Activity 6/ Write 5 GY 402 Sedimentary Petrology (W) Paper Critical Review 2 Introduction: Time for another critical paper review, this one dealing with a more complex sedimentological study. The subject for today is provenance; the origin of sediment and what it can tell you about paleotectonic setting(s). Enjoy! 1) Discussion component (Activity 6): As we did for the previous critical review exercise, I want you to actively participate in an open discussion concerning the merits of the attached paper. I will expect you to be able to identify the purpose of the paper, the quality of the data presented, the limitations of the author(s)'s interpretations and the quality of their writing. I am also interested in how you feel this paper relates to GY 402 AND whether or not you learned something from reading it. Did you like the paper or did it really suck? Why? At the start of the activity session, I would first like you to get into your groups and to spend the first 10 minutes coming up with a "collective opinion" about the paper you all read. After that, well it will be a free for all discussion about the journal article, beaches in general and if you so desire, life the universe and everything. The activity grade that you will receive will be based on your group's efforts (i.e., you will receive a single group grade for the activity). Sink or swim together! 2) Writing Component (Write 5): Unlike Activity 4 which required a review after the discussion session, this time I want your 1 page written critical review before the discussion. Use the same format that you did for the midterm question. This writing exercise is due at 12:00 noon Thursday (right after the end of the discussion) as it will also be used for a peer review exercise (Peer 2), that is due the next day. Journal of African Earth Sciences 85 (2013) 31–52 Contents lists available at SciVerse ScienceDirect Journal of African Earth Sciences journal homepage: www.elsevier.com/locate/jafrearsci Provenance, diagenesis, tectonic setting and reservoir quality of the sandstones of the Kareem Formation, Gulf of Suez, Egypt Samir M. Zaid Geology Department, Faculty of Sciences, Zagazig University, 44511 Zagazig, Egypt a r t i c l e i n f o Article history: Received 20 November 2011 Received in revised form 6 April 2013 Accepted 26 April 2013 Available online 11 May 2013 Keywords: Provenance Diagenesis Reservoir quality Kareem sandstones Gulf of Suez a b s t r a c t The Middle Miocene Kareem sandstones are important oil reservoirs in the southwestern part of the Gulf of Suez basin, Egypt. However, their diagenesis and provenance and their impact on reservoir quality, are virtually unknown. Samples from the Zeit Bay Oil Field, and the East Zeit Oil Field represent the Lower Kareem (Rahmi Member) and the Upper Kareem (Shagar Member), were studied using a combination of petrographic, mineralogical and geochemical techniques. The Lower Rahmi sandstones have an average framework composition of Q95F3.4R1.6, and 90% of the quartz grains are monocrystalline. By contrast, the Upper Shagar sandstones are only slightly less quartzose with an average framework composition of Q76F21R3 and 82% of the quartz grains are monocrystalline. The Kareem sandstones are mostly quartzarenite with subordinate subarkose and arkose. Petrographical and geochemical data of sandstones indicate that they were derived from granitic and metamorphic terrains as the main source rock with a subordinate quartzose recycled sedimentary rocks and deposited in a passive continental margin of a syn rift basin. The sandstones of the Kareem Formation show upward decrease in maturity. Petrographic study revealed that dolomite is the dominant cement and generally occurs as fine to medium rhombs pore occluding phase and locally as a grain replacive phase. Authigenic quartz occurs as small euhedral crystals, locally as large pyramidal crystals in the primary pores. Authigenic anhydrites typically occur as poikilotopic rhombs or elongate laths infilling pores but also as vein filling cement. The kaolinite is a by-product of feldspar leaching in the presence of acidic fluid produced during the maturation of organic matter in the adjacent Miocene rocks. Diagenetic features include compaction; dolomite, silica and anhydrite cementation with minor ironoxide, illite, kaolinite and pyrite cements; dissolution of feldspars, rock fragments. Silica dissolution, grain replacement and carbonate dissolution greatly enhance the petrophysical properties of many sandstone samples. Ó 2013 Elsevier Ltd. All rights reserved. 1. Introduction The Middle Miocene Kareem Formation is an important hydrocarbon bearing-reservoirs in the southwestern part of the Gulf of Suez including Zeit Bay Oil Field and East Zeit Oil Field (Hilaly and Darwish, 1986; Saudi, 1992; Darwish and El-Araby, 1993; Alsharhan and Salah, 1995; Zahran, 2005; Fig. 1). The Middle Miocene Kareem sandstones served as one of the primary source of oil and gas, while the Middle Miocene evaporites (Belayim Formation) represent the excellent capping rocks for these reservoirs. Almost 23% of the oil is produced from the sandstones of the Kareem Formation (Alsharhan and Salah, 1997). In the Gulf of Suez area, the Miocene rocks have wide geographic distribution, either exposed or subsurface. Provenance studies of clastic sedimentary rocks often aim to reveal the composition and geological evolution of the sediment E-mail address: samir_zaid75@yahoo.com 1464-343X/$ - see front matter Ó 2013 Elsevier Ltd. All rights reserved. http://dx.doi.org/10.1016/j.jafrearsci.2013.04.010 source areas and to constrain the tectonic setting of the depositional basin. Previous works have revealed that the chemical composition of clastic sediments is a function of a complex interplay of several variables, including the source rock composition, the extent of weathering, transportation and diagenesis (Taylor and McLennan, 1985; Bhatia and Crook, 1986). However, the tectonic setting of the sedimentary basin may play a predominant part over other factors, because different tectonic settings can provide different kinds of source materials with variable chemical signatures (Pettijohn et al., 1987; Bhatia, 1983; Chamley, 1990; Armstrong-Altrin and Verma, 2005). Many attempts have been made to refine provenance models using the framework composition (Suttner et al., 1981; Dickinson et al., 1983; Weltje et al., 1998) and geochemical features (Bhatia, 1983; Suttner and Dutta, 1986; Roser and Korsch, 1986, 1988; Armstrong-Altrin et al., 2004). Significant contributions have been made by several studies in relation to the regional geology, petroleum prospects, sedimentology and tectonic evolution of the Kareem Formation including the 32 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 Fig. 1. Location map of studied wells, Gulf of Suez, Egypt. EGPC Stratigraphic Committee (1964), Hilaly and Darwish (1986), Darwish and El-Araby (1993), Salah (1994), Alsharhan and Salah (1994, 1995) and Salem et al. (2000). However, very few studies have ever been related to reservoir properties, diagenesis and its implications for reservoir quality except Alsharhan and Salah (1997) and Zahran (2005). In this regard, there still exists a gab between the understanding the reservoir properties and factors controlling the reservoir quality of Kareem sandstones. With the main of helping to close the gab, this paper gives an account of the petrophysical properties of reservoir rock to characterize the reservoir and also describes how the diagenetic aspects, petrophysical parameters and detrital composition influence the reservoir quality. The stratigraphic columns of Zeit Bay Oil Field and East Zeit Oil Field include the rock units from Paleozoic to Post Miocene normally encountered in the Gulf of Suez (Fig. 2). The Miocene sequences were previously subdivided by the EGPC Stratigraphic Committee and Subcommittee (of 1964 and 1974, respectively) into two main groups, the Gharandal and Ras Malaab. The term ‘‘Gharandal’’ was introduced by Said (1962) to describe the strata that lie beneath the Miocene evaporites on the Sinai side of the Gulf of Suez. The rocks were divided into two formations: the Nukhul and the Rudies. The term ‘‘Ras Malaab’’ was first introduced to describe surface exposures at the entrance to Wadi Gharandal. As the name ‘‘Gharandal’’ was already reserved for the underlying clastic group, the closest geographic name, ‘‘Ras Malaab,’’ was chosen for this group (EGPC, 1964). This group was redefined and subdivided by the EGPC (1974) into the Zeit, South Gharib, Belayim, and Kareem formations, in descending order. The Kareem Formation disconformably overlies the Rudies Formation and unconformably overlies by the Belayim Formation. The average thickness of the Kareem Formation is around 165 m. The Kareem Formation is composed mainly of interbedded sandstones, shales and carbonates with minor anhydrites in its lower parts. The sandstones of the Kareem Formation is medium to dark greenish grey, brownish grey, argillaceous and fossiliferous. The siliciclastics were deposited in alluvial and submarine fans building out from the rift shoulder, while the carbonates and anhydrites were precipitated in local lagoons as a result of sea level fluctuations. The formation is divided into the Rahmi and overlying Shagar members, and is Langhian to Serravalian in age (Alsharhan and Salah, 1997). S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 33 Fig. 2. Stratigraphic succession of the Gulf of Suez with correlated lithostratigraphic columns of East Zeit and Zeit Bay wells (Darwish and El-Araby (1993) and Zahran (2005) after modifications and additions). Rahmi Member consists of interbedded shales, sandstones and four beds of anhydrite with very thin beds of carbonate. The sandstones are yellow to yellowish-white in color. Rahmi Member is also referred to informally in the oil industry as the ‘‘Markha Member’’. Shagar Member consists mainly of interbedded shales and carbonates with thin laminae of sandstone and siltstone (Tewfik et al., 1992). The member unconformably overlies the Rahmi Member, and lies below the evaporites of the Belayim Formation (Youssef, 1986). 2. Geological setting The study area is located within the main structural units in the Gulf of Suez region (Fig. 1). The Gulf of Suez is a rift graben formed as a result of tectonic movements initiated in the Oligocene which continued with intensity until Post-Miocene times. Tensional faults of considerable displacements determine the configuration of the graben and its boundaries. According to Said (1990), the Gulf of Suez is divided into three uplifted belts separated by two structural lows (Fig. 1). The highs and lows are of Gulf parallel trend and dissected by NE–SW Aqaba trending faults. Five major tectonic episodes have been recorded in the Gulf of Suez. These, from base to top, the pan-African event, the Hercynian event, the Neo-Tethyan event, the Syrian Arc event and the Gulf of Suez event. The stratigraphic sequence in the Gulf of Suez (Fig. 2) comprises three stages; pre-rift, syn-rift and post rift stratigraphy. During the post rift stage, a rapid subsidence from the early Miocene to the Recent within the central depression of the rift has allowed for accumulation of up to 5 km of continental and marine sediments. Sedimentation is primarily governed by block structures with a thick series of clastics and evaporites in the grabens and erosion or carbonate buildup on the crests of the titled blocks. At the end of the Aquitanian there was renewed tectonic activity in the Gulf of Suez which included uplift of the rift shoulders and rapid subsidence of central trough (Zahran, 2005). The major structural blocks of the Gulf of the Suez region were delineated and tilted at that time leading to the erosion of Nukhul sediments of the structure highs. This subsidence and fragmentation of a rift during the Burdigalian resulted in increased clastic influx to the basin (Rudies Formation). There was a general marine transgression within the rift and deeper parts of the basin accumulated a thick sequence of shales and carbonates. Rapid subsidence, accompanied by the deposition of mixed carbonates, clastics and evaporites (Kareem Formation) continued through the Serravalian. The Kareem Formation consists mainly of the Rahmi lagoonal facies overlain by the Shagar Member generally along the shores of the present Gulf, the distribution of the anhydrites follows the Kareem shoreline (Tewfik et al., 1992). The sediment thickness within the Kareem Formation ranges from 400 to 1400 feet. The predominantly marine Rudies and Kareem formations together with the Nukhul Formation make up the Gharandal Group which is sometimes given a name of ‘‘Globigerina Marls’’. From Mid Serravalian to the Latest Messinian, the Gulf of Suez and Red Sea rift was restricted from the open ocean and underwent almost continuous evaporite deposition in the subsiding basin, resulting in the accumulation of up to 3 km of shallow, subaqueous, marine evaporitive carbonates, anhydrite, clastics and halite which forming Belayim, South Gharib and Zeit formations. This entire sequence forms the Ras Malaab Group. S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 SR–R P SR–R P SA–R P SR–WR P SA–R P SA–R P SA–R P SA–R P SA–R P SA–SR P SA–SR F>P SR–R P SR–R P SR–R P SR–R P SA–SR P SA–SR P SA–SR P Grain roundness Grain contact 2809 SR–WR P R–WR P SR–R P SR–WR F>P EZ20 9 M–C Ms 2805 2784 EZ19 8 F–M Ms EZ18 8 F–M Ms 2782 2780 EZ17 8 F–M Ps Ms SR–WR P EZ16 7 F–M Ps Ms SA–R P>C 2779 2760 EZ15 7 F–M Ms EZ14 6 M–VC M–Ps 2756 2744 EZ13 6 M–VC M–Ps EZ12 5 M–C Ms 2741 2734 EZ11 5 M–C Ps EZ10 4 M–C Ps 2733 Lower Kareem (Rahmi Member) at East Zeit Bay Field EZ9 4 F–C Ps ZB17 9 M–C Ps ZB16 8 M–C Ps ZB15 8 M–C M–Ps ZB14 7 M–C Ms ZB13 7 F–M Ms ZB12 6 F–M Ms ZB11 6 F–M Ms ZB10 5 F–M Ms ZB9 5 F–M Ms ZB8 4 F–M M–Ps ZB7 4 M–C M–Ps 1565 1561 1550 1547 1533 Lower Kareem (Rahmi Member) at Zeit Bay Field Textural data/depth Table 1 Textural data of the Lower Kareem Rahmi Member. 1577 1578 1580 4.1. Sandstone petrofacies and texture The Kareem Formation is composed of sandstones and less common shales and carbonates. The study deals with the petrographic characteristics of sandstones, and their diagenetic influences on reservoir quality. As the carbonates in the Kareem Formation do not constitute potential reservoirs in the southern Gulf of Suez, they have not been included in this study (Evans, 1990; Alsharhan and Salah, 1997). The analyzed sandstone samples of the Lower and Upper Kareem Formation are fine to coarse grained, subrounded to well rounded and moderate to poorly sorted (Tables 1 and 2). All types of major grain contact, including point, long, and concave–convex are present. However, an abundance of point contact was noted. The framework grains of the sandstones are composed of monocrystalline quartz (Qm), polycrystalline quartz (Qp), K-feldspar (K), plagioclase (Pl), and lithic fragments (LF). Quartz dominates over feldspar and lithic fragments (Tables 3 and 4). Sandstone classification was made using Dott–McBride scheme (Fig. 3). The sandstones of the Kareem Formation are mostly quartzarenite with subordinate subfeldspathic arenites (subarkoses) and feldspathic arenites (arkoses). Quartzarenites present in the Lower Kareem (Rahmi Member) where the subarkoses and arkoses recorded only in the Upper Kareem (Shagar Member). The Lower Kareem (Rahmi) sandstones have an average framework composition of Q95F3.4R1.6, Framework constituents comprise 80% of the rock, and the matrix and cement constitute about 20%. Matrix partly consists of clay minerals and detrital constituents. The observed type of cement includes ferroan and nonferroan dolomite and calcite, silica and anhydrite (Fig. 4). Average existing pore space constitutes 14% of the rock (Table 3, 1591 1582 4. Results Sample no. Core no. Av. grain size Grain sorting In this study we examined 152 m of 9 cores taken from a well in Zeit Bay Oil Field (depths of 1452–1604 m) and 188 m of 10 cores taken from a well in East Zeit Oil Field (depths of 2653– 2841 m), representing the Lower Kareem sandstones (Rahmi Member) and the Upper Kareem sandstones (Shagar Member). Thin sections prepared from 76 blue epoxy-impregnated samples were examined under the binocular microscope. The amounts of detrital components, as well as the textural modal grain size and sorting parameters, were determined by counting 300 points in each of 38 selected representative thin sections. Sorting was estimated by comparison with the standard charts of Beard and Weyl (1973). Carbonate cements were stained for identification with an acid solution of alizarin red and potassium ferrocyanide (Dickson, 1965). The morphology and the textural relationships between minerals were examined in 8 gold-coated samples by scanning electron microscope (SEM) equipped with energy-dispersive spectrometer (EDS), using an accelerating voltage of 10 kV. In order to identify the clay minerals present in the sandstones, X-ray diffraction analyses of the <2 lm fraction were performed for studied samples. Major element concentrations for fifteen selected samples were determined by X-ray Fluorescence (XRF) Spectrometry technique on fused beads (Rollinson, 1993). X-ray Fluorescence Spectrometry technique and SEM analyses were performed at the laboratory of the National Research Center of Egypt. Analytical precision is better than 3% for the major oxides. Loss on ignition (LOI) was estimated by firing the dried sample at 1000 °C for two hours. Moreover, the total iron is expressed as Fe2O3. EZ21 10 M–C Ms 2835 3. Sampling and methods 1531 34 35 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 Table 2 Textural data of the Upper Kareem Shagar Member. Textural data/depth Sample no. Core no. Av. Grain size Grain sorting Grain roundness Grain contact Upper Kareem (Shagar Member) at Zeit Bay Field Upper Kareem (Shagar Member) at East Zeit Bay Field 1463 1465 1470 1474 1520 1523 2666 2668 2678 2679 2680 2720 2722 2723 ZB1 1 F–C M–Ps SA–SR P ZB2 1 F–C Ps SA–SR P ZB3 2 M–C M–Ps SA–SR P ZB4 2 F–C Ms SR–R P ZB5 3 F–M Ms SR–R F>P ZB6 3 M–C Ms SR–R F EZ1 1 F–C Ps SA–SR P>F EZ2 1 F–C M–Ps SA–SR P>F EZ3 2 VF–C M–Ps SA–SR P EZ4 2 VF–C M–Ps SA–R P EZ5 2 VF–C M–Ps SA–R P EZ6 3 VF–C M–Ps SR–R P EZ7 3 M–C Ms SR–WR P EZ8 3 M–C Ms SR–WR P Abbreviations: VF–C = very fine to coarse grained; F–C = fine to coarse; F–M = fine to medium; M–C = medium to coarse; M–VC = medium to very coarse; M–Ps = moderate to poorly sorted; Ms = moderately sorted; Ps = poorly sorted; SR–R = Subrounded to rounded; SA–SR = Subangular to subrounded; SA–R = Subangular to rounded; SR– WR = Subrounded to well rounded; R–WR = Rounded to well rounded; P = Point contact; P > C = Point contact > concave convex contact; P > F = Point contact > float contact; F > P = Float contact > Point contact. Fig. 4a). Quartz is mainly monocrystalline type with undulatory extinction (Fig. 4a and e). Few quartz grains are of polycrystalline type. Some of quartz grains contain inclusions of rutile, zircon and tourmaline (Fig. 4e). Long, point, and concavo-convex contacts are common (Fig. 4e) and are caused by pressure solution and compaction. Some quartz grains display syntaxial overgrowths (Fig. 4d), and some others are corroded at their margins (Fig. 4b and c). Heavy minerals, mica flakes, clay minerals (especially kaolinite) and bioclastic shell fragments are also existed (Fig. 4f). Mica and heavy minerals (rutile, zircon and tourmaline) appear in accessory quantities (<1.0%, Table 3). The Upper Kareem (Shagar) sandstones have an average detrital framework composition of Q81.3F14.6R4.1. Framework constituents comprise 73% of the rock, and the matrix and cement constitute about 27%. The framework is cemented with dolomite, anhydrite, calcite and silica (Fig. 5). Average existing pore space constitutes 9.7% of the rock. The quartz grains are of undulose and plutonic types. They are dominantly monocrystalline (Fig. 5c and d) and rarely polycrystalline. Some grains are corroded and partially replaced by dolomite and/or anhydrite cement in part (Fig. 5c and d). Many of quartz and feldspar grains have a secondary overgrowth (Fig. 5b–d). Feldspars include K-feldspars, and plagioclase, which is partially altered to sericite. Perthite, orthoclase and microcline fragments are also present. The lithic fragments are mainly of granitic, volcanic or carbonate composition. Glauconite pellets, algal fragments and planktonic foraminiferal tests are also recorded (Darwish and El-Araby, 1993). Some bioclasts (Foraminifera) are selectively leached and partially occluded a secondary intraparticle and moldic porosity. Most of pore filling dolomite cement is corroded (Fig. 5e and f) and partially occluded vuggy porosity (Fig. 5a and c). The important constituent framework grains of the sandstones of the Kareem Formation are quartz including both monocrystalline and polycrystalline type. Monocrystalline quartz grains are generally stretched and show undulatory extinction. Polycrystalline quartz grains represent weakly foliated grains of equant and prolate shapes. Sedimentary lithics include fragments of quartzose siltstone, siliceous and non-siliceous shale fragments and carbonate rock fragments. The siliceous materials usually have fine-grained texture and commonly contain a siliceous matrix. The carbonate grains commonly represent coarsely crystalline limestone grains generally coated with iron oxide. In addition to the main framework constituents, a suite of heavy minerals including opaques are observed in the studied sandstones. These mineral grains include hematite, rutile, tourmaline, zircon, and muscovite. The sandstones of the Kareem Formation are loosely indurated to hard. The mean grain size ranges from fine to coarse-grained. A major portion of the framework grains is rounded to subrounded and unimodal. These sandstones are (76%) moderately well sorted, followed by (14%) well sorted, and (10%) moderately sorted. 4.2. Clay mineralogy The clay minerals identified in sandstones are kaolinite, illite and smectite. Kaolinite dominated in Upper Shagar sandstones, while both illite and smectite are recorded with kaolinite in the Lower Rahmi sandstones (Fig. 6). These variations may be related to relative changes in the climatic conditions in the source area. The moderate crystallinity exhibited by the clay minerals indicates their detrital origin from weathering horizons and soils developed on silicic rocks, and transportation in a fluvial environment (Keller, 1956; Abu-Zeid et al., 1989, 1991). Source area weathering is confirmed by the low percentage of smectite and absence of chlorite (Fig. 6). The predominance of kaolinite with little or without illite, especially at the Upper Member, indicates their sedimentary origin under continental conditions (Lonnie, 1982; Tsuzuki and Kawabe, 1983; Amer et al., 1989). 4.3. Diagenetic minerals The most common diagenetic constituents of the sandstones of the Kareem Formation in studied wells are dolomite, calcite, anhydrite, quartz, and kaolinite: (1) Authigenic quartz is present in all samples under investigation. It was better developed in large intergranular pore networks and the pores are often occluded by large quartz overgrowths (Fig. 4b). It ranges between 0.3% and 2.5% with an average of 0.5%. Quartz cement mainly occurs as syntaxial overgrowths (Fig. 4d). Also, it occurs as syntaxial outgrowths in clay-coat-rich sandstones (Fig. 4b and c). Thus, quartz overgrowth is recorded as second cement in this unit after iron oxide. The pore waters required for the precipitation of these overgrowths would have been acidic or slightly alkaline, in an environment containing sufficient dissolved silica to allow quartz overgrowths formation. During diagenesis sediments were subjected to different conditions, which might activate sources of silica for quartz cementation, such as dissolution of feldspar (Hawkins, 1978), pressure solution (Bjørlykke et al., 1986; Houseknecht, 1988; Dutton and Diggs, 1990; Bjørlykke and Egeberg, 1993; Dutton, 1993; Walderhaug, 1994), replacement of quartz and feldspar by calcite (Burley and Kantorowicz, 1986) and transformation of clay (Hower et al., 1976; Boles and Franks, 1979; Rodrigo and Luiz, 2002). The dissolved silica of the sandstones of the Kareem Formation was probably derived from the extensive dissolution of feldspar and 36 Table 3 Detrital grains modes and the derived QFL indices of the Lower Kareem Rahmi Member. S. no. Core no. Depth Qm Qp KF Pl Lp Lv Ls M Op Hm Gl Bio Clays QFL% Qt Zeit Bay Field L Qm Cement and/or matrix F P.C.P Lt ZB7 4 1531 90.8 2.2 2.5 0.1 0.3 0 0.7 0.1 0.2 Tr 0 Tr 3 96.2 2.7 1.1 93.9 2.7 3.3 11.7 16 ZB8 ZB9 4 5 1533 1547 91.5 89.5 2.6 2.3 2.5 2 0.2 0.4 0.2 0.5 0 0 1.3 1.5 0.2 1 Tr Tr Tr Tr 0 Tr Tr Tr 1.5 2.8 95.7 95.4 2.7 2.5 1.5 2.1 93.1 93.0 2.7 2.5 4.1 4.4 12.9 11.5 17 16 ZB10 ZB11 5 6 1550 1561 84.5 85.5 2.8 2.6 3.5 2.5 1.2 0.5 0 0.2 0 0 1.5 1 Tr 0 Tr 0.6 Tr Tr Tr Tr Tr Tr 6.5 7.1 93.4 95.4 5.0 3.3 1.6 1.3 90.4 92.6 5.0 3.3 4.4 3.9 15.5 15.7 14.5 14.2 ZB12 ZB13 6 7 1565 1577 88 87 2.8 3 2.9 4 0.5 0.2 0.2 0.1 0 0 1 0.3 Tr 0.3 Tr Tr Tr Tr Tr Tr Tr Tr 4.6 5.1 95.2 95.1 3.6 4.4 1.3 0.4 92.2 92.0 3.6 4.4 4.1 3.4 16.2 15.7 13.8 12.5 ZB14 ZB15 7 8 1578 1580 89 87 2.5 3 3.4 3.5 0.5 0.6 0 0 0 0 2 0.8 Tr 0.3 0.7 0.7 Tr Tr 0 0 0.5 0.3 1.4 3.7 93.9 94.7 4.0 4.3 2.1 0.9 91.4 91.6 4.0 4.3 4.6 3.9 16.8 14.1 13 12.5 ZB16 ZB17 8 9 1582 1591 88 83 2 2 5.4 5 0.2 0.2 0 0.1 0 0 0 1.6 1.4 3.2 Tr Tr Tr Tr 0 Tr Tr Tr 3 5 94.0 92.5 5.9 5.7 0.1 1.8 92.1 90.3 5.9 5.7 2.1 3.8 14.5 15.3 13.5 13 EZ9 4 2733 85.5 2 6.6 0.6 0 0 1.6 0.5 Tr Tr Tr 0 3.3 90.9 7.5 1.7 88.8 7.5 3.7 17.4 11.5 EZ10 EZ11 4 5 2734 2741 86 84.5 2.1 2.6 5.8 4.7 0.9 0.8 0 0.1 0 0 0.4 1.5 0.5 0.5 Tr Tr Tr Tr Tr Tr 0 0 4.3 5.5 92.5 92.4 7.0 5.8 0.4 1.8 90.3 89.6 7.0 5.8 2.5 4.4 15.5 14.6 12.5 14.5 EZ12 EZ13 5 6 2744 2756 88 89 2 3 3.3 3.9 0.3 0.3 0 0 0 0 1.8 2.1 0.4 0.4 Tr Tr Tr Tr Tr 0 Tr Tr 4.2 1.3 94.3 93.6 3.8 4.3 1.9 2.1 92.2 90.5 3.8 4.3 3.9 5.1 13.1 11.9 15.5 16 EZ14 6 2760 88.5 2 2.7 0.6 0.4 0 2.1 Tr Tr Tr Tr Tr 3.7 94.0 3.4 2.6 91.9 3.4 4.6 12.7 15 EZ15 EZ16 7 7 2779 2780 87 89 2.3 2.3 3.6 3.5 0.2 0.3 0.5 0 0 0 1.5 2.5 Tr Tr Tr 1.1 Tr Tr Tr Tr 0.3 0.7 4.5 1.7 93.8 93.5 4.0 3.9 2.2 2.6 91.4 91.2 4.0 3.9 4.5 4.9 11.9 15.9 16.5 13.5 EZ17 EZ18 8 8 2782 2784 88.5 87 2 3 3 3.7 0.3 0.6 0 0 0 0 1 0.3 0.7 0.7 Tr Tr Tr Tr Tr Tr 0 0 3.5 4.7 95.5 95.1 3.5 4.5 1.1 0.3 93.4 92.0 3.5 4.5 3.1 3.3 15.5 16.6 13 12.2 EZ19 EZ20 9 9 2805 2809 90 89 2.1 2.1 4.5 5 0.6 1.3 0.4 0 0 0 0.3 0.3 0.2 Tr Tr Tr Tr Tr 0 0 0 0 1.9 2.3 94.1 93.2 5.2 6.4 0.7 0.3 91.9 91.1 5.2 6.4 2.8 2.4 15.8 16.3 13.8 12.5 EZ21 10 2835 91.6 3 2 1 0 0 0.3 0.2 Tr Tr 0 0 1.9 96.6 3.1 0.3 93.6 3.1 3.3 14.3 13.0 83–91.5 87.8 2.0–3.0 2.4 2.0–6.6 3.7 0.1–1.3 0.5 0–0.5 0.13 0–0 0 0.3–2.5 1.14 0–3.2 0.6 0–0.7 0.7 0–Tr 0 0–Tr 0 0–0.7 0.2 1.3–6.5 3.6 92.4–96.6 94.2 2.5–7.5 4.4 0.1–2.6 1.3 88.8–93.9 91.7 2.5–7.5 4.4 2.1–5.1 3.8 11.5–17.4 14.6 11.5–17.0 14.0 Range Average S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 East Zeit Oil Field QmFLt% F Average 3 Abbreviations: Monocrystalline quartz (Qm); Polycrystalline quartz (Qp); K-feldspar (K); Plagioclase (Pl); Plutonic lithic fragment (Lp); Volcanic lithic fragment (Lv); Sedimentary lithic fragment (Ls); Mica (M); Opaque (Op); Hematite (Hm); Glauconite (Gl); Bioclasts (Bio); Q = Quartz; F = Feldspar; Fr = Fracture; D = Dolomite; I = Iron oxide; QO = Quartz overgrowth; PC = Point contact; LC = Line contact; CXC = Concave convex contact; Dd = Dolomite dissolution; P = pores; Qc = Quartz corrosion; FO = Feldspar overgrowth; Il = Illite; Py = Pyrite; K = Kaolinite; An = Anhydrite. Qt = Qm + Qp, F = Pl + KF, L = Lp + Lv + Ls, Lt = L + Qp, Q = total quartzose grains, F = total feldspar, Pl = plagioclase, KF = K-feldspar, L = unstable lithic fragments, Lt = lithic + polycrystalline quartz grains and P.C.P = pointe counted porosity. 9.7 14.8 1.2 0.0 21.1 1.8 70.0 0.8 0.2 0.0 3.1 0.0 1.7 0.5 1.3 74.1 22.5 3.4 72.3 22.5 5.2 9.6 5.7– 12.4 17.4 6.2–21.3 0.5– 11.5 4.8 30.5 11.9– 30.6 64.2– 83.2 64.7 2.3 0.5– 8.5 11.9– 30.6 30.5 67.2 67.2– 90.9 Tr 0– 5.8 0.0 0– 6.2 Tr Tr– 1.5 Tr 0– Tr 1.7 Tr– 2.7 0– 0.3 0.0 1.6 0.5– 8.3 0– 0 0.0 0.7 0– 0.7 62– 83 0.5 29.8 5.2– 29.8 2.5 0– 2.7 64.2 0– 1.5 7.8 10.5 18.7 14.1 EZ8 2723 Range 5.7 12.4 21.3 6.2 5.1 3.3 30.6 28.2 20.4 27.0 73.6 67.0 64.2 68.4 2.1 1.3 3.9 3.0 20.4 27.0 67.3 70.4 0.7 Tr 0.0 0.7 Tr 0.3 Tr Tr Tr Tr Tr Tr 2.7 1.3 0.3 0.0 0.0 0.0 1.5 1.3 3.7 3.0 0.0 0.0 0.0 0.0 0.5 0.0 0.0 0.0 28.1 27.0 1.5 0.6 17.8 26.3 3.0 2.0 62.0 66.8 3 3 EZ6 EZ7 2720 2722 2 2 EZ4 EZ5 2679 2680 69.8 66.5 2.0 3.0 1.5 0.5 Tr 1.3 0.7 75.7 70.0 0.7 Tr 2.9 0.0 30.6 28.2 5.9 6.0 12 7.8 8.3 15.0 19.2 18.6 11.5 9.4 3.1 21.1 16.9 14.3 71.5 76.2 75.8 2.1 8.5 6.9 16.9 14.3 21.1 76.8 74.5 78.8 Tr 0.0 0.7 2.0 0.0 Tr 0.3 0.7 Tr 0.0 0.0 2.3 2.3 1.5 0.0 0.0 0.0 2.0 8.3 6.7 0.0 0.0 0.0 0.0 0.0 0.0 11.6 12.3 0.6 0.0 1.5 19.6 16.5 12.4 1.0 3.0 2.5 69.6 74.0 72.5 2666 1 1 2 EZ1 East Zeit Bay Field EZ2 EZ3 2668 2678 7.8 10.5 6.7 5.0 1.7 0.5 20.7 10.9 13.3 28.0 27.9 30.3 70.4 69.2 78.2 68.7 5.6 2.8 1.7 0.5 27.9 30.3 13.3 28.0 0.2 Tr 81.1 69.2 Tr 0.0 0.0 0.0 0.0 0.0 0.3 0.3 Tr Tr 0.0 0.0 Tr Tr 5.3 2.3 1.7 0.5 0.0 0.0 0.0 0.0 0.0 0.5 0.0 0.5 27.8 29.7 0.6 1.0 12.0 26.7 0.0 0.0 74.0 68.0 3 3 ZB5 ZB6 1520 1523 2 2 ZB3 ZB4 1470 1474 70.0 69.0 2.7 0.5 0.0 0.0 Tr Tr 1.7 Tr 1.5 0.3 2.2 0.7 70.4 69.2 8.3 3.3 11 8.5 15.7 18.1 5.0 4.8 11.9 13.9 81.0 83.2 4.2 2.7 13.9 11.9 83.9 83.5 5.8 Tr 1.7 6.2 Tr Tr Tr Tr Tr Tr 0.0 0.0 2.0 3.4 0.0 0.0 0.5 0.5 1.0 0.8 10.0 12.2 0.6 2.3 76.0 77.0 1463 1 1 ZB1 Zeit Bay Field ZB2 1465 P.C.P QmFLt% Qm Clays Hm Ls Lv Lp Pl KF Qp Qm Depth Core no. S. no. Table 4 Detrital grains modes and the derived QFL indices of the Upper Kareem Shagar Member. M Op Gl Bio F L QFL% Qt F Lt Cement and/or matrix S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 37 volcanic lithic fragments, kaolinitization and chemical compaction (Zhang et al., 2008; Umar et al., 2011). (2) Carbonate cement is the second cement in the studied sandstones. It ranges from 4.5% to 20.1% with an average of 2.8%. The carbonate cement contains ferroan and nonferroan calcite and dolomite. Generally, dolomite cement is more common than calcite cement phase (Figs. 4, 5 and 7). In some cases, dolomite occurs as coarsely crystalline cement (Figs. 4b and 7a and b). Ferroan dolomite occurs mainly as fine and medium rhombs pore occluding phase (Figs. 4c, 5d and 7f) and locally as a grain replacive phase (Fig. 7a). The source of magnesium is those released through the washing of clay minerals. On the other hand, wide spread ferroan carbonate cementation is thought to have occurred under reducing alkaline pore water conditions (Morad, 1998; El-ghali et al., 2009). The ions required for cement formation were probably derived from alumino-silicate grain dissolutions, and clay mineral transformations. Weakly ferroan calcite is the minor carbonate cement phase in the sandstones of the Kareem Formation. It commonly occurs in association with detrital carbonate components suggesting that these acted as nuclei for cement formation. The ferroan calcite cement has survived dolomitization most probably due to poor permeability for the circulation of Mg-rich fluids (Fig. 7a and b). (3) Authigenic feldspars are less abundant in the sandstones of the Kareem Formation. They are most frequent as an early diagenetic mineral and predate any tectonic deformation (Kastner, 1971). They are formed almost exclusively as overgrowths on detrital feldspar grains in sandstones. In the studied samples, feldspar overgrowths are ubiquitous, usually as incipient overgrowths (Fig. 5b), and sometimes intergrown with authigenic clay phase. Feldspar overgrowths in sandstones have presumably resulted from the dissolution and kaolinitization of silicate grains, particularly feldspars and micas, which can be accomplished by meteoric waters (Morad et al., 2000; El-ghali et al., 2009). Meteoric water influx into the sandstones is attributed to relative sea-level fall and basin ward shift of the shore line. This would be a form of ‘‘distillation’’ of an impure to pure feldspar and would explain the general dependence on the presence of detrital feldspars in most of the studied samples of the Upper Kareem (Shagar) sandstones. (4) Authigenic anhydrite typically occurs as poikilotopic rhombs or elongate laths infilling pores but also as vein filling cement (Figs. 4a and e and 5a and d). The anhydrite was precipitated after the quartz, calcite and dolomite (Fig. 5a and d). The sulfate for anhydrite precipitation could have been derived from the dissolution and reprecipitation of early gypsum cementation as gypcrete, since it is highly soluble and remobilization of anhydrite is common during diagenesis (Schmid et al., 2004). Sullivan et al. (1990) suggested that sulfate for anhydrite precipitation may be supplied by fluids expelled from surrounding evaporites. (5) The authigenic kaolinite that is so common in some sandstone has the appearance of a well crystallized, pure pore filling that was precipitated from a solution and shows no evidence of alteration from a precursor clay mineral (Pettijohn et al., 1973). 38 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 Fig. 3. QFL triangular diagram shows the classification of reservoir sandstones of the Kareem Formation (modified from Dott (1964) and McBride (1963). PC Q PR a QO D Q Vu 100 µm b I QS d DC D FC QC QO D QO D An D I I QC Fr 100 µm FC c Sh fr PR LC 100 µm D An Q Fr F D VU MO Qin 100 µm e VXC 100 µm f Ca 100 µm Fig. 4. Photomicrographs of quartzarenites showing: (a) Laths of authigenic anhydrite (An) vein filling cement (Note: reduction in primary porosity (PR)). (b) Dust line of iron oxide cement (I) separating detrital quartz (Q) from authigenic silica (QO). Quartz grains are fractured (Fr) and corroded at their margins (QC) and primary pores are occluded by large quartz overgrowth (QO). (c) Quartz cement occurs as syntaxial outgrowths (QO) in clay-coat-rich sandstones (Note: fine to medium dolomite rhombs (D) pore occluding phase). (d) Some quartz syntaxial overgrowths (QS) post date iron oxide (I) (hematite) and pre-dated dolomite cement (D). (e) Closely packed, long (LC), point and concave–convex contact (VXC) of quartz, chert, and highly altered feldspar. Note: quartz inclusions (Qin), pore filling authigenic anhydrite (An) and reduction in primary porosity (PR). (f) Compaction and dissolution of bioclastic shell fragments (ShFr) with oversized pore left (Note: vuggy (Vu) and moldic (Mo) pores). The kaolinite is determined in the sandstones of the Kareem Formation as booklets and vermicular aggregates in mud intraclast, mud matrix, pseudo matrix and detrital grains, as pore filling cement (Fig. 7e), and as grain coating on detrital grains (Fig. 7c). Also, the late phase kaolinite is precipitated on early phase quartz overgrowth (Fig. 7d). The kaolinite formation is dependent on: (a) sufficient porosity and permeability to allow migration of interstitial pore waters and to provide growth space, (b) the presence of K-feldspar and/or muscovite as a source of Al and Si, and (c) pore waters of an acidic pH. The presence of illite is visible as fibrous illite, mat like and lath like crystals within kaolinite, mud matrix, and mud intraclast. It is oriented perpendicular to grain surfaces. Additionally, illite seems as platelets occur arranged on the framework grain surfaces and as high birefringence patches. So, illite cover kaolinite and quartz grain edge (Fig. 7d). Illite, which typically forms during progressive burial under elevated temperature (90– 130 °C; Morad et al., 2000) required high K-pore water to achieve illitization in the sandstone. On the other hand, the occurrence of mixed layer illite/smectite is less common in the sandstones of the Kareem Formation. The honeycomb like texture of grain coating clays is mixed layer illite/smectite. Mixed clay occurs as a minor pore lining to locally pore-filling clay with ragged-platy morphology. SEM analysis indicates that illite/smectite post-dates the quartz cementation (Fig. 7c). 39 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 D Ca An FO D F DC VU QC QO VU a b D An c QO D DC An 100 µm DL Py D QC d 100 µm QO e f Fig. 5. SEM images and photomicrographs of subarkose and arkose showing: (a) Pore filling authigenic anhydrite cement (An) after calcite (Ca) and dolomite (D). (b) Feldspar overgrowth (FO) and corroded dolomite (DC) overgrown by anhydrite cement. (c) Monocrystalline quartz grains (Q) and authigenic silica (QO) are corroded (QC) and partially replaced by dolomite cement (D). (d) Pore filling dolomite (D) partially replaced by authigenic anhydrite cement. (An) Note: authigenic anhydrite after quartz overgrowth (QO) and dolomite cement (D). (e) Quartz overgrowth (QO) is partially replaced by later dolomite cement (D), thus predate dolomite. Note: leaching and corrosion of dolomite cement (DC). (f) Framboidal pyrite (Py) crystallites locally replace dolomite cement. Note: dolomite cement is partially leached (DL) and corroded. Fig. 6. Lithologic logs, clay content %, Chemical Index of Alteration (CIA), Chemical Index of Weathering (CIW) and Maturity Index (MI) of the Middle Miocene Kareem sandstones at studied wells. (6) Pyrite is known as a diagenetic mineral in sandstones and implies reducing conditions, presumably reflecting a deoxygenated environment of deposition. Pyrite cement is recorded as partial cement at certain levels within sandstones. Pyrite cement is also present in trace amounts as framboids located within dissolved grains and dolomite matrix (Fig. 5f). Pyrite cementation continued at a later stage of diagenesis, locally occluding the pores. 4.4. Geochemistry The geochemical classification diagrams of Pettijohn et al. (1972) and Herron (1988) for the sandstones of the Kareem Formation (Fig. 8a and b) provide the same petrographic results. The major element contents of the sandstones of the Kareem Formation are given in Table 5 with their ratios between elements. These elements are compared in Table 6 with the average composition of 40 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 Il/sm D D Il/sm D VU D QO 100 µm a I P VU K K D c QO D QO 100 µm b Fr QC D Il d QC f e 100 µm Fig. 7. SEM images and photomicrographs of arenites and subarkoses showing: (a) Dolomite (D) after a shell fragment with dissolved margins. Dolomite is coarsely crystalline and locally present as a grain replacive phase. (b) Recrystallization of microcrystalline dolomite cements (D) forming coarsely crystalline dolomite that enhanced intercrystalline porosity. (c) Quartz overgrowths (QO) engulfed by dolomite (D) and coated by illite/smectite (il/Sm) thus predate illite/smectite and dolomite. (d) Iron oxide (I) coating around detrital quartz, thus predate silica (QO) and dolomite cements (D). Note: kaolinite (K) coating on quartz grains; while illite (Il) cover kaolinite and quartz grain edges. (e) Pore filling authigenic kaolinite (K) engulfs, thus post-dates quartz overgrowth (QO). (f) Fine to medium dolomite rhombs (D) present as pore occluding phase and locally as a grain replacive phase. Note: quartz grains are fractured (Fr) and replaced by dolomite cement. Fig. 8. Chemical classification of sandstone samples from the Middle Miocene Kareem Formation based on (log (SiO2/Al2O3) versus log (Na2O/K2O) diagram of Pettijohn et al. (1972), and (b) the log (SiO2/Al2O3) versus log (Fe2O3/K2O) diagram of Herron (1988). passive margin sandstones (Bhatia, 1983), Amazon big river sands (Potter, 1978) and average arkosic sandstones (Pettijohn, 1963) to be used later for investigating provenance and tectonic setting. Table 5 shows that, most of sandstone samples are rich in SiO2 (69.9–94.2%). The source of silica is mainly quartz, chert, quartzite, feldspars and clay minerals. Sandstones have a wide range of Al2O3 (0.97–11.78%), MgO (0.07–6.6%), K2O (0.12–6.0%) and Fe2O3 (0.03–4.5%). Al2O3 and K2O content may relate to the presence of K-feldspars (orthoclase and microcline), illite and mica, while MgO content may relate to the abundance of dolomite cement and Fe2O3 content may relate to the abundance of iron oxide heavy minerals and partly to Fe-containing clay minerals. In contrast, the sandstones of the Kareem Formation possess low average contents of Na2O, TiO2, MgO, and CaO. The source of Na2O is principally related to plagioclase feldspar. Ti-opaque minerals and rutile are the main holders of TiO2. MgO content is related mostly to the presence of dolomitic materials as fragments or cement. Carbonate cement and rock fragments and diagenesis of plagioclase are the main source for CaO. Kareem sandstones are highly depleted in most of the major elements except SiO2 (due to enrichment in quartz) suggesting an intense degree of weathering and reworking that removed ferromagnesian minerals and feldspars. Generally, most major elements show positive correlations with Al2O3 (Fig. 9). However, these elements show marked negative correlations with SiO2, confirming that much of SiO2 is present as quartz grains (Akarish and El-Gohary, 2008). The high K2O/Na2O ratios (av. 8.27%, Table 5) are attributed to the common presence of K-bearing minerals such as K-feldspar, mica, illite, muscovite and biotite (McLennan et al., 1983; Nath et al., 2000; Zhang, 2004; Osae et al., 2006). A positive correlation between K2O and Al2O3 (r = 0.92) implies that the concentrations of the K-bearing minerals have significant influence on Al distribution and suggests that the abundance of these elements is primarily controlled by the content of clay minerals (McLennan et al., 1983; Jin et al., 2006; Akarish and El-Gohary, 2008). Alteration of rocks during weathering results in depletion of alkalis (Na2O, K2O) and preferential enrichment of Al2O3 in sediments (Cingolani et al., 2003). Therefore, weathering effects can be evaluated in terms of the molecular percentage of the oxide components, using the formulae of Chemical Index of Weathering (CIW = [Al2O3/(Al2O3 + CaO + Na2O] 100; Harnois, 1988) and Chemical Index of Alteration (CIA = [Al2O3/(Al2O3 + CaO + Na2O + K2O] 100); Nesbitt and Young, 1982). 5. Discussion Based on the petrographic study, the sandstones of the Kareem Formation are classified as quartzarenites, subarkoses and arkoses. Quartzarenites present in Lower Kareem, where the subarkoses and arkoses recorded only in Upper Kareem. The average contents of different quartz grains in these sandstones show granitic and/or 41 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 Table 5 Chemical composition of the Middle Miocene Kareem sandstones. Depth S. no. SiO2 Al2O3 TiO2 CaO MgO Na2O K2O Fe2O3 MnO P2O5 LOI Sum SiO2/Al2O3 K2O/Al2O3 K2O/Na2O TiO2/Al2O3 Fe2O3/Al2O3 log SiO2/Al2O3 log Fe2O3/K2O CIW CIA Lower Kareem (Rahmi Member) Upper Kareem (Shagar Member) 1531 1550 1577 1582 2734 2760 2784 2835 1463 1470 1520 2668 2679 2720 2723 ZB7 93.10 1.20 0.07 0.05 1.27 0.03 0.13 1.10 0.03 0.00 2.82 99.80 77.58 0.11 3.82 0.06 0.92 1.89 0.93 93.46 84.87 ZB10 87.50 1.12 0.09 0.13 6.60 0.17 0.77 1.13 0.03 0.06 2.38 99.98 78.13 0.69 4.53 0.08 1.01 1.89 0.17 78.87 51.14 ZB13 90.30 0.97 0.06 0.14 5.08 0.06 0.12 1.05 0.01 0.00 2.49 100.28 93.09 0.12 2.00 0.06 1.08 1.97 0.94 82.91 75.19 ZB16 90.10 0.97 0.06 0.14 5.30 0.06 0.12 1.08 0.01 0.00 2.49 100.33 92.89 0.12 2.00 0.06 1.11 1.97 0.95 82.91 75.19 EZ10 88.30 1.12 0.09 0.13 5.80 0.17 0.77 1.13 0.03 0.06 2.38 99.98 78.84 0.69 4.53 0.08 1.01 1.90 0.17 78.87 51.14 EZ14 90.60 1.09 0.06 0.09 3.20 0.06 0.12 1.50 0.01 0.07 3.22 100.02 83.12 0.11 2.00 0.06 1.38 1.92 1.10 87.90 80.15 EZ18 90.10 1.16 0.06 0.11 3.90 0.14 0.82 1.00 0.01 0.01 3.28 100.59 77.67 0.71 5.86 0.05 0.86 1.89 0.09 82.27 52.02 EZ21 94.20 1.20 0.20 0.00 0.20 0.14 0.81 1.03 0.02 0.01 3.23 101.04 78.50 0.68 5.79 0.17 0.86 1.89 0.10 89.55 55.81 ZB1 90.30 5.90 0.21 0.01 0.07 0.19 1.10 1.13 0.01 0.03 2.06 101.01 15.31 0.19 5.79 0.04 0.19 1.18 0.01 96.72 81.94 ZB3 90.00 6.02 0.22 0.15 0.80 0.19 1.13 1.15 0.05 0.03 1.35 101.09 14.95 0.19 5.95 0.04 0.19 1.17 0.01 94.65 80.37 ZB5 69.90 11.78 0.69 0.20 1.10 0.30 6.00 4.50 0.12 0.03 4.60 99.22 5.93 0.51 20.00 0.06 0.38 0.77 0.12 95.93 64.44 EZ2 90.10 4.21 0.12 0.07 3.06 0.20 0.86 1.09 0.02 0.00 1.32 101.05 21.40 0.20 4.30 0.03 0.26 1.33 0.10 93.97 78.84 EZ4 90.50 4.33 0.12 0.12 1.10 0.39 1.20 1.20 0.02 0.00 2.02 101.00 20.90 0.28 3.08 0.03 0.28 1.32 0.00 89.46 71.69 EZ6 79.60 8.49 0.30 0.20 0.40 0.20 5.20 2.00 0.04 0.03 1.70 98.16 9.38 0.61 26.00 0.04 0.24 0.97 0.41 95.50 60.26 EZ8 75.96 9.57 0.50 0.14 0.18 0.17 4.82 2.90 0.01 0.06 5.77 100.08 7.94 0.50 28.35 0.05 0.30 0.90 0.22 96.86 65.10 gneissic source. These have been confirmed by overall variation in the relative abundance of different types of quartz grains (monocrystalline and polycrystalline). The narrow grain-size range suggests either more or less uniform size of the sediments supplied to the basin or the uniform hydrodynamic conditions prevailing during deposition of these sandstone units (Ahmad and Bhat, 2006). The greater abundance of alkali feldspar than plagioclase further supports for granitic and/or gneissic source. The dominance of moderately well sorted either reflects the change in water turbulence during deposition or pulses of sediment supply during episodes of rifting and uplift. The overall sorting indicates alluvial and marine fan-delta settings (Folk, 1980; Alsharhan and Salah, 1997). 5.1. Tectonic setting Dickinson and Suczek (1979) and Dickinson et al. (1983), have related detrital sandstone compositions to major provenance types such as stable cratons, basement uplifts, magmatic arcs and recycled orogens. To interpret the tectonic discrimination source fields, the Lower and the Upper Kareem sandstones were plotted on QtFL and QmFLt ternary diagrams of Dickinson et al. (1983). The Lower Kareem sandstones fall in the craton interior, whereas the Upper Kareem sandstones fall in the transitional continental, craton interior and partly in recycled orogenic fields (Fig. 10a and b). Fig. 10a and b shows that the Lower Kareem sandstones are mature and derived from relatively low lying granitoid and gneissic sources. The low percentage of unstable grain (feldspar and other rock fragments) <6%, the dominance of monocrystalline quartz, and alteration of feldspar grains, indicate that Lower Kareem sandstones were transported from the far along the rift. However, the Upper Kareem sandstones are derived from craton interior, transitional continental and recycled orogenic setting. The high percentage of unstable grain >15%, indicate that the Upper Kareem sandstones show short transport distance and quick burial. This means that the Upper Kareem sandstones are typically rift sandstone and their deposition constrained the beginning of the faulting in studied area (Zaid, 2012). This result supports and gives a great evidence for the unconformable relationship between the Lower Kareem (Rahmi Member and the overlying Upper Kareem (Shagar Member) (Youssef, 1986; Tewfik et al., 1992). The percentages of major elements (Table 5) were used to discriminate the tectonic setting of sandstones (Schwab, 1975; Bhatia, 1983; Roser and Korsch, 1986, 1988; Armstrong-Altrin et al., 2004). The discriminate function diagrams were used to understand the provenance for the Lower and Upper Kareem sandstone terrain. The discriminate function diagram of Roser and Korsch (1988) suggests that both Lower Rahmi and Upper Shagar sandstones may be derived from mature polycyclic continental sedimentary rocks Table 6 Comparison of the average chemical compositions of the studied Middle Miocene sandstones and other different sandstones. SiO2 Al2O3 TiO2 Fe2O3 MnO CaO MgO Na2O K2O P2O5 K2O/Na2O Fe2O3/MgO Al2O3/SiO2 Modern Big Rivers (Amazon) (Potter, 1978) Arkose (Pettijohn, 1963) Passive Margin (Bhatia, 1983) Present work 85.32 7.47 0.78 2.76 0.05 1.12 1.02 0.23 1.14 0.02 5.00 3.78 0.09 80.18 9.04 0.31 2.37 0.28 2.81 0.52 1.56 2.91 0.10 1.86 2.89 0.11 81.95 8.41 0.49 3.28 0.05 1.89 1.39 1.07 1.71 0.12 1.60 2.89 0.10 87.3 3.94 0.19 1.53 0.03 0.11 2.54 0.16 1.6 0.03 8.27 4.05 0.05 42 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 r = 0.91 0.8 0.7 100 SiO2% TiO2% r = 0.85 0.6 0.5 0.4 0.3 0.2 0.1 0.0 60 0 2 4 6 8 10 12 14 0 2 4 Al2O3% 8 10 12 14 0.14 5 r = 0.82 r = 0.66 0.12 4 0.10 MnO% Fe2O3% 6 Al2O3% 3 0.08 0.06 0.04 2 0.02 1 0.00 0 2 4 6 8 10 12 14 0 2 4 Al2O3% 6 8 10 12 14 Al2O3% 0.25 7.00 r = 0.5 0.20 r = 0.65 6.00 MgO% CaO% 5.00 0.15 0.10 4.00 3.00 2.00 0.05 1.00 0.00 0.00 0 2 4 6 8 10 12 14 0 2 4 Al2O3% 8 10 8 0.50 12 14 r = 0.92 r = 0.6 0.40 6 K2O% Na2O% 6 Al2O3% 0.30 0.20 4 2 0.10 0.00 0 2 4 6 8 10 12 14 Al2O3% 0 0.00 2.00 4.00 6.00 8.00 10.00 12.00 14.00 Al2O3% Fig. 9. Co-variation of major elements versus Al2O3 for the Middle Miocene Kareem sandstones. Notice the positive correlation of Al2O3 with the major elements, SiO2 and MgO show negative correlation. (Fig. 11a). The discriminate degrees of Bhatia (1983) favor a passive margin setting for Lower Kareem sandstone and active continental margin setting for Upper Kareem sandstone (Fig. 11b). The plotting of samples in the active continental margin field is not consistent with the petrography and the chemical composition. According to Bhatia (1983), Potter (1986) and Roser and Korsch (1988), passive margin sandstones exhibit variable composition. Their characteristics may overlap those of active continental margin sandstones, but they can be distinguished by their higher K2O/Na2O ratio and depletion in Al2O3, CaO, Na2O and TiO2 with respect to those from other settings, features reflecting their recycling and matured nature. Moreover, Bhatia classification gives poor results for fine siliciclastic sediments, which may be misclassified (Roser and Korsch, 1985, 1988). Tectonic discrimination diagrams of Roser and Korsch (1986), and Bhatia (1983) suggest that both lower and upper sandstone falls in the field of passive tectonic margin (Fig. 11c). In silica-rich sands (SiO2 > 70%), with a K2O/Na2O ratio more than unity (Bhatia, 1983) and a FeO + MgO content less than 5% (Taylor and McLennan, 1985), the correlation with a passive margin setting is distinct. The sandstones of the Kareem Formation match all these parameters (Table 5). The uniform chemical characteristics of the sandstones of the Kareem Formation (e.g., high SiO2/Al2O3, K2O/Na2O; Table 5), strongly suggest that the Kareem sandstones derived from recycled older rocks and also from stable continental areas away from the rift area and deposited in a passive margin of a syn rift basin. S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 43 Fig. 10. (a) QtFL and (b) QmFLt ternary diagrams for the sandstones of the Kareem Formation, after Dickinson et al. (1983). 5.2. Source area weathering Chemical data from the Lower and the Upper Kareem sandstones were plotted according to the formula of Nesbitt and Young (1982) and Harnois (1988). The average CIW value of the Lower and Upper Kareem sandstones is 84.6% and 94.7% respectively, which indicates a high weathering (recycling) for both Lower and Upper Kareem sandstones. These CIW values (n = 15, mean = 89.3, s = 6.6; median = 89.5), in general, can be due to either absence of intense recycling in a humid climate or intense recycling in an arid/ semiarid climate (Osae et al., 2006; Wanas and Abdel-Maguid, 2006). The average CIA value of the Lower and Upper Kareem sandstones is 65.6% and 71.8% respectively, which indicates a moderate degree of weathering in the source region for the Lower Kareem, and a higher degree of chemical alteration for the Upper Kareem 44 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 Fig. 11. The tectonic discriminate function diagrams for the sandstones of the Kareem Formation of (a) Roser and Korsch (1988), (b) Bhatia (1983) and (c) Roser and Korsch (1986) A: Oceanic island Arc, B: continental island Arc, C: active continental margin, D: passive margin. sandstones. The low CIA values of the Lower Kareem sandstones are due to the direct input of immature continent detrital minerals into the depositional system (Bakkiaraj et al., 2010). The variation in CIA values (n = 15, mean = 68.5, s = 12.1; median = 71.7), may reflect changes in the proportion of feldspars and the various clay minerals in the analyzed samples. Size sorting during transportation and deposition generally results in some degree of mineral differentiation which may modify the CIA (Pettijohn, 1975; Nesbitt and Young, 1982). The sandstones of the Kareem Formation show upward decrease in maturity. The Lower Member of the Kareem Formation shows a higher degree of alteration (CIA and CIW) than the Upper Member. This may imply that the Upper Member of Kareem sandstones is geochemically moderately immature. Their source areas possibly suffered from weathering, but this was not intense. The Climate precipitation Semi-quantitative weathering index High mountain 0 Relief Moderate hills 1 Low plains 2 Semi arid and Mediterranean Temperate subhumid 0 0 0 0 1 0 1 2 Tropical humid 2 0 2 4 Fig. 12. Log-ratio plot after Weltje et al. (1998). Q: quartz, F: feldspar, RF: rock fragments. Fields 1–4 refer to the semi-quantitative weathering indices defined on the basis of relief and climate as indicated in the table. presence of relatively high proportions of equant subangular to subrounded feldspars, poor to moderate sorting, open matrix-supported texture and partly sutured quartz grains, point to short transportation from a source area with a mix of weathering products from older bed rock (Pettijohn, 1975). In contrast, the Lower Rahmi Member has higher alteration values characteristic of sediments derived from an extensively weathered, chemically mature, source terrain. On the other hand, the mineralogical Maturity Index (MI = [quartz/(quartz + feldspar + rock fragments]); Bhatia and Crook, 1986; Mansour et al., 1999), ranges from 0.64 to 0.94 (Fig. 6), suggesting moderate to relatively high mineralogical maturity. Also, MI decreased from 0.94 at the Lower Member to 0.64 near the top. These relationships may reflect that the chemical composition may be correlated, to a great extent, with the petrographic modal data. Petrographic evidence such as heterogeneous roundness for different grains (coarser ones are rounded and finer ones are angular) implies the importance of mechanical effects for grain shape configuration. Coarse-grained feldspars are related to a low degree of chemical weathering. Moreover, the rounded quartz overgrowths indicate recycling, which, in turn, can modify the compositional data towards the quartz-rich sandstones. The point count data for the sandstones of the Kareem Formation samples on Weltje et al. (1998) diagram, shows that the Lower Kareem sandstones plot in the field number 4, suggesting the sedimentation in a Fig. 13. The effect of source rock on the composition of the sandstones of the Kareem Formation using Suttner et al. (1981) diagram. S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 45 Fig. 14. (a) The ratio SiO2/Al2O3 and Q/(F + RF) in the different types of Kareem sandstones. (b) Chemical maturity of the sandstones of the Kareem Formation expressed by bivariant plot SiO2 versus Al2O3 + K2O + Na2O, Fields after Suttner and Dutta (1986). low-relief and tropical, humid climatic conditions, whereas the Upper Kareem sandstone samples plot in the field number 2, indicating either deposition on a low-relief with a temperate and subhumid climate or on tropical, humid conditions within an area with a moderate relief (Fig. 12). Many of the sandstone samples plot in plutonic field, indicating a plutonic source (Fig. 12). The sedimentary environment of the Kareem Formation is probably one of a linear fault controlled the coastline adjacent to a relatively low relief hinterland with small scale alluvial drainage systems. Despite the subtropical to tropical sea conditions, carbonate production was inhibited due to siliciclastic input (Zahran, 2005). QFRF ternary diagram of Suttner et al. (1981), indicate a metamorphic source rock in a humid climate for the Lower Kareem sandstones and a plutonic source rock in a humid climate for the Upper Kareem sandstones (Fig. 13). However, this particular diagram can discriminate only sources of metamorphic and plutonic rocks (humid or arid conditions) and does not discriminate between different tectonic settings. The diagrams (Figs. 12 and 13) are defined for first-cycle sediments and the effect of recycling and long distance transportation can shift the data on these diagrams toward the humid conditions (Jafarzadeh and Hosseini-Barzi, 2008). These considerations probably imply that new diagrams should be proposed such as those suggested in the field of sedimentary rock geochemistry (Armstrong-Altrin and Verma, 2005) and already proposed in the area of igneous rock geochemistry (e.g., Agrawal et al., 2004; Verma et al., 2006). To make use of the chemical parameters, the ratio of SiO2/Al2O3 against that of quartz, quartzite and chert/(feldspar + rock fragments), (Q/F + RF) was plotted (Fig. 14a) which is interpreted to reflect the maturity of sandstones (Pettijohn, 1975). Higher SiO2 ratio coincides with higher silica phases of quartz, quartzite and chert which in turn reflect that such sandstones are mature. Fig. 14a indicated that the sandstone maturity decreased from the Lower to the Upper Kareem. A bivariant plot of SiO2 against total Al2O3 + K2O + Na2O proposed by Suttner and Dutta, 1986) was used in order to identify the maturity of the sandstones of the Kareem Formation as a function of climate (Fig. 14b). This plot revealed the semi-humid to humid climatic conditions of the samples investigated. Paleoweathering conditions can also be detected using the Al2O3–CaO + Na2O–K2O (A–CN–K) ternary diagram of Nesbitt and Young (1984) (Fig. 15), where unweathered rocks are clustered along the left-hand side of the K-feldspar-plagioclase join (Nesbitt and Young, 1984; Holail and Moghazi, 1998). All the samples ana- Fig. 15. A–CN–K ternary diagram of molecular proportions of Al2O3–(CaO + Na2O)– K2O for the Middle Miocene Kareem sandstones (after Nesbitt and Young (1984)). Also plotted is the average upper continental crust (Taylor and McLennan, 1985), as well as some rock forming minerals important in silicate rock weathering; shown at the side is the CIA scale. Arrows 1–3 represent the weathering trends of granodiorite, adamellite and granite, respectively (Nesbitt and Young, 1984). The sandstones of the Kareem Formation fall closer to moderately to highly weathered minerals. lyzed here plot parallel to the Al2O3–K2O edge, supporting the conclusion that the sandstones of the Kareem Formation were derived from a granite source terrain. The plotting of the samples away from the weathering trend, along the A–K edge toward the K apex, shows the samples are enriched in K and depleted in Ca and Na. The high K2O contents of the sandstones can be explained in various ways. It may be due to post-depositional changes, probably late diagenetic reactions occurring during and following burial through the reaction of basin waters, trapped seawater or brines with minerals of profiles, i.e. K-metasomatism, (Nesbitt and Young, 1989; Fedo et al., 1995). This process can occur through two different paths, representing the conversion of kaolinite (as a matrix) to illite and/or conversion of plagioclase to K-feldspar (Fedo et al., 1995). Another possibility is that the K is primarily related to the presence of detrital K-bearing minerals (McLennan et al., 1983; Nath et al., 2000; Zhang, 2004). 46 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 The sandstone samples of the Kareem Formation plot close to Al2O3–K2O boundary, indicating moderate to intense weathering conditions in the source area. Obviously the highest degree of alteration (in terms of CIA) is compatible with the sediments having maximum kaolinite and less feldspar content. CIA values correlated well with kaolinite content (Fig. 6). They decrease upwards with a decrease in kaolinite and increase in feldspar. 5.3. Provenance A high percentage of quartz (92.2–96.6%) and textural features such as medium to fine grains, moderately sorting and the subangular to subrounded shape and low-percentage of feldspar (2.5– 7.5%) and other rock fragments (0.1–2.6%); (Table 3), show transportation from distant/remote sources or extensive reworking of the sediments and indicates a cratonic or a recycled source for the Lower Kareem Rahmi Member (Al-Habri and Khan, 2008). Whereas, the textural features such as medium to coarse grains, poorly sorting and the subangular to subrounded shape and high-percentage of unstable grain: feldspar (11.9–30.6%) and other rock fragments (0.5–8.5%); (Table 4), indicate that the Upper Kareem Shagar sandstones show short transport distance and quick burial. The Kareem sandstones deposited in the craton interior to transitional continental (Fig. 10), derive from the exposed basement shield area, probably platform or uplifted basement rocks. They might be derived mainly from weathered and low-lying crystalline basement rocks or from recycled sediments. The presence of mixed altered and fresh feldspars may reflect immature sediments interfingered with more mature phases. This would favor a weathered crystalline granitic source terrain (Pettijohn, 1975; Roser et al., 1996; Akarish and El-Gohary, 2008). Relatively unstrained monocrystalline quartz grains that contain common inclusions are present in all samples, suggesting a plutonic origin (Basu et al., 1975; Potter, 1978; Hindrix, 2000). The polycrystalline quartz grains composed of three or more crystals with straight to slightly curved intercrystalline boundaries indicate that the sandstones of the Kareem Formation were derived from plutonic igneous rocks (Folk, 1974; Blatt et al., 1980). The low percentage of feldspar and rock fragments or their absence in many samples especially from the Lower Kareem Rahmi Member favors a cratonic source, mature transport regime and long moderate chemical weathering in a warm dry climate (Amireh, 1991; AlHabri and Khan, 2008). The quantitative petrography provides important information on the nature of the source area. The high proportion of quartz, as well as the dominance of K-feldspar over the more chemically unstable plagioclase in the sandstones of the Kareem Formation suggests that the source was exposed to prolonged weathering and that the sediment is at least partly multicyclic (Osae et al., 2006). This mineralogy is consistent with their derivation from plutonic rocks. However, the presence of rare rounded detrital quartz grains, sedimentary lithic fragments, and rounded grains of zircon and tourmaline, suggest that a component of the provenance is older (pre-existing) sedimentary rocks. Moreover, the presence of greater than 70% SiO2 implies the sandstones are rich in quartz from quartz-rich crystalline provenance. K2O/Na2O ratio can be considered as a simplified chemical provenance indicator (Potter, 1978). Higher values of this ratio reflect derivation from granites rather than from basic rocks. This is also confirmed by the clay mineral content, as an illite and kaolinite were considered to be inherited from weathering horizons and soils developed on silicic (granitic) rocks. In addition, the low percentage of smectite (9%) and the absence of chlorite clay minerals also preclude mafic source rocks. In the rift basins, arkoses are common and sandstones have low mineralogical maturity because the sediment may have been derived from uplifted horsts along the rift where erosion pierced the sedimentary cover and cut into the crystalline basement, as is also the case with the sandstones of the Kareem Formation. The coexistence of arkosic and subarkosic sandstones with subordinate quartzarenites was interpreted as an interplay of pulses of rapid uplift of the source area and quick subsidence of the basin, followed by a period of quiescence within an overall transgressive– regressive cycle in a rift tectonic regime. During quiescence, the first-cycle quartz sand may have been supplied from a nearby quartz-rich source area. A unique combination of tropical climate, low relief, low rate of sedimentation and long residence on the beach formed the mature, first-cycle quartzarenite (Suttner et al., 1981). However, the imprint of climate, although preserved for the first 75 km of transportation in high gradient streams, is rapidly destroyed as soon as a high-energy marine environment (beach) is reached (Suttner et al., 1981). The relative proportion of quartz (87.7%) to feldspars (9.9%) and lithic fragments (2.4%) in the present study sediments is dependent not only on the source rock and climate, but also to some extent on the degree of stability of the basin of deposition (Dickinson and Suczek, 1979). During basin instability, sediments supplied from the source area were quickly buried and more or less retained the original composition, except for the modification of unstable constituents (lithic fragments and feldspars) induced by chemical weathering, which has a greater capacity to alter sandstone composition (Basu, 1976; James et al., 1981; Franzinelli and Potter, 1983; Suttner and Dutta, 1986; Dutta, 1987). The above-mentioned observations reveal that the sediments of the sandstones of the Kareem Formation may have been derived from a variety of source rocks (mixed provenance). This interpretation is also supported by the presence of abundant opaque mineral grains including iron oxides (hematite), which reflect derivation from metamorphic and igneous rocks. The presence of alkali feldspars indicates their source as plutonic and metamorphic rocks (Trevena and Nash, 1981). The suite of heavy minerals including zircon, rutile, and tourmaline indicates an acid igneous source for these sandstones. While the presence of rounded grains of rutile and zircon, is an indication of the reworked source for these sandstones. 