISOTOPES
4.1 Introduction
Because water is the dominant constituent of ore-forming fluids, knowledge of the waters origin is fundamental to any theory of ore formation (Taylor, 1974).
Natural waters of various origins exhibit systematic differences in their hydrogen and oxygen isotopic contents that can be deciphered by measuring stable isotopes ratios.
Stable isotopic data can place a number of constraints on the source of the veinforming fluids and associated gold mineralization and the conditions of vein formation (Ohmoto and Rye, 1979; O’Neil, 1986; Kerrich, 1987; Ohmoto and
Goldhaber, 1997; Jia and Kerrich, 1999; Jia et al., 2000, 2001). For this reason, in the last four decades there have been a considerable number of studies that investigated the practical use of stable isotopes to explore for a range of hydrothermal mineral deposits. The studies have concentrated on the existence and extent of oxygen and hydrogen isotopic haloes within and beyond the limits of visible wallrock alteration, and the use of stable isotopes as vectors to ore zones by sampling limited exposures such as exploration drillholes (Bierlein et al., 2004).
Stable isotope studies in orogenic gold deposits (OGD) have been carried out extensively in the last twenty-five years for those deposits. This type of deposit is located mainly in the most gold-productive Precambrian shields in Australia and
Canada, particularly the Late Archean greenstone belts and Paleoproterozoic fold belts, and in the late Neoproterozoic and younger Cordilleran-style orogens mainly along the margins of Gondwana, Laurentia and the more recent circum-Pacific (Cox et al., 1995; Goldfarb et al., 1988, 1991; Jia et al., 2001, 2003; Haeberlin, 2002;
Bierlein et al., 2004; Shelton et al., 2004; Salier et al., 2005).
41
The purpose of this study is to obtain oxygen, hydrogen, and sulfur isotopic data from gold-bearing quartz-sulfide veins and their sericite alteration haloes in order to constrain the origin of the fluids. Coupled with geological observations, these measurements will lead to a better understanding of the orebody and can be compared with previous data published from known orogenic gold deposits from North America and South America.
4.2 Oxygen and Hydrogen Isotopes
4.2.1 Sampling
For oxygen isotopes, 16 samples of quartz and quartz-carbonate veins were collected from outcrops and diamond drill cores in and around the Centauro pit area
(Figure 4-1). The sample set includes quartz veins from all previously distinguished events according to the paragenetic sequence of ore and gangue minerals described for La Herradura deposit (de la Torre, 2004). The set of samples is also trying to cover all types of quartz veins, according their differences in color, shape, thickness, mineralogical association, attitude, crosscutting relationships, and depth in the deposit
(Table 4.1, Figure 2.2). All of these quartz vein samples are hosted in quartz-feldspar gneiss, and most of them have sericitic haloes (Figure 4.2). Some of the veins come from deep holes (e.g., 650 m) below and around the Centauro pit. These veins carry high values of gold that correlate closely with the presence of sulfide mineralization like pyrite, galena and sphalerite (Figure 4.2). Individual pieces of quartz veins were crushed gently and, from each sample a small fragment measuring between 100 to
200 microns size was mounted in epoxy along with oxygen isotope standards and polished to expose the sample interiors.
42
For hydrogen isotopes, 15 samples were collected from outcrops and cores from diamond drill cores in and around the Centauro Pit (Figure 4.1). Sericite was hand-picked under a microscope from intergrown vein quartz or from the innermost part of the sericitic alteration halo and was analyzed for its hydrogen isotope composition. The sericite is clearly hydrothermal in origin and is not remnant wallrock phase; although in the samples coming from alteration haloes some isotopic heritage from the wall rock can be expected.
Figure 4.1. Map of La Herradura mine showing locations of samples used for
oxygen and hydrogen isotopes. Coordinate system is UTM, NAD27.
43
Table 4.1. Description of samples for oxygen and hydrogen isotopes from La Herradura Gold Deposit.
Sample East North MASL Description
478-2 322,186 3,447,835 127 Quartz-pyrite-siderite-ankerite vein. 3 mm thicknes. Host rock is Quartz Feldspar Gneiss.
478-4
478-5
525-1
525-2
528-1
528-3
530-1
530-2
530-3
531
532-2
533
HGT-14, 487.30m
HGT-14 488.70m
HGT-14, 541.40m
HGT-14, 541.40m
HGT-14, 570.10m
HGT-14, 570.35m
HGT-16 344.90m
HGT-17 651.90m
LH-AE
-317
-318
-369
-369
-58
-60
-35
-33
-397
-397
-120
-678
118
-60
-60
-58
-58
127
127
-65
-65
3,447,089
3,447,104
3,447,092
3,447,094
3,447,251
3,447,251
3,447,243
3,447,243
3,447,835
3,447,835
3,447,165
3,447,165
3,447,114
3,447,114
3,447,089
3,447,089
3,447,238
3,447,238
3,447,823
3,447,297
3,447,325
322,259
322,269
322,258
322,271
322,734
322,734
322,724
322,724
322,186
322,186
322,321
322,321
322,276
322,276
322,259
322,259
322,718
322,718
321,576
322,481
322,263
Quartz vein 5 cm thicknes, microbreccia, sericite haloes.
Quartz-sericite vein 3 cm thickness, siderite-ankerite at borders.
Quartz-carbonate extensional vein 10 Cm thickness, carbonates are in the borders. Host rock is Quartz Feldspar Gneiss. Sericitepyrite alteration.
Deformed, early quartz vein 2 cm thickness, no sulfides. Cutting early deformed Fe-carbonate vein. Host rock is Quartz Feldspar
Gneiss.
Quartz-Fe-oxide (Py)-Fe-carbonate (ankerite). 2 Cm thickness. Sericite alteration halo.
Quartz-Fe-oxide (Py)-Fe-carbonate (ankerite). 2 Cm thickness. Sericite alteration halo.
Quartz-pyrite (now hematite) veins 2 cm thickness, Sericitic alteration halos.
Quartz-pyrite (now hematite) veins 2 cm thickness, Sericitic alteration halos.
Quartz crystals euhedral habit with hematite (on pyrite case) disseminated and on fractures. Sericitic alteration halos.
Quartz-pyrite vein 1 cm thickness. Sericitic alteration halo
Quartz-pyrite (now hematite) vein, 2 cm thickness, white color,low-dipping. This zone corresponds to high-grade mineral (2 g/t gold). Sample comes from a quartz crystal.
Quartz-Fe-carbonate vein, subhorizontal. Pyrite disseminated + Au.
Light gray quartz vein, 20 cm width on Quartz Feldspar Biotite Gneiss. Qz has disseminated pyrite clusters <1 cm. Sericite alteration halo
Quartz-pyrite-sphalerite vein, 8 mm thickness, sericitic alteration halo
Quartz-pyrite-sericite 13 mm thickness. Host rock is Quartz Feldspar Gneiss. Sericite from the core of the vein.
Quartz-pyrite-sericite 13 mm thickness. Host rock is Quartz Feldspar Gneiss. Sericite from alteration halo
Quartz-pyrite-sphalerite vein, irregular form, 2 cm thickness, sericitic alteration halo.
Quartz-pyrite-galen vein, 4 mm thickness. Sericite halo. Host rock is Quartz Feldspar gneiss
Light gray quartz veinlet, cut by siderite-ankerite. Drusic textures.
Quartz-Pyrite (5 mm) vein 10 mm thickness. Host rock is Quartz Feldspar Gneiss
Quartz milky color, 50 Cm thickness.
