Zircon U–Pb, molybdenite Re–Os and muscovite Ar–Ar isotopic dating of the Xitian W–Sn polymetallic deposit, eastern Hunan Province, South China and its geological significance
Graphical Abstract
Introduction
China ranks first in the world in terms of tungsten resources and reserves, and has some of the largest tungsten deposits. According to the mineral commodity summaries of the United States Geological Survey (USGS, 2016), China has more than 57% tungsten reserves of the world, and yielded more than 81% of the world’s total tungsten production in 2015. The Nanling region in the central part of South China accounts for more than 92% of the Chinese tungsten resource; thus it is the most important Tungsten–Tin (W–Sn) polymetallic province, and it has a close spatial relationship with the Yanshanian granites (Hsü, 1943, Lu, 1986, Mao et al., 2013a, Mao et al., 2013b). Several large-scale W–Sn polymetallic deposits are distributed within the Nanling region, such as the Shizhuyuan, Furong, Yaogangxian, Xihuashan, and Pangushan deposits (Fig. 1). The Shizhuyuan deposit is the largest among the economically important skarn-, greisen- or vein-type W–Sn polymetallic deposits in South China (Mao and Li, 1995, Mao et al., 1995, Mao et al., 1996a, Mao et al., 1996b, Zaw et al., 2007, Yin et al., 2002). It mainly occurs at the contact between the Late Devonian dolomitic limestone and the Late Jurassic (Yanshanian) granitoid, with 750, 000 t WO3, 490, 000 t Sn, 300, 000 t Bi, 130, 000 t Mo and 200, 000 t Be (Lu et al., 2003). Mining activities have been carried out in the Nanling region for several tens of years, but there remains an untouched reserve of 1.7 million tons of tungsten and 1.2 million tons of tin (Che et al., 2005, Peng et al., 2006, Zaw et al., 2007, USGS(United States Geological Survey), 2016).
The Xitian W–Sn polymetallic deposit in eastern Hunan Province is one of the largest newly-discovered deposits during the latest phase of exploration (1999–2011) in the Nanling region, an area with a great potential for W and Sn resources (Wu et al., 2004, Fu et al., 2009, Fu et al., 2012) (Fig. 2). It has four types of mineralization; these are skarn-type hosted at the contact zone between the Yanshanian granite pluton and the Devonian dolomitic limestone, and greisen- and vein-types, as well as structurally altered rocks within or near the Yanshanian granite. The deposit has a Sn reserve of 586,000 tonnes with a grade of 0.26–0.36% and a W reserve of 46,300 tonnes with a WO3 grade of 0.28–0.63% (Mao et al., 2013a). In addition, Pb, Zn, Mo, Nb and Ta are the by-products from the mineralization (Wu et al., 2004, Luo et al., 2005).
Numerous field investigations, together with geochemical, geochronological, and isotopic studies have been sporadically carried out in the area of the Xitian deposit since 1999 and reported in the Chinese literature (Luo et al., 2005, Ma et al., 2005, Zeng et al., 2005, Cai and Jia, 2006, Xu et al., 2006, Chen et al., 2013, Zhou et al., 2013, Niu et al., 2015, Deng et al., 2015). Various geochronologic techniques have been adopted in the studies, including the K–Ar, Rb–Sr, Sm–Nd isochrons, and LA-ICPMS, SHRIMP, and SIMS zircon U–Pb. However, the lack of systematic application of modern techniques has resulted in a limited consensus on the exact timing of the granitic intrusion, although it has been tentatively dated between 175-161 Ma by regional petrographic correlation (HNBGMR, 1988). The intrusion has been subdivided into two stages, 233–227 Ma and 155–150 Ma (Ma et al., 2005, Niu et al., 2015, Su et al., 2015), and three stages, at ~ 230 Ma or Indosinian, at ~ 155 Ma or Early Yanshanian, and ~ 114 Ma (Whole rock Rb-Sr dating) or Late Yanshanian (Chen et al., 2014, Fu et al., 2009). How the Xitian deposit relates to these stages is a matter of debate. A combination of molybdenite Re–Os, muscovite Ar–Ar, and fluid inclusion Rb–Sr dating (Liu et al., 2008a, Liu et al., 2008b, Fu et al., 2009, Fu et al., 2012, Wu et al., 2012, Wang et al., 2015) has yielded an age of 157–150 Ma or Late Jurassic for the deposit. However, Niu et al. (2015) argued the presence of another mineralization in 227–233 Ma, and Deng et al. (2015) even obtained a molybdenite Re–Os age of 225.5 ± 3.6 Ma. It is therefore necessary to undertake a systematic study to date the deposit and the adjacent granite to resolve this conundrum.
This paper aims to accurately date the Xitian W–Sn deposit and the associated granites. Zircon U–Pb, molybdenite Re–Os and muscovite Ar–Ar isotopic dating, together with field, petrographic and geochemical studies, have rigorously been carried out in these years. These data confirm the two stages of the Xitian granitic intrusion and, what is more, the temporal relationship between the deposit and the Early Yanshanian magmatism. This is helpful in better understanding the W–Sn mineralization of the Nanling region. The new data are combined with recently published geochronology of other W–Sn deposits in the Nanling region to accurately and precisely constrain the timing of mineralization and to identify the geodynamic processes that contraolled the metallogenesis.
Section snippets
Regional geology
The South China Block (SCB) is composed of the Yangtze Block (YZB) to the west and the Cathaysian Block (CAB) to the east (Fig. 1a), which amalgamated during the Neoproterozoic Sibao (also called “Jiangnan” or “Jinning”) orogeny (Chen and Jahn, 1998, Li, 1998a, Li, 1998b, Zhao et al., 2011). The YZB comprises Neo-Archean metamorphosed basement, sporadically exposed in Yunnan, Guizhou, and Hubei provinces (Gao et al., 1999, Qiu et al., 2000, Charvet, 2013). The CAB is composed of Proterozoic
Geology of the Xitian deposit
The Xitian W–Sn polymetallic deposit is located within the Chaling–Chenzhou deep fault, a major regional-scale structure, whose activity is presumably related to the formation of the deposits (Wang et al., 2003a, Wu et al., 2004) (Fig. 1b). It is an S–N-trending extensional granite dome, surrounded by Paleozoic sedimentary rocks that were deformed into a series of NE-trending folds and NE- or NEE-trending strike-slip faults (Wu et al., 2012). These folds with a steeply NE-dipping axial plane
Zircon U–Pb dating
Two samples were chosen for U-Pb dating. The sample from drill core ZK50901-1 is a coarse-grained porphyritic biotite K-feldspar granite (Fig. 3a) and the sample from ZK14B04-2 is a fine-grained porphyritic biotite granite (Fig. 3c). The first sample was collected at a depth of 250-253 m in the Shaiheling mining district (Fig. 2), and the second sample at a depth of 198-200 m in the Longshang mining district (Fig. 2, Fig. 4).
Zircons were separated by conventional heavy liquid and magnetic
Zircon U–Pb ages
Zircon CL images of the Xitian granite are displayed in Fig. 5. In the images, most of the zircons are transparent, euhedral and prismatