Metallogenesis and depositional environment of the Archean-Proterozoic carbonaceous phyllites from the Dharwar Craton, India
Graphical abstract
Introduction
Carbonaceous phyllites are distributed all around the world with wide range of depositional regimes in the stratigraphic record (Tourtelot, 1979, Eric et al., 2019). These organic carbon rich meta sedimentary rocks serve as tools to understand the global biogeochemical cycles and are also used to interlink geological events such as hydrothermal activity and marine anoxia (Schieber, 2011, Fakhraee and Katsev, 2019). Some beds of black shale contains minor elements in concentrations more than a hundred times their average crustal abundance (Krauskopf, 1955). During the cycles of weathering and erosion of the earth's surface some minor elements as well as sulfide tend to remain in resistant minerals that are transported to sedimentary basin. They are generally characterized by enrichment of redox sensitive trace elements and have potential metal resources such as PGE and gold (Pages et al., 2018, Khanchuk et al., 2018). Kotov et al. (1993) have suggested a two-phase development with syn-tectonic hydrothermal remobilization of Au from the black shales. Carbonaceous sequences often accommodate large gold deposits, such as Muruntau (central Uzbekistan), Bakyrchik (eastern Kazakhstan), Kumtor (Kyrgyzstan), and Sukhoi Log (Russia; Yermolaev et al., 1995). These stratiform deposits occur in carbonaceous shales containing fine-grain carbon of mainly biogenic origin as well as chemogenic origin (Laverov et al., 2000, Vinokurov et al., 1997). The presence of carbonaceous shales all along the geological time scale indicates that the geological processes played a prominent role in their deposition rather than the geological setting (Tourtelot, 1979). As these rocks show conspicuous confinement to ocean anoxia, they provide reliable insights into the microbial life and paleo-redox conditions that prevailed during the Precambrian (Marin-Carbonne et al., 2020, Jørgensen et al., 2019). Precambrian carbonaceous shales are characterized by enrichment of precious metals like gold and PGE while those of Phanerozoic have high hydrocarbon potential (Ohkouchi et al., 2015, Baioumy et al., 2018). The occurrence of carbonaceous shales in the sedimentary basins of India have been reported by many workers viz. Sandur greenstone belt (Manikyamba and Kerrich, 2006), Singhbhum Craton (Majumdar et al., 2019), Cuddapah Basin (Manikyamba et al., 2008, Basu et al., 2017), Vindhyan Basin (Paikaray et al. 2008), Krishna–Godavari Basin (Rao, 2001); Damodar Valley (Mani et al., 2015), Cambay Basin (Bhaskar, 2013), Kachchh Basin (Srivastava et al., 2018) and Mizoram Basin (Sawant et al., 2017). Though many workers have conducted extensive studies on these shales, reports on the Archean and Proterozoic shales of India are very meagre. In the present paper, we report the gold, PGE and δ34S concentrations of carbonaceous phyllites from Archean Chitradurga, Gadag greenstone belts and Proterozoic Cuddapah basin to document the role of organic matter during the metallogenesis and deposition. As Precambrian era is intrinsically characterized by the rise of atmospheric oxygen i.e., Great Oxidation Event (GOE), the study of Archean and Proterozoic carbonaceous phyllites is vital to understand and decipher the Precambrian biogeochemical conditions.
Section snippets
Dharwar Craton
Dharwar Craton of southern peninsular India is one of the largest cratons around the globe covering an area of about 4.5 × 105 km2 and possesses ubiquitous occurrence of greenstone belt sequences ranging in age of 3.4 to 2.5 Ga, volcano-sedimentary sequences and TTG-granitoids (Manikyamba and Ganguly, 2020, Pahari et al., 2020) . This craton has been divided into western and eastern sectors by the Closepet granite based on the lithological association of greenstone belts, grade of metamorphism
Sampling and analytical techniques
Unweathered samples of carbonaceous phyllites were collected from fresh outcrops for the present study. Among twenty-seven samples, five are from G. R. Halli area (N14°17′27.49″, E76°24′21.53″) of Chitradurga greenstone belt, fourteen are from Kabulayankatti (N15°17′49.42″, E75°38′45.34″) of Gadag greenstone belt and eight samples are from Mangampeta (N14°10′14.64″, E79°19′23.14″) of Cuddapah Supergroup (Fig. 1). In Chitradurga (CCP; Fig. 2A-B) and Gadag carbonaceous phyllites (GCP; Fig. 2C-D),
Ore petrography and mineral chemistry
The carbonaceous shales collected from the studied rocks show predominance of quartz, albite and micaceous minerals such as muscovite, illite which occur as thin laminations associated with jet-black coloured carbonaceous matter. Pyrite is the most common sulphide mineral in all the samples, occurs as individual grains and also in association with other sulphide minerals. The Chitradurga carbonaceous phyllites are characterized by abundance of pyrite which is present in the quartz-veins (Fig. 3
Pyrite chemistry - genetic implications of refractory gold
Pyrite is an ubiquitous sulphide in hydrothermal system and important repository of many precious metals including gold and PGE (Meng et al., 2020, Tang et al., 2019, Voute et al., 2019). Textural and chemical characterization of pyrites including trace element studies, provide significant insights into the metallogenesis as well as the paleo-redox conditions (Parnell et al., 2018). Based on the textural evidences, pyrite microcrystals (Py-I) of Chitradurga and Gadag occur sporadically within
Conclusions
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The Archean carbonaceous phyllites show enrichment of gold and PGE concentrations compared to the Proterozoic carbonaceous shales. The Chitradurga carbonaceous phyllites have high concentrations of gold (avg. Au = 180 ppb) compared to those of Gadag (avg. Au = 38 ppb) and Mangampeta (avg. Au = 23 ppb). Contrarily, the PGE concentrations in Gadag are comparatively higher (ΣPGE = 55 ppb) than Chitradurga (ΣPGE = 37 ppb) and Mangampeta (ΣPGE = 27 ppb)
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Gold and PGE mineralization in the Archean and
Declaration of Competing Interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Acknowledgements
The authors thank Dr V.M. Tiwari, Director, CSIR‐NGRI, for permitting to publish this work. C.M. acknowledges the funds provided from Council of Scientific and Industrial Research (CSIR) to National Geophysical Research Institute, Hyderabad, through the projects of the CSIR-Emeritus Scientist, INDEX project and Ministry of Earth Sciences (MoES/PO (Geosci)/8/2014. The authors thank Prof. Franco Pirajno for efficient editorial handling and two anonymous reviewers for their valuable and
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