5.4. Diagenetic sequence The role of diagenesis of the sandstones of the Kareem Formation was interpreted on the basis of pore geometry, size and filling material. The depositional environment, composition, textures, pore-fluid composition and migration and burial history are the main factors which affect the Kareem Formation diagenesis (Metwalli et al., 1987; Alsharhan and Salah, 1997). The main physical and chemical diagenetic processes have been identified as the following: Deposition of the Kareem Formation sands took place through rapid influxes of terrigenous material that was deposited on the neritic zone of the continental shelf. The sands were mildly compacted so that a fair proportion of the primary intergranular porosity was preserved, and some ductile components were slightly compressed. Compaction led to partial leaching of detrital grains. Sandstones are subjected to mechanical and chemical compactions during its progressive burial as evidenced from close packing of detrital framework which has caused a reduction in primary porosity of the sandstones (Fig. 4a and e). This compaction is also evidenced by concave–convex, sutured contacts of neighboring clastic grains (Fig. 4e) and a certain degree of stylolitization. The occurrence of chemical compaction is clear along detrital quartz grains. The presence of quartz fracturing (Figs. 4b and c and 7f) S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 and deformation of mud intraclasts provides evidence of mechanical compaction (Fig. 4f). The sandstones of the Kareem Formation were subjected to some mechanical compaction till carbonate cementation occurred which ceased the effect of mechanical compaction. However, mechanical compaction continued in sandstones with little or rare dolomite as indicated by their sutured and long grain contacts (Umar et al., 2011). Chemical compaction occurred by pressure dissolution both along intergranular contacts and fractures (Zhang et al., 2008). Feldspar dissolution is well recorded in some sandstone samples. This dissolution is due to relatively acidic conditions, in which the stability of feldspars is reduced. Dissolution appears to postdate compaction (Fig. 5c). This process caused a local increase in porosity. Iron-oxide cement occurs as a coating around detrital grains (Figs. 4b and c and 7d) and/or patches filling pore spaces in the sandstones of the Kareem Formation. It predates other diagenetic events, such as early silica and dolomite cement (Fig. 7d). The absence or weak coating at grain contacts suggests that the ironoxide mineral is of diagenetic origin, not an oxidized rim of detrital grains. It appears that, the hematite cement in the sandstones of the Kareem Formation may be derived in solution from iron rich minerals such as hornblende, pyroxene, olivine, magnetite, biotite and chlorite, which release their iron in sediments, under oxidizing diagenetic environment, the iron was precipitated as hematite or as goethitic precursor oxide and subsequently converted to hematite (Darwish and El-Araby, 1993). Authigenic silica is common in sandstones that lack early calcite and dolomite cements (Umar, 2007). The detrital core may be clearly outlined by dust rims. Quartz overgrowths engulf, and thus post-date, hematite (Figs. 4b and c and 7d), but are, in some cases, engulfed by, and thus predate, anhydrite and/or dolomite (Figs. 4b–d, 5d and e and 7c). The presence of authigenic clays modified the overgrowth habit of quartz (Rossi et al., 2002; Umar et al., 2011). Quartz overgrowth is partially replaced by later dolomite cement (Figs. 5e and 7c and f). The kaolinite exists as pore filling aggregates (Fig. 7e) postdates the quartz overgrowth phase (Umar et al., 2011). SEM analysis indicates that mixed layer clays (illite–smectite) post-date the quartz cementation (Fig. 7c). The precipitation of secondary silica was accompanied, and most probably succeeded by partial or complete dissolution of the carbonate fragments (Fig. 4f). The presence of silica overgrowths maintained the framework, so that the oversize pores left after the dissolution of the carbonate fragments were preserved (Fig. 4f). Carbonate cementation is represented by calcite and/or dolomite cements recorded in the quartzarenites, subarkose and arkose 47 of the Kareem Formation reflecting an increase in pH and/or temperature in the pore waters. The carbonate cements and pore-fills are mainly dolomitic (Figs. 4b–d, 5c and d and 7f). The ions required for ferroan dolomite cement formation were probably derived from alumino-silicate grain dissolution, and clay mineral transformation (Tucker and Wright, 1990). Cementation particularly by quartz and by dolomite prevented further significant compaction. Dolomite rhombs that found between the quartz grains cause close-packed textures (Figs. 5d and 7f) of crystal mosaics or isolated rhombs. The aggrading recrystallization of the primary dolomite is recorded in the studied sandstone types (Fig. 7a and b). Illite occurs as grain coating of detrital grains or pore filling cement (Fig. 7d). It is found mostly within the matrix and partly in pore spaces, and therefore the textural relationship with other authigenic mineral is not clear. For this reason, it is difficult to determine the relative time of illite authigenesis. Silica dissolution and replacement of quartz grains by calcareous cement was recorded in some samples (Fig. 5d). Silica dissolution and replacement by carbonate cements are controlled by changes in pH, partial pressure of CO, and temperature; they typically occur when the pore waters are under saturated with respect to carbonate (Pettijohn et al., 1987). This process leads to a decrease in sandstone porosity. The chemistry of the interstitial fluid grows strongly alkaline and unsaturated with silica; so the major parts of the silica overgrowths, and to a lesser extent, parts of the detrital quartz grains were dissolved. This process causes a local increase in porosity. Carbonate cements are partially leached (Fig. 5f) as the fresh water influx and the pore fluids were rendered acidic. As a result of dolomitization and expelling the excess calcium, a rise in the Ca/Mg ratio of the interstitial fluid happened and led to the precipitation of anhydrite both as pore filling (Fig. 4a and e) and as a replacement of dolomite (Fig. 5d). It is probable that a mixing with fresh water occurred at this phase supplying the sulfate ions (Tucker and Wright, 1990). Recrystallization of some anhydrite clasts took place most probably at this stage. Pyrite occurs in some sandstone samples and display typical euhedral shapes (Fig. 5f). Pyrite replaced other diagenetic minerals, indicating that it is the last diagenetic phase. 5.5. Paragenetic sequence The inferred paragenetic sequence of the sandstones of the Kareem Formation is shown in Fig. 16. The sandstones have undergone intense and complex episodes of diagenesis, including early and late diagenesis due to the influence of depositional environment, deep burial and uplift. The paragenetic sequence is inferred with respect to time by SEM, XRD and thin section study. Fig. 16. Paragenetic sequence of the sandstones of the Kareem Formation, Gulf of Suez. 48 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 During early diagenesis, minor amounts of pore-filling and replacement calcite and quartz overgrowths occurred. During burial, mechanical compaction started to reduce pore spaces. Compaction is documented by a tight grain supported fabric of sandstones. The compaction continued in all sandstones till the precipitation of massive carbonate (especially calcite) in some sandstones ceased further compaction and continued up to a late stage in sandstones with little carbonate cement. Mechanical compaction continued from early to late diagenetic stages. Mechanical compaction can be observed by a physical breakdown of feldspar grains (Fig. 5c). The dissolution and alteration of unstable grains such as feldspar and granitic rock fragments to kaolinite (Fig. 7e) was the second important diagenetic event in terms of relative timings. Partial kaolinitization of feldspar took place. The iron oxides were precipitated at the second diagenetic stage (Fig. 4b). Sources for iron oxide (hematite) cements might be the libration of iron by alteration of iron rich minerals such as hornblende, pyroxene, olivine, magnetite, biotite and chlorite. Chemical compaction was activated at this stage allowing pressure solution to provide the silica for quartz cementation. Quartz cement had started to precipitate in open pores before carbonate cementation. This is evidenced by the presence of well developed quartz overgrowths engulfed and corroded by dolomite cement (Figs. 4b and c, 5d and 7c). Quartz overgrowth is well developed and continued to late diagenetic stage in samples with little/or rare carbonate cement. The presence and growth of illite on kaolinite indicates its later origin than kaolinite (Fig. 7d). Also, rarely of mixed layer clays (illite–smectite) partially embedded and grown on authigenic silica indicates its later origin than quartz cementation. The precipitation of authigenic silica was predated partial or complete dissolution of the carbonate fragments as indicated by well preserved oversize (moldic and vuggy) pores left after the dissolution of the carbonate fragments (Fig. 4f). The carbonate cementation started slightly later than quartz cementation as indicated by euhedral quartz overgrowths which are embedded and partially replaced by dolomite (Fig. 4d). During the alteration and the dissolution of bioclastic shell fragments, Mg ions were librated and reacted to precipitate dolomite overgrowth on calcite cement (Fig. 4f). Illite may be formed diagenetically by a number of processes. The most important processes include replacement of feldspar and volcanic fragments particularly along thin cleavage planes and illitization of kaolinite (Fig. 7d). The late diagenetic events started by the dissolution and replacement of silica by carbonate cements (Figs. 4c and 5d). This process typically occurs when the pore waters are under saturated with respect to carbonate (i.e., the interstitial fluid is strongly alkaline) so the major part of the silica overgrowths, and to a lesser extent, parts of the detrital quartz grains were dissolved. Partial leaching of the carbonate cement occurred when the pore fluids were rendered acidic. Authigenic anhydrite typically occurs as pore filling and partially replaces dolomite cement (Fig. 5d). This indicates their later origin after dolomitization. Octahedral pyrite crystallites locally replace dolomite cement (Fig. 5f) and authigenic clays, indicating that it is the last diagenetic phase. It is probably formed during the sulfate reduction phase. The relative importance of compaction and cementation to destruction of porosity of sandstone, within the Kareem Formation is illustrated in Fig. 17, a Houseknecht plot (Houseknecht, 1987). The data shows a two-fold distribution. The majority of points plot in the cementation field, whereas a small clustered subpopulation apparently lost porosity by compaction. Much of the porosity within the clustered subpopulation is locally to severely enhanced by secondary dissolution. Alsharhan and Salah (1997) who studied the Kareem Formation, indicated the same causes of porosity reduction. They pointed out that primary porosity was originally much higher but has been greatly reduced by successive phases of cementation and mechanical compaction during diagenesis, and that porosity reduction continued due to mechanical compaction in sandstones with little or rare carbonate cement. The petrographic analyses reveal a number of controls on porosity development, which include the depositional controls (grain size, sorting, roundness, grain contact and grain density) and the diagenetic controls (cementation and compaction). The main controls on reservoir quality are carbonate and silica cement and total clay contents (Fig. 18). Petrographic examination of grain size, grain sorting and roundness against point counted porosity show positive correlations (Tables 1–4; Figs. 4b and c and 5c and d). However, these positive relations reveal that the overall porosity development is probably controlled by the interplay of cementation and secondary porosity creation. The study reveals that the porosity increases with samples of floating to point contacts (Fig. 4b and c) and decreasing with long, concave–convex and sutured contacts as shown in (Fig. 4e). A scatter plot of helium porosity and horizontal permeability against point counted porosity show a positive degree of association (Fig. 18a and b). Type and nature of cement and pore-occluding cement control on porosity development. A scatter plot of detrital and authigenic clay, authigenic quartz overgrowth; carbonate cement, anhydrite and other cement against point counted porosity show a poor degree of association (Fig. 18d–h). Dolomite cement is the strong control on porosity. Dolomite cement, especially the non-ferroan poikilotopic type, tend to sit in pores, blocking pores throats and so reduce permeability more than grain coating cements such as quartz. In the sandstones of the Kareem Formation, only samples with low dolomite cement contents have very high permeability values. Samples of less than Fig. 17. Houseknecht plot compaction and cementation versus porosity destruction of Kareem sandstones, Gulf of Suez. 49 B 25 r = 0.63 20 15 10 5 0 0 10 20 Pointed counted porosity (%) A Point counted porosity (%) S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 25 r = 0.49 20 15 10 5 0 30 0 500 25 D r = 0.5 20 15 10 5 0 2.6 2.65 2.7 2.75 2.8 r = 0.6 20 15 10 5 0 0 20 15 10 5 0 0.5 Point counted porosity (%) Point counted porosity (%) F r = 0.56 10 5 0 1.6 2 Other cement (%) point counted porosity (%) Point counted porosity (%) H 15 1.2 8 10 12 15 10 5 0 20 40 60 80 100 Total carbonate (%) 20 0.8 6 r = 0.55 0 r = 0.5 0.4 4 20 1 25 0 2 25 Quartz and feldspars overgrowth (%) G 2000 Detrital and authigenic clays (%) 25 0 1500 25 Grain density (gm/cm3) E 1000 Horizontal permeability (m.d) Point counted Porosity (%) C Pointed counted porosity (%) Helium Porosity (%) 25 r = 0.7 20 15 10 5 0 0 10 20 30 Anhydrite (%) Fig. 18. Relationships of helium porosity, horizontal permeability, grain density and different rock cements versus visual point counted porosity, Kareem sandstones, Gulf of Suez. 20% total carbonate generally have porosities greater than 12%, while samples possessing greater than 12% total carbonate have less than 10% porosity. The helium porosity values of cored intervals range between 6% and 30%, indicated poor to very good quality, while the horizontal permeability values of most samples range between 200 m.d and 2090 m.d, indicated good to excellent quality. The pore type and the main total porosity have been determined from petrographic and SEM studies in conjunction with conventional core analysis data. Three main pore types have been recognized in the core samples: (a) primary intergranular macropores, (b) secondary intragranular mesopores, and (c) insignificant intraparticle and intracrystalline micropores. Local occurrences of moldic, fractured and vuggy porosity greatly enhance the petrophysical properties of most samples. Pore interconnection is typically poor to good and may vary locally to be very good. Pores generally display irregular pore walls, as a result of common dissolution enlargement of pores. Occasional planar pore walls are associated with well developed quartz overgrowths. 50 S.M. Zaid / Journal of African Earth Sciences 85 (2013) 31–52 6. Conclusions The Middle Miocene Kareem sandstones served as one of the primary source of oil and gas in the southwestern part of the Gulf of Suez including Zeit Bay Oil Field and East Zeit Oil Field. The Kareem Formation disconformably overlies the Rudies Formation and unconformably overlies by the Belayim Formation. The sandstones of the Kareem Formation are mostly quartzarenites with subordinate subarkoses and arkoses. Quartzarenites present in the Lower Kareem Rahmi Member where the subarkoses and arkoses recorded only in the Upper Kareem Shagar Member. Dolomite, calcite, anhydrite and pyrite are important accessory authigenic and detrital components. In The Lower Kareem, sandstones are mature and derived from craton interior to transitional continental setting (i.e., sandstones were transported from the far along the rift). This indicated by the low percentage of unstable grain such as feldspar <4% and other rock fragments <2%, the dominance of monocrystalline quartz, and most of feldspar grains altered. However, the Upper Kareem sandstones are derived from craton interior, transitional continental and recycled orogenic setting. The high percentage of unstable grain >15%, indicate that the Upper Kareem sandstones show short transport distance and quick burial. This means that the Upper Kareem sandstones are typically rift sandstone and their deposition constrained the beginning of the faulting in the studied area. The sandstones of the Kareem Formation show upward decrease in alteration (CIA and CIW) and also show upward decrease in maturity (MI). These relationships may reflect that the chemical composition may be correlated, to a great extent, with the petrographic modal data. Petrographic analyses reveal a number of controls on porosity development, which include both textural and mineralogical factors. Grain size, grain sorting and roundness against point counted porosity show positive correlations. However, these positive relations reveal that the overall porosity development is probably controlled by the interplay of cementation and secondary porosity creation. The study also reveals that the point counted porosity is directly proportional to helium porosity, horizontal permeability and connectivity, but it inversely proportional to grain density. Sandstone reservoir quality is largely determined by diagenetic processes that either reduce or enhance porosity. The most important diagenetic processes in the sandstones of the Kareem Formation are compaction, cementation by dolomite, calcite, quartz, anhydrite, clays, and iron oxide. Compaction, both mechanical and chemical, has a large influence on the intergranular volume. The intergranular volume is partly correlated to the amount of diagenetic carbonates, indicating that porosity reduction continued in sandstones with little or no carbonate cement, whereas massive cementation by dolomite prevented later compaction and preserved a larger intergranular volume. Mechanical compaction and authigenic cements reduce the porosity and permeability, whereas dissolution of unstable clastic grains and soluble cements increase porosity in sandstone. The present porosity of sandstone varies from 6% to 30% with an average of 18%. The primary porosity of the sandstones is reduced due to intense mechanical compaction and due to filling of early authigenic cements such as carbonate, quartz, clay minerals and iron oxides. The successive burial was responsible for the reduction in porosity due to compaction as indicated by long and sutured contact between neighboring clastic grains. In some samples, the early carbonate cement reduced or prevented further compaction and the resulting close packing of clastic grains. Authigenic kaolinite and iron oxide also played an important role in the preservation of porosity. Kaolinite and mixed layer clays have reduced the permeability but preserve porosity as intercrystalline porosity. Grain-coating rims of iron oxide in some cases prevented the formation of quartz overgrowths and thus preserved porosity. The dissolution of unstable clastic grains began in the early stages of diagenesis which produced an empty pore volume for secondary cementation. Some pores were protected by clay and/ or iron oxide coats and remained open. Another episode of dissolution occurred in the late stages and dissolved authigenic minerals, mainly carbonates, thus producing secondary porosity. Dolomite and ferroan dolomite cements are the strong control on porosity. Samples of less than 20% total carbonate generally have porosities greater than 12%, while samples possessing greater than 12% total carbonate have less than 10% porosity. Petrophysically, the reservoir quality of the Kareem Formation is locally moderate- to good. Porosity types are dominated by primary interparticle forms and secondary intragranular and insignificant intraparticle and intracrystalline micropores. 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