44
Se
Ak
A
Hm
C
Qz
B
Qz
Se
Hm
Se
Qz
D
E F
Qz
Sf
Se
Qz
Sf
Figure 4.2. Representative samples used for stable isotope studies. A . Sample 528.
Quartz-iron carbonate-pyrite (now hematite) vein, sericite haloes with disseminated hematite after pyrite.
B
. Sample 530-2. Quartz-hematite after pyrite with sericite haloes.
C
. Sample LH-AE. Milky quartz, strong fracturing, collected from a quartz shear vein being the feeders for gold mineralization.
D
. HGT-14 541.40. Quartzsericite vein with sericite haloes. This sample is coming from deep drill holes beneath the actual mining exploitation in Centauro pit.
E
. Sample HGT-13 643.30m. Quartzpyrite-sphalerite-galena vein with sericitic halo. This sample is from deeper diamond drill holes in the Centauro pit. A 2-m width geochemical sample containing this vein has 6 g/t gold, indicating that there is a spatial relationship between gold and sulfides.
F . Sample HGT-17 655.85m. Quartz-pyrite-sphalerite-galena vein from deeper diamond drill holes in the Centauro pit. Geochemical assay from a 2-m interval sample containing this vein assays 1.8 g/t gold. Ak: ankerite, Hm: hematite, Qz: quartz, Se: sericite, Sf: sulfide.
45
4.2.2 Analytical Methods
The oxygen isotopic compositions of quartz pieces were measured in situ within the quartz polished sections by using the UCLA CAMECA ims 1270 ion microprobe. Samples were coated with ~ 350 Å of gold. The ~0.1–0.4 nA primary
Cs
+ beam was shaped into a spot ~ 8–10 m m in diameter (usually in aperture illumination mode). Charge compensation was achieved using a normal-incidence electron fl ood gun (Slodzian, 1980). Low-energy (~0–30 eV) negative secondary ions were measured at high-mass resolving power (M/ D M) of about 6500. Measurements were made by magnetic peak switching through 25 cycles of counting
16
O
- for 3s, and
18
O
- for 5s. The secondary
16
O
- current was measured in a Faraday cup equipped with a Keithley 642 electrometer, and
18
O
- signals were pulse-counted on an electron multiplier with a deadtime of typical 20 ns. The analysis conditions typically yielded equivalent count rates of 20–40 million counts per second of
16
O
-
. Measured secondary ion intensities were corrected for background (
16
O
-
), and for deadtime (
18
O
-
). With the count rates employed in these experiments, the total magnitude of these corrections is small (<2‰), and thus the additional uncertainties resulting from background and deadtime corrections are negligible (<0.1‰). Zircon was used as a standard ( d
18 O = 18.4 ‰) to correct for instrumental mass fractionation. Isotopic data are reported in standard d notation relative to Vienna SMOW.
The d D values for sericite were measured on a continuous-flow gas-ratio mass spectrometer (ThermoQuest Finnigan Delta PlusXL) in the Environment Isotope
Laboratory at The University of Arizona. Samples were combusted at 1400°C using
46 the Thermal Combustion Elemental Analyzer (TCEA) coupled to the mass spectrometer. Standardization is based on NIST SRM 8540. Precision (1 s ) is better than ± 2.5 per mil on the basis of repeated internal standards. Isotopic data are reported in standard d D notation relative to Vienna SMOW.
4.2.3 Analytical Results
The range of d
18 O values for vein quartz samples collected and analyzed during this study is 14.1 to 16.1 per mil, except for one sample whose value is 25.2 per mil. This erratic value is interpreted to come from silica formed by weathering of aluminosilicate minerals, or the sample was contaminated during its preparation. d
18 O quartz values are very uniform in most of the samples (Table 4.2). This uniformity implies a very uniform temperature distribution and source of ore fluids, throughout the history of mineralization, regardless of their color, shape, thickness, attitude, mineralogical association, crosscutting relationships, and depth in the deposit. The quartz was in equilibrium with the ore fluids of between 8.2 and 10.2 per mil, using the quartz-water fractionation equation from Clayton et al. (1972) and assuming vein formation at 330°C, the temperature obtained from sulfur isotopes, although the actual temperature for ore deposition might be slightly higher or lower.
For sericite, the measured d D range is -109 to -57 per mil, but most values are between -76 and -61 per mil (Table 4.2). Extrapolation of water-muscovite fractionations factors (Suzuoki and Epstein, 1976) indicates about 41 ‰ fractionation at 330°C. This fractionation yields d D values for ore fluids between -65 and -15 per mil, with most values falling in a narrower interval of -34 to -19 per mil.
47
Table 4.2. Oxygen and Hydrogen Isotope data from La Herradura Gold Deposit.
Sample d
18 O quartz (‰ )
δ D sericite (‰) d 18 O ore fluids (‰)
1 d D ore fluids (‰)
2
478-2 15.9
10
478-4 15.7
-109 9.8
-67
478-5 25.2
19.3
530-1
530-2
530-3
531
525-1
525-2
528-1
528-3
532-2
533
HGT-14, 487.30m
HGT-14 488.70m
HGT-14, 541.40m
HGT-14, 541.40m
HGT-14, 570.10m
HGT-14, 570.35m
HGT-16 344.90m
15.3
14.2
14.1
14.5
14.4
14.6
15.4
14.9
14.3
16.1
-65
-57
-73
-62
-63
-61
-70
-71
-71
-58
-76
-75
-100
9.4
8.3
8.2
8.6
8.5
8.7
9.5
9
8.4
10.2
-23
-15
-31
-20
-21
-19
-28
-29
-29
-16
-34
-33
-58
15.5
9.6
HGT-17 651.90m
14.5
-64 8.6
-22
LH-AE 15.6
9.7
1 The d
18 O values for ore-forming fluids were calculated from the quartz-water equilibrium equation of Clayton et al. (1972). 2 The d D for ore-forming fluids were calculated from the muscovite-water equilibrium fractionation factor of Suzuoki and
Epstein (1976). Temperature of deposition was obtained from fluid inclusions and sulfur isotopes, T =330°C.
4.3 Sulfur Isotopes
4.3.1 Sampling
Twenty-six sulfur isotope measurements on pyrite, sphalerite, and galena were obtained from 12 samples of quartz-sulfide veins, collected from diamond drill cores deep below the Centauro pit (Figure 4.3). All quartz-sulfide veins have sericitic
48 alteration haloes and are hosted in quartz-feldspar gneiss. Individual grains of pyrite, galena, and sphalerite were hand-separated. The first suite of samples consisted of ten sulfide species that were used for determining the source of the sulfur in the deposit.
Later, a second suite of samples was sent to the laboratory in order to use mineral pairs for the estimation of the temperature of deposition of the sulfides and gold mineralization (Figure 4.4) and compare those with the temperatures obtained from fluid inclusions.
Figure 4.3 Map of the La Herradura mine, showing location of samples used for Sulfur
Isotopes. Coordinate system is UTM, NAD27.
49
Py gold
Figure 4.4. Reflected light microphotograph, showing pyrite with strong fracturing and later gold mineralization in the fractures. The sample corresponds to DDH HGT-13, 367m. The Au assay in this area is 40 g/t gold.
4.3.2 Analytical Methods
Values of d
34 S of different sulfides were measured on a continuous flow gasratio mass spectrometer (Finnigan Delta PlusXL). Samples were combusted at 1030
°C with V
2
O
5
using an elemental analyzer (Costech) coupled to the mass spectrometer. Standardization is based on international standards OGS-1 and NBS123 and several other sulfide minerals that have been compared between laboratories.
Calibration is linear in the range -10 to +30 per mil. Precision is estimated to be ±
0.15 ‰ or better (1 σ ), based on repeated internal standards. Isotopic data are reported in standard d
34 S notation relative to Canyon Diablo Troilite (CDT).
50
4.3.3 Analytical Results
Sulfur isotopic data for 26 sulfide samples are summarized in Table 4.3. The d
34 S values of sulfides fall in a narrow range between 3.1 and 6.6 per mil. Individual species show a narrower range of d
34 S, pyrite from 4.7 to 6.7 per mil, sphalerite from
4.8 to 5.6 per mil, and galena from 3.4 to 3.9 per mil. There is no systematic variation of isotope values with depth (Fig.4.5, Table 4.3). The d
34 S of pyrite ≥ d
34 S of sphalerite > d
34 S of galena, consistent with the order of equilibrium fractionation among these minerals (Bachinski, 1969).
4.3.4 Sulfur Isotope Geothermometry
The isotopic compositions obtained from coexisting sulfide species were used as a geothermometer, assuming that they have achieved isotopic equilibrium. Ohmoto and Lasaga (1982) demonstrated that at temperatures above 300°C, sulfides species can achieve isotopic equilibrium. The pyrite-galena pair, as the most sensitive geothermometer (Ohmoto and Rye, 1979), was chosen to estimate the temperature of formation of quartz-sulfide veins and deposition of related gold mineralization.
Temperatures were calculated using equations in Campbell and Larson (1998). The calculated temperature for deposition of sulfides in samples HGT-13-401.20 and
HGT-17-655.85 range between 319 to 343°C, with an average temperature of 330
±20°C (Table 4.3). For sample HGT-13-755.45, however, some disequilibrium is expected because the calculated average temperature is 407°C. Also, by using the pyrite-sphalerite mineral pair, the calculated temperature for sample HGT-13-643.30 the average temperature is 343°C.
51
Pyrite-galena values give the most precise temperature estimates. The temperatures obtained from samples HGT-13-401.20 and HGT-17-655.85 (328, 330,
342 and 319°C), whose average is 330 ±20°C, and is in agreement with temperatures obtained from fluid inclusions (275 to 285°C) in the same type of quartz veins.
52
Table 4.3. S isotope database and calculated temperatures for deposition of sulfides.
Temperature deposition calculated from Campbell and Larson (1998).
Sample Vein morphology mineral d
34
S (‰) T (°C)
HGT-14,487.30m
vein py 5.3
HGT-14,488.70m
HGT-14,488.70m
HGT-14,541.40m
vein vein py sp py
5.6
5.2
4.7
HGT-14,570.10m
HGT-17,651.90m
vein vein
HGT-17,655.15m
HGT-17,655.85m
HGT-13,367.20m
HGT-13,401.20m
HGT-13,401.20m
HGT-13,643.30m
HGT-13,643.30m
HGT-13,757.45m
HGT-13,757.45m
HGT-17,655.85m
HGT-13,655.85m
vein vein brecciated vein brecciated vein brecciated vein vein vein vein vein vein vein py
Sp
Py
Gn
Py
Gn
Py
Gn
Py
Gn
Py
Gn
Py gn py sp
Gn sp py py
Gn
Py
Sp
6.4
5.6
6.1
3.9
6.2
3.9
5.8
3.1
6.0
3.1
6.6
3.7
6.6
3.4
5.7
5.3
3.6
4.8
6.2
5.7
3.7
6.4
5.6
328
330
354
333
417
398
343
319
53
Figure 4.5. Plot of d
34 S Vs elevation. Values for individual species are clustering. Arrow shows decreasing isotopic values from pyrite to sphalerite to galena. It implies that sulfide species may have achieved isotopic equilibrium.
4.4 Carbon Isotopes
4.4.1 Sampling
Isotopic and carbon content measurements were carried out on ankerite crystals and on quartz veins, which contains CO
2
-bearing fluid inclusions. Three ankerite samples were collected from outcrops in the Centauro pit and from the outer part of the deposit (Figure 4.6). Quartz veins were collected from outcrops within the
Centauro pit and from diamond drill cores deep below the Centauro pit. All quartzsulfide veins have sericitic alteration haloes and are hosted in quartz-feldspar gneiss.
100 mg of each sample was hand-separated and then finely crushed by using a mortar and pestle.
54
Figure 4.6. Location of samples used for Carbon isotopes. UTM, NAD27
4.4.2. Analytical Methods d
13 C and carbon content were measured on a continuous continuous-flow gasratio mass spectrometer (Finnigan Delta PlusXL) coupled to an elemental analyzer
Costech). Samples were combusted in the elemental analyzer. Standardization is based on acetanilide for elemental concentration, NBS-22 and USGS-24 for d
13 C. Precision is better than ± 0.09 ‰, based on repeated internal standards.
55
4.4.3 Analytical Results
Carbon content and carbon isotopic data for all samples are summarized in
Table 4.4 and presented as a plot of d
13 C versus 1/concentration of C in figure 4.7.
Carbon contents are based accurately on chromatogram peak areas, except for sample
14-488, whose carbon content is approximated from peak heights. The end members are fluid inclusion-bearing quartz and ankerite, which have approximately fixed compositions. Any mixing trend will appear as a straight line connecting the two end members. Some quartz yielded very little C concentrations, suggesting a strong influence of CO
2
from fluid inclusions. Some quartz yielded a relatively large amount of C (sample 17-651). Concentrations and isotopes are consistent with the presence of some carbonate mineral. One sample is intermediate, lying near the straight line between the two end members. These data suggest that there are two sources of C, one associated with carbonate minerals, d
13 C=0 to -6‰, and one associated with fluid inclusions, d
13 C < -18‰. The low d
13 C carbon source is organic C.
56
Table 4.4. Carbon content and d
13 C values of fluid inclusion-bearing quartz and ankerite.
Sample %C % C corr 1 / %C d 13C ‰
528-FI
530-FI
13-643-FI
17-651-FI
14-488-FI
488-A
523-A
528-A
0.06
0.02
0.02
9.60
0.06
0.02
0.02
9.37
1.7
12.0
12.0
12.0
16.26
64.02
53.91
0.11
0.59
0.08
0.08
0.08
-8.1
-17.8
-18.4
-5.7
-6.4
-0.9
-1.6
-2.8
0
-2
-4
-6
-8
-10
-12
-14
-16
-18
-20
0 10 20 30
1 / %C
40 50 60 70
Quartz
Ankerite
Figure 4.7. Plot of d
13 C versus 1/ concentration of C.
57
4.5. Interpretation and Discussion
Together the calculated d
18 O and d D values from La Herradura gold deposit plot in the field of metamorphic waters from Taylor (1974) (Figure 4.6). These results indicate a deep crustal source for the ore fluids, most likely of metamorphic origin, and are consistent with derivation of fluids from metamorphic dehydration reactions or by exchange of meteoric water with aluminosilicate-metamorphic rock. The narrow range of d
18 O, 8.2 to 10.2 per mil for the ore fluids from La Herradura gold deposit, is typical for the estimated d
18 O values for ore fluids from orogenic gold deposits of all ages from Neoarchean to Cenozoic, with values between 6 to 11 per mil for the
Precambrian (McCuaig and Kerrich, 1998) and 7 to 13 per mil for the Phanerozoic
(Bierlein and Crowe, 2000).
The d
34 S values from sulfides fall in a narrow range between 3.1 and 6.6 per mil, consistent with a magmatic source for the sulfur. This magmatic source could be either a non-exposed igneous body or from igneous clasts in sedimentary protolith, that were devolatilized during metamorphic events. Carbon isotope data suggests sedimentary or metasedimentary origin of the carbon.
On the basis of stable isotopic data, there is no much evidence for variation in temperature and composition of ore fluids across the deposit or with the interpreted timing of vein formation. This indicates either that a very large volume of ore-forming fluid circulated at the same type of mineralization or that a large volume of rock was being subjected to a very uniform metamorphic facies. This scenario is similar to most of the Laverton gold province in Australia (Salier et al., 2005) and the OGD in
Eastern Andean Cordillera of Peru (Haeberlin, 2002).
58
0
- 40
Primary magmatic H
300-600°C
Metamorphic
- 80
- 120
M ete or ic
w at er s hydrothermal waters
- 160
Ka ol in ite
li ne
(w ea th er in g)
-10 0 10 20 30 d 18 O, ‰
Figure 4.8.
Plot of d D Vs d
18 O of water coexisting with gangue minerals at 330°C by using equation of Clayton et al. (1972).
59
CHAPTER 5. FLUID INCLUSION STUDY
5.1. Introduction
The main objectives of fluid inclusion studies on gold-rich and barren quartz veins in orogenic gold deposits are to estimate the chemical composition of the ore forming fluids, constrain the temperature and pressure at which these fluids were trapped, and define the P-T-V-X history of the vein-forming fluids. Most of the existing studies on fluid inclusions in orogenic gold deposits worldwide have documented aqueous and CO
2
-rich fluid inclusions with estimated homogenization temperatures at 300 ± 50°C and 1-3 kbar (Groves et al., 1998). However, there are also many important lower and higher temperature deposits (200 to 700°C) formed over a continuum of depths that range between 2-20 km and at pressures varying from
<1 to 6 ± 1 kbar (Barnicoat et al., 1991; Groves et al., 1998; Goldfarb et al., 2005).
The salinities of fluid inclusions generally vary between 3 to 12 equiv. wt percent
NaCl, independently of the depth of formation of the deposit and the ages of mineralization. The low salinity has been interpreted to account for the low basemetal concentrations of gold deposits in metamorphic belts (Goldfarb et al., 2005), however, there are notable exceptions with higher salinities observed at certain deposits, such as Muruntau (Graupner et al., 2001) and in the Abitibi subprovince
(Boullier et al., 1998), but these brine-bearing fluid inclusion generation postdates gold deposition.
The chemistry and origin of this type of ore fluid in northwest Sonora has not been studied in detail; however, some temperature and paleodepths have been obtained from several gold occurrences located in the trend of the Mojave-Sonora
60 megashear. Available studies include Albinson (1989), Silberman (1992), Perez et al.
(1996), Lang (2003), and Noriega (2006), which all report low salinity fluids (all <10 wt% NaCl), a highly variable presence of CO
2
, epithermal to mesothermal temperatures (~150 to ~340°C), and paleodepths between 1.5 to 7.0 km, mostly based on stratigraphic reconstruction and the chemical and physical properties of the ore fluid inclusion assemblage.
The objective of this study is to obtain information on temperature, pressure, and composition of the fluids that formed auriferous quartz veins and to compare these data with previous results published Phanerozoic orogenic gold deposits from
North America and Peru. The latter is included because information has been published recently for these deposits.
5.2. Sampling
A total of 40 samples of quartz veins were collected from outcrops and diamond drill core in and around the Centauro pit area. Nineteen samples were prepared as removable doubly-polished fluid inclusion sections of 100 to 150 microns in thickness and, twelve of them were selected for petrographic descriptions of fluid inclusions and microthermometry studies in order to determine P-T-X characteristics of the fluids (Figure 5.1 and Table 5.1). Sampling was mainly focused on thin, discontinuous, extensional quartz veins with sericite envelopes, where the best identifiable fluid inclusions are found. These veins are spatially related to larger shear quartz veins, localized along major structures that control the distribution of ore-grade mineral (Figure 5.2 and 5.3). Most veins show development of elongated quartz
61 crystals growing at high angle to the wall of the vein, suggesting growth under tension
(Figure 5.4). A few of them contain carbonate and iron oxides as a selvage on the quartz vein (Figure 5.5). All sampled veins were hosted by Proterozoic quartzfeldspar gneiss.
5.3. Analytical Method
Petrographic characteristics of fluid inclusions in 12 samples were examined in transmitted light using a Nikon binocular petrographic microscope. Seven samples were selected for thermometric analysis in order to determine P-T-X characteristics of the ore fluids. These studies were performed on 73 fluid inclusions hosted in quartz, using an SGE, Inc.-adapted USGS gas flow heating-freezing stage (Were et al., 1979).
The SGE stage has a precision of +0.1°C and +1.4°C at 0.0°C and 374°C, respectively, and horizontal thermal gradients are below 0.2°C/cm. The stage was calibrated using SYN FLINC synthetic fluid inclusions (Sterner and Bodnar, 1984).
62
Figure 5.1. Map of La Herradura mine showing locations of samples used for fluid inclusions petrography and microthermometry studies. UTM, Datum NAD27.
63
Table 5.1. Samples used for fluid inclusion petrography-microthermometry, La Herradura.
Sample Area East North MASL Description
LH-1
482-1
Megapit North 322107 3447864
Centauro Pit 322376 3447114
154
-16
Shear vein, white color (milky). 50 Cm width, no Fe-oxides.
yellowish-white quartz vein 1-2 m thickness, sigmoidal form.
The core is mainly quartz and scarse jarosite; at borders hematite in fractures, color is reddish black.
482-2
525
528
Centauro Pit 322376 3447114
Centauro Pit 322321 3447165
Centauro Pit 322276 3447114
-16
-65
-60
Quartz vein, light gray color, cut by sericite-hematite veinlets. Feoxides dissminated and fractures, derived from pyrite.
Quartz-carbonate extensional vein < 1 cm thickness, carbonates are like selvages. Subhorizontal vein. Host is Quartz feldspar gneiss, sericite-py alteration.
Quartz-Fe-oxide (Py)-Fe-carbonate (ankerite). Sericite alteration halo.
530
532
Centauro Pit 322259 3447089
Centauro Pit 322258 3447092
HGT-14-
488.70m
HGT-14
541.40m
HGT-14
570.10m
HGT-16
344.90m
Centauro Pit
East
Centauro Pit
East
322734 3447251
322724 3447243
Centauro Pit
East
322718 3447238
North of Dunas
Zone
321576 3447823
Coordinate system is UTM NAD27
-58
-35
Quartz crystals euhedral habit with hematite (after pyrite) disseminated and on fractures. Sericitic alteration halos.
Quartz-pyrite (now hematite) vein, 2 cm thickness, white color,low-dipping. This zone corresponds to high-grade mineral
(2 g/t gold)
-318 Quartz-pyrite-sphalerite vein, 8 mm thickness, sericitic haloes.
-369
-397
-119
Quartz-pyrite vein, 13 mm thickness, sericite alteration haloes.
Host rock is quartz-feldspar gneiss.
Quartz-pyrite-sphalerite vein, irregular form, 2 cm thickness, sericitic alteration halo.
Light gray quartz veinlet, cut by siderite-ankerite. Drusic textures.
Figure 5.2. Photograph showing shear veins and associated flat extension veins (from
Rhys, 2005).
64
Sericite-pyrite envelope
Quartz vein
Figure 5.3. Photograph showing extensional quartz vein with sericite-pyrite
envelope. Centauro pit, bench -72.
Figure 5.4. Photomicrograph of extensional quartz veins. Note fibrous quartz crystals growing at high angles to the walls of the veins, which indicate growth under tension. El Centauro pit; full section view in crossed polars (from Lang,
2003).
65
Figure 5.5.
P hotograph showing quartz vein with carbonate and Fe oxides as a selvage. Note the strong sericite envelope.
5.4. Petrographic Characteristics of Fluid Inclusions.
Most of the studied samples contain quartz veins with deformational textures, commonly with crystals of quartz growing 120° to the hanging wall, suggesting that the quartz vein grew under tension (Lang, 2003). The fluid inclusions assemblages selected for microthermometry are located near the center of the veins, where the euhedral quartz crystals are less deformed and preserve the larger and best fluid inclusions to be studied. The shape of the fluid inclusions studied vary from irregular, elongate, ovoid and circular, with size ranging from 4 to 20 microns, averaging 8 microns in size. Most of the fluid inclusions studied were interpreted as primary according criteria of Shepherd et al. (1985). In the same way, there is a large group of secondary planes (fractures?), containing small and secondary fluid inclusions with sizes less than 1 micron. Only one type of fluid inclusion was observed (Figure. 5.6)
66 containing three phases (CO
2
-rich vapor, CO
2
-rich liquid and aqueous liquid), arranged concentrically. The CO
2
phase covers from 8 to 50 % of the inclusion area, but the vast majority fall in a narrower range of 15 to 30 %. No daughter minerals were seen.
Fluid (mainly water)
CO2 liquid
CO2 vapor
Figure 5.6. Photomicrograph showing fluid inclusions. The inclusion contain an
aqueous fluid, CO
2
liquid and CO
2
vapor. Sample HGT-14-488.70m. Plane polarized
light; inclusion is 20 m m long.
67
5.5. Analytical Results
Microthermometry data were collected from 54 fluid inclusions scattered in 7 samples, and is summarized in the Table 5.2. Freezing and heating analyses were focused on large groups of inclusions with constant liquid/CO
2
ratios, which were considered representative of most inclusions in a given sample. The temperatures obtained for each fluid inclusion were run at least ten times in order to assure the quality of the data obtained. Freezing runs were carried out before heating runs, because larger inclusions, independent of shape, were destroyed by decrepitation during heating runs. The principal observations are summarized below.
• The melting temperature of the CO
2
phase for all fluid inclusions was between
-56.6 and -56.9°C (Table 5.2). A pure CO
2
solid phase melts (triple point) melts at -56.6°C. The slightly more negative values indicates the presence of additional, but in this case very minor, gaseous components like CH
4
, N
2
, and others gases in the CO
2
bubble (Shepherd et al., 1985).
• Clathrate melting temperatures were measured on 45 fluid inclusions, with temperatures ranging from 6.5 to 8.5°C in nearly all cases, but mostly around
7.5 to 8.5°C (Fig. 5.7). Based on these temperatures, the salinities of fluid inclusions were estimated using the FLINCOR program (Brown, 1989), with values ranging from 3 to 6.6 equiv. wt % NaCl, although the vast majority fall in a range of 3.5 to 4.8 wt % NaCl (Table 5.2). These estimates agree with others estimated by using the equation of Bozzo et al. (1973), valid for clathrate melting temperatures between 10 and about 0°C, with salinities ranging from 0 to 16 equiv. wt % NaCl.
68
• Homogenization temperatures of the CO
2
vapor phase into the CO
2
liquid phase were measured in 54 fluid inclusions. The temperatures obtained range from 24.1 to 30.2 °C, with the majority occurring between 27 and 29 °C
(Figure 5.8).
• The final homogenization temperature of the CO
2
bubble into the aqueous liquid phase was obtained in 39 fluid inclusions. The measured temperatures range consistently between 245 and 295°C, but the majority are between 275 and 285°C (Figure 5.9). Many of the larger inclusions, independent of shape, but with higher volumes of CO
2
, decrepitated at temperatures around 240 and
270°C due to high internal pressure.
• Calculations of fluid compositions using the FLINCOR program (Brown,
1989), indicate fluids containing between 2.2 and 7.4 mol % CO
2
.
• Pressures (Table 5.2) were estimated for each sample using the melting temperature of clathrate, the homogenization temperature of the CO
2
vapor to liquid, the estimated volume fraction of CO
2
, and the final homogenization temperature obtained, using the methods outlined in Brown and Lamb (1989),
Bowers and Helgeson (1983), and the FLINCOR Program (Brown, 1989).
Isochores were plotted for each sample from its final homogenization temperature to 334°C (Fig. 5.10), and the equations of the “tendency line” were obtained from each one. The algebraic “average isochore” was obtained,
69 plotted and, then the “average tendency line” was obtained. The intersection of this isochore (average) with the average temperature from all the samples fixes the minimal P-T trapping (average) for fluid inclusions. The upper intersection of the “average isochore” with an independent geothermometer (Roedder and
Bodnar, 1980), in this case 330 ±20°C for deposition of sulfides obtained from sulfur isotopes, fixes the maximal P-T trapping for fluid inclusions. Based in the calculations outlined above and using the equation from Bowers and
Helgeson (1983), the trapping pressure of the fluid inclusions lies between 1.6 and 2.7 kbar (Figure 5.10). This corresponds to paleodepths of between 4.3 and 7.3 km, considering an average density of 2.7 g/cm 3 for the quartz feldspathic gneiss that hosts the mineralization in the La Herradura mine. The density for the host rock was obtained from thousands of measurements carried out by the Peñoles exploration team. The lower values for temperature and trapping pressure for sample HGT-16-344.90m compared to all other samples might reflect a decrease in the pressure regime related to episodic extension and opening of fractures during entrapment of these fluid inclusions.
All Data, n=45 fluid inclusions
16
14
12
10
11
13
15
8
6
5
4
2
1
0 0
0
5.8
6.3
6.8
7.3
7.8
8.3
8.8
Clathrate Melting Temperature (C)
Figure 5.7. Clathrate melting temperatures for all samples. The salinity of fluid inclusions can be estimated from these measurements (Bozzo et al., 1973).
All Data, n=54 fluid inclusions
20
18
16
14
12
19
14
10
8
6
9
7
4
3
2
1 1
0
24.5
25.5
26.5
27.5
28.5
29.5
30.5
CO
2
Homogenization Temperature (C)
Figure 5.8. Temperatures of homogenization for CO
2
(to liquid) for all samples.
70
71
All Data, n=39 fluid inclusions
12
10
8
8
10
9
6
5
4
3
2
2
1 1
0 0 0 0 0
0
242.5
247.5
252.5
257.5
262.5
267.5
272.5
277.5
282.5
287.5
292.5
297.5
302.5
Homogenization Temperature (C)
Figure 5.9. Final homogenization temperature for all samples. The results span a
remarkably narrow range in temperature, even though the samples come from across
the entire deposit as well as from depth beneath Centauro pit, with most results
between 265 and 285°C.
Calculated isochores for fluid inclusions
4000
3500
3000
2500
Range in trapping pressure
Steepest isochore
2000
1500
Maximum P-T
Shallowest isochore
1000
500
0
Average isochore
Average measured homogenization temperature (272.5°C)
Temperature (°C)
Independent geothermometer
(330°C, S isotopes)
100 120 140 160 180 200 220 240 260 280 300 320 340 360 380 400 420
Figure 5.10 Plot of maximum and minimum isochors for fluid inclusions. Intersection of homogenization temperature with the isochores establishes trapping pressure for fluid inclusions.
72
Table 5.2. Microthermometry summary.
Sample
482-1
Petrography
Size (nm)
7x5
Microthermometry of fluid inclusions *
Volume %
CO
2
CO2 melting
T
20 -56.6
Clathrate melting T
7.5
T CO2 homog (L)
28.7
Flincor program (Brown, 1989)
Brown and Lamb (1989)
Bowers & Helgeson,
1989
T filling mol % CO
2
Wt % NaCl CO
2
density Pressure (bars)
279.0
2.9
4.8
0.64
1684
482-2
528_1
530_1
HGT-14-488.7
HGT-14-570.1
HGT-16-344.9
10x5
5x8
10X8
6x5
11X20
10X4
20
25
30
20
15
50
-56.6
-56.7
-56.6
-56.6
-56.6
-56.6
7.9
8.1
8.2
8.1
7.9
8.25
28.6
27.3
27.6
27.9
27.4
29.9
282.6
265.5
274.0
265.0
271.0
279.2
2.9
3.8
4.5
3.0
2.3
6.8
4.1
3.7
3.5
3.7
4.1
3.5
* At least 10 measurements for each fluid inclusion. T is Celsius.
0.64
0.66
0.66
0.66
0.67
0.60
1770
1310
1232
1495
2015
670
5.6. Interpretation and Discussion
The results obtained in this study are very similar to those obtained from Lang
(2003). Petrographic studies indicate that the ore fluids were entrapped at the same time during the syn-deformational precipitation of the auriferous quartz veins, because higher values of gold correlates closely with extensional quartz-sulfide veins
(Figure 4.4). There is no significant variation of temperature or fluid composition in the deposit. This is in agreement with previous information obtained from stable isotopes. The uniformity in the characteristics of ore fluids implies that these fluids remained uniform and homogeneous over much of the vertical extent of the hydrothermal conduit.
On the basis of the depth of formation, the ore fluids, where fluid inclusions were collected, lie on the transition between epizonal and mesozonal classes (Groves et. al,
1998), corresponding to the greenschist metamorphic facies. Summarizing, ore fluids have the following characteristics:
• Mostly liquid-rich fluids.
73
• H
2
O-CO
2
composition (2.3 to 6.8 mol % CO
2
).
• A nearly pure CO
2
phase
• Low salinities, with values between 3.5 and 4.8 equiv. wt % NaCl.
• Final homogenization temperatures of the CO
2
bubble into the aqueous liquid phase range consistently between 245 to 295°C, but the majority are between
275 and 285°C (Figure 5-11).
• Trapping pressures between 1.6 and 2.7 kbar. This is equivalent to 4.3 to 7.3 km under a lithostatic pressure regime, lying in the transition between epizonal to mesozonal classes, in the greenschist metamorphic facies.
74
CHAPTER 6: DISCUSSION AND CONCLUSIONS
6.1. DISCUSSION
Mojave-Sonora Megashear
La Herradura mine occurs within a northwest trending belt that consists of metamorphic rocks of greenschist and amphibolite facies and granitoids of
Proterozoic age (Nourse et al., 2005). The most outstanding tectonic feature in northwestern Mexico is the controversial Mojave-Sonora megashear (MSM) that separates two different basement blocks. The Caborca block lies to the west and has basement ages ranging from 1.8 to 1.7 Ga. The North American block to the east has basement ages ranging between 1.7 and 1.6 Ga. The La Herradura gold deposit is located within the older basement, i.e., in the Caborca block, as is confirmed with the new ages obtained by using U-Pb isotopes in zircons from within intrusive rocks and the gneiss belt hosting the orebody. These new ages agree with those previously published for similar rocks from the Caborca block (Anderson and Silver, 2005).
Metavolcanic rocks outcropping to the north of La Herradura deposit yield ages of
167.8 ± 3.5 and 159 + 3.5, -3.7 Ma for rhyolite and andesite, respectively. These data are also in agreement with the characteristic Lower to Middle Jurassic ages in the
Caborca block. Moreover, on the basis of biostratigraphic studies, González et al.,
(2005) argued that the Late Permian-Early Jurassic El Antimonio Group, which is part of the Caborca Block, was originally positioned in southern Nevada and southeastern California, and later translated to its present location by MSM.
However, Boucot et al. (2008), from paleontological studies indicated a continuous
Devonian continental shelf along the entire southern margin of Laurentia that
75 contradicts the early Late-Jurassic Mojave-Sonora megashear as a viable hypothesis for large-magnitude offset of Proterozoic through Middle Jurassic rocks from
California to Sonora.
As an alternative hypothesis to the MSM, Nourse et al. (2005) suggest that the two sequences of Proterozoic rocks in the region are the result of
Paleoproterozoic accretion. No ultramafic rocks (which might expected along a suture) of this age have been reported in northwestern Sonora. However, little of the trace of the putative suture would be exposed, because of the development of later
Tertiary alluvial basins.
A different alternative for the large-scale structure could be a combination of the paleoproterozoic accretion proposed by Nourse et al., (2005), and its subsequent reactivation as a result of younger tectonic events. Reactivation of this structure might have occurred during the emplacement of granitoid intrusions related to the
Permo-Triassic magmatic arc of Mexico (stretching from Chihuahua to Chiapas) described by Torres et al., (1999). These authors report ages from 287 to 232 Ma, for the magmatic arc. A 233 Ma monzodiorite intrusion outcropping to the southwest of
Sonoyta (Campbell and Anderson, 2003) should be part of this magmatic arc, bridging the gap between the Permo-Triassic granitoid belt of México and the Late
Permian-Triassic (243 to 208 Ma) plutonic rocks of southern California (Barth et al.,
1997). In addition, González et al. (2005) reported 270-240 Ma zircon grains within the El Antimonio Group, an Upper Permian-Triassic and Lower Jurassic sedimentary succession in northwestern Sonora. It is also possible this magmatic arc supplied part or all of those Permian volcanic detritus reported for the Upper Triassic Chinle
Formation of the Colorado Plateau (Stewart et al., 1986).
76
Younger reactivations of the mega-structure would have occurred during subsequent tectonic events, like the Jurassic magmatic arc, the Late Cretaceous-Early
Tertiary Laramide orogeny and, the Mid-Tertiary Basin and Range extension.
However, the limited number of known Permo-Triassic intrusions in the area leaves room for doubts about these interpretations. Intrusions of this age are not reported for the North America plate. They could be an exclusive characteristic of the Caborca block; only detailed mapping and geochronology will cast further light on the discussion.
Association of gold and the Mojave-Sonora megashear
Regardless of the origin and the age, a large-scale structure is believed to play an important role in the distribution of gold deposits, displaying a northwestern belt from southern California to northwestern central Sonora. The belt includes the
Picacho mining district, La Choya, Quitovac, La Herradura, Tajitos, Cerro Colorado,
El Chanate, San Francisco and Lluvia de Oro, among other important gold prospects
(Figure 2 of Silberman and Giles, 1988). Most of these gold deposits occurs within or adjacent to a regional structure, hosted by Precambrian, Mesozoic, and Tertiary rocks
(Fig. 2 from Silberman and Giles, 1988). La Herradura is an outstanding example of this class of deposits hosted in Precambrian rocks, as well as La Choya for Mesozoic rocks, and Cerro Colorado for Tertiary rocks.
There are several geochemical analyses published from the gold occurrences located in northwest Sonora and Southern California (Silberman and Giles, 1988;
Durgin and Teran, 1996, and Losh et al., 2005). These data show that the structurally controlled Au deposits considered by Silberman and Giles (1988) have Au/Ag ratios
77 of 2/1 to 6/1. In Arizona, the Au/Ag ratios range between 1/44.5 to 1/88.9 (Titley,
1997). The contrasting Au/Ag ratios suggest different metallogenic provinces in terms of underlying basement sources of precious metals. The higher ratios are found on both sides of the MSM.
Origin of the fluids
The ore fluids leading that deposited the La Herradura orebody were most likely generated following the prograde metamorphism of the continental plate during the Laramide orogeny. This timing is consistent with the age obtained for mineralization from Re-Os isotopes, which is 61.0 ± 2.1 Ma. The change in plate motions, passing from a compressional to a transpressional regime, could have reactivated older healed large-scale structures, which permitted the ore fluids migrate upwards, until they reached the more favorable ductile-brittle transition, which permitted the precipitation of gold in second-order structures. This structural relationship has been observed in most OGD (Goldfarb et al., 1988, 1991, 2005;
Rushton et al., 1993; Haeberlin 2002; Haeberlin et al., 2003; 2004; Sillitoe and
Thompson, 2006). In the La Herradura deposit, first-order structures could correspond to the trace of the postulated MSM or to the boundary of accretion between paleoterranes proposed by Nourse et al. (2005). Second-order structures may correspond to thrust faults developed during Sevier and/or Laramide orogenies.
The gold mineralization in La Herradura gold deposit came after peak metamorphic conditions. In the Centauro pit, some mineralization is hosted in metamorphic pegmatites, which have a retrograde greenschist overprint. The petrographic studies of fluid inclusions indicate that the ore fluids were entrapped at
78 the same time as the syn-deformational precipitation of the auriferous quartz veins, because of the correlation of distribution of gold with quartz-sulfide veins (Figure
4.4).
The calculated d
18 O and d D values from the La Herradura ore fluids at 330
°C range mainly in a narrow interval between 8.2 to 10.2 per mil, and -34 to -19 per mil, respectively. These values indicate a deep crustal source for the ore fluids, most likely of metamorphic origin, and are consistent with derivation of fluids from metamorphic dehydration reactions or by exchange of meteoric water with aluminosilicate metamorphic rocks. The uniformity of d
18 O values also implies a very uniform source of fluids, normally being driven at orogen scale, and related to a single distal source, as has been documented for OGD hosted in the Superior and
Yilgarn cratons (Robert et al., 2005), and the OGD in Eastern Andean Cordillera of
Peru (Haeberlin, 2002).
The high radiogenic initial ratios of 187 Os/ 188 Os (0.3578) rules out mantle and oceanic sources, at least for the gold-associated pyrite. Therefore, source must be continental crust. In the same way, carbon in fluid inclusions is of organic origin implying a sedimentary or metasedimentary origin for the carbon. This fact discards an igneous source for the carbon.
The uniformity of d
34 S (3.1 and 6.6 per mil) suggest no partial reduction of sulfate. These values indicate that the sulfur source was isotopically uniform and derived directly from the mantle, from magmas, or indirectly from dissolution and/or desulfidation of primary sulfide minerals of average crustal sulfur isotopic composition (Hagemann and Cassidy; 2000). For La Herradura, the source of sulfur is
79 either a non-exposed igneous body or igneous clasts in sedimentary protolith that were devolatilized during metamorphic events.
Drawing all isotopic data from La Herradura deposit, the fluids probably originated in Au-enriched metasediments, containing organic C. The gold, sulfides, and other metals, are removed from a previously gold-enriched rock.
Pressure-temperature (P-T) gradients of regional metamorphism drive gold mobilization and desulfidation reactions from amphibolite or higher grade rocks, into lower-grade rocks. Under amphibolites facies, pyrite breaks down to pyrrhotite ± Feoxides ± Fe-silicates at amphibolite facies temperatures (Thompson, 1972; Connolly and Cesare, 1993), which produces HS ligands for selective complexing of gold. The fluids transport gold as Au-S complexes, either Au (HS)
2
- or HAu(HS)
2.
Base metal transport is restricted to the low Cl contents, because brines in paleobasins did not survive to greenschist or higher metamorphic facies.
Causes of ore deposition
Several generations of fluids were generated during episodic fracturing during
Laramide time, probably as a response to the fluctuations in lithostatic-hydrostatic pressure. Fluids migrate through large-scale structures to shallower levels, until they reach the brittle-ductile transition, where permeable rocks improve movement of fluids, thereby pressure and temperature decrease and some gold precipitates, as is the case for the gold in extensional veins. However, the precipitation of gold is mainly driven by changes in the pH of the ore fluids, as a result of chemical reactions between ore fluids and wall rock, as is evidenced by the alteration of feldspar to sericite. Also, the high Fe/Fe + Mg ratios of wall rock promote the deposition of gold.
80
In La Herradura, the deposition of gold is favored for the higher Fe/Fe + Mg ratios in the granitoids within the Caborca block, compared to the granitoids within the North
American block. Iriondo (2001) published Fe/Fe + Mg ratios ranging from 0.85 to
0.89 for granitoids within the Caborca block, and 0.72 to 0.82 for those located within the North America blocks. The precipitation of early pyrite, galena and sphalerite reduce the sulfur activity of the ore-forming fluids in the early mineralization stages.
This change promotes gold deposition by destabilization the gold bisulfide complex
(Henley and Brown, 1985). Later, as the hydrothermal system evolved, precipitation of gold continues in the shift of the fluids, from a slightly acid-near neutral to a slightly higher pH, into a more oxidized ore-fluid that favored the precipitation of gold accompanied by hematite. Subsequent stages in the evolution of fluids precipitated iron and magnesium carbonates in the periphery of the deposit.
Based on fluid inclusion and stable isotopic studies, there is no evidence of variations in temperature and composition, except for C isotopes, for the ore fluids across the deposit or with interpreted timing of vein formation. The isotopic uniformity of quartz veins implies that isotopic values of ore-forming fluids remained uniform and homogeneous over much of the vertical extent of the hydrothermal conduit.
Comparison of La Herradura ore fluids versus OGD in North America and Peru
The geochemistry of the ore-forming fluids from La Herradura compares well with those from OGD described in North America and Peru. The calculated d
18 O and d D for the ore-forming fluids, combined with the temperature of formation of veins
81 and deposition of gold mineralization, overlap with the isotopic data field from other orogenic gold deposits from North America and Peru (Figure 6.1). In the Juneau gold belt, Goldfarb et al. (1991) estimated d
18 O and d D values for the ore fluids between
7.2 to 12.8 and -25 to -15 per mil, respectively, for a vein hosted in late Paleozoic (?) through Cretaceous metasedimentary ( ± metavolcanic) sequences. In the Carson and
Counterville deposits from the Mother Lode, California, Jia et al. (2003) reported d
18 O and d D values between 9 to 12 and -20 to -15 per mil, respectively, for the ore fluids involved in the formation of quartz vein hosted in Paleozoic-Mesozoic metasedimentary, volcanic, and ultramafic rocks. Also Jia et al. (2003) published d
18 O and d D calculated values between 7 to 8 and -130 to -120 per mil, respectively, for the quartz veins hosted in mid-Paleozoic to early Mesozoic metasedimentary and igneous rocks in the Sheba district, in the Klondike, Yukon Territory. The low δ D
H2O values reflect secondary exchange between recrystallizing mica and meteoric waters.
Leitch et al. (1991) reported calculated d
18 O between 10 to 14 per mil for the
Bralorne and Pioneer mesothermal veins in Bridge River, southern British Columbia, and Maheux (1989) published d D calculated values between -38 ±18 per mil for antimony-associated gold mineralization in the Bridge River district, British
Columbia, Canada. These veins are hosted in Permian (?) to Jurassic metavolcanics and metasedimentary rocks. Haeberlin (2002) obtained d
18 O and d D calculated values between 8.2 to 10.2 and -130 to -120 per mil, respectively, for the ore fluids involved in the Carboniferous orogenic gold deposits in the Pataz gold province, Peru.
These deposits are hosted in Paleozoic intrusions and in volcanic and sedimentary rocks.
82
From fluid inclusion study, the more common characteristics are the chemistry of the fluids (Table 6.2), these characteristics include low salinities, the presence of
CO
2
, which in individual deposits can be variable (Goldfarb et al., 1998), dependant in the depth and pressure of trapping for fluid inclusions. Another very important shared feature is the temperature of homogenization for fluid inclusions, mostly on the order of 200 to 350°C, which means that the ore fluids were trapped in the greenschist metamorphic grade host rocks, with pressures ranging from 1.2 to 2.3 kbar. In the Pataz gold province in Peru, however, the estimated pressure in the early stages was 4.5 kbar, and in the later evolution of fluids, these were moving to smaller pressures in response to a tectonic uplift (Haeberlin, 2002).
Based in the tectonic and structural setting, the geometry and style of mineralization, the chemistry and the origin of the ore fluids involved in La Herradura gold deposit, it is conclusive that this deposit corresponds to an orogenic gold deposit type, the first OGD described in the northwestern Mexico.
83
Table 6.1 Oxygen and Hydrogen Compositions of Quartz and Quartz-Carbonate veins in the Western North American Cordillera and
Counterparts Worldwide (modified from Jia et al., 2003).
Gold Province/
District
Juneau Gold Belt
Vein location
Juneau d
18 O quartz (‰) d D sericite(‰)
15.2 to 20.8
-75 to -53
T (°C)
300 d 18 O ore fluids
(‰)
1 d D ore fluids (‰)
2
7.2 to 12.8
-35 to -15
References
1
Mother Gold, California -20 to -15 2
Klondike, Yukon Territory
Carson and Coulterville
Oro Rico and McAlpine
Sheba
16.5 to 18.6
15.0 to 17.5
14.6 to 15.1
14.7 to 15.1
300
323 ±18
9 to 12
6 to 11
7 to 8
8.9 ±0.6
-130 to -120
6
1
3
Bridge River, southern BC Pioneer 17.8 to 18.1
11 to 12 -15 1
Tasman orogenic belt
Bendigo, Australia
Birimian greenstone belt
Ashanti, west Africa
Superior Province of Canada
Abitibi belt
Yilgarn Craton, W. Australia
Norseman-Wiluna belt
Eastern Andean Cordillera,
Perú
Bralorne and Pioneer
Central and North
Deborah
Ashanti gold field
Hollinger-McIntype,
Dome
Kalgoorlie and Norseman
Pataz-Marañon Valley Au belt
17.1 to 19.4
14.4 to 17.2
12.8 to 15.6
12.5 to 15.0
11.4 to 13.4
10.9 to 14.2
-60 to -39
230 ~ 350
350 ±25
400 ±50
220 ~ 450
220 ~ 500
330
10 to 13
8 to 11
9 to 12
6 to 11
5 to 9
-38 ±18
-37 to -17
-53 to -37
-80 to -20
-40 to -10
4,5
7
8
9
10
6.2 to 8.6
-19 to -40 11
1
La Herradura, Mexico Centauro Pit 14.1 to 16.1
-109 to -57 330
8.2 to 10.2
The d
18 O values for vein-forming fluids were calculated from quartz-water equilibrium equation of Clayton et al. (1972)
-19 to -34
2 The d D for vein-forming fluids were calculated from muscovite-water equilibrium fractionation factor of Suzuoki and Epstein (1976)
12
References: 1 = Goldfarb et al. (1991), 2 = Jia et al., 2003, 3 = Rushton et al. (1993), 4 = Leitch et al. (1991), 5 = Maheux (1989), 6 = Weir and
Kerrick (1987), 7 = Jia et al. (2001), 8 = Oberthür et al. (1996), 9 = Kerrich (1987), 10 = Golding et al. (1989), 11 = Haeberlin (2002), 12 = this study.
84
Figure 6.1. Plot of d D Vs d
18 O of water coexisting with gangue minerals. Data from selected orogenic gold deposits from North America and Perú, compared to La Herradura gold deposit.
Table 6.2. Comparison of fluid inclusions results from La Herradura with orogenic gold deposits located in the circum-Pacific of North and South America.
Deposit Temp °C
Salinity wt% NaCl
CO2 mol%
Pressure (Kbar) Source
Juneau Gold Belt, SE
Alaska
200-325 <5 wt% >50% 1.5
Goldfarb et al.(1988)
Weir and Kerrick (1987) Mother Gold, California 250-325
Klondike in Yukon,
Canada (Sheba)
Bridge River, British
Columbia, Canada
Pataz-Marañon, Peru
323 +- 18
230~350
140 - 330
2
4.3 ±1.5
<5
1 to 8
<10
5.8-7.9
5-15 low
<2 Kb
.3 - .9 to 2.3
±.7
1.75
2.1-4.5
Rushton et al. (1993)
Leitch et al. (1991) and
Maheux (1989)
Haeberlin (2002)
245-295 3.5-4.8
2.3-6.8
1.6-2.7
This study La Herradura
85
6.2. CONCLUSIONS
The La Herradura mine is located in northwestern Sonora Mexico. It occurs within a northwest trending belt of metamorphic rocks of greenschist and amphibolite facies, and granitoids, of Proterozoic age. The deposit is hosted preferentially in the more competent quartz-feldspar gneiss, 1.75 Ga age. It is limited to the east and west for Victoria and
Ocotillo shear zones respectively; these shears exhibit a northwest trend, that are separating the Proterozoic structural block to the east from Jurassic clastic rocks and subvolcanic intrusions, and to the west by Upper Paleozoic limestone. Most of the gold mineralization occurs in thin quartz-sulfide (leached in outcrop) veins following en echelon tensional swarms. These veins are low-dipping (<30°) and are interconnected to a thicker set of fault-fill higher-grade quartz vein systems, that are believed to be the feeders for gold mineralization in the entire deposit.
Stable isotope data indicate that ore fluids have a metamorphic origin, probably derived from a deep crustal source as a result of regional metamorphic dehydration reactions of the continental plate, following a prograde metamorphism during Laramide
Orogeny The calculated temperature deposition of sulfides accompanying gold mineralization is 330 ±20°C. Fluid inclusion studies in quartz-sulfides-gold bearing veins show that the ore fluids are CO
2
-rich, low in salinity, and have homogenization temperatures between 285-295 °C, and a calculated trapping pressure between 1.6 and
2.7 Kbar.
86
The age obtained from Re-Os isotopes on pyrite and magnetite-gold associated is
61.0 ± 2.1 Ma. This is the first age obtained on mineralization for this type of deposits in
Mexico.
The style and geometry of mineralization, stable isotopes and fluid inclusions studies, indicate that La Herradura gold deposit can be classified as an orogenic gold-type deposit, the first OGD described in northwest Mexico.
87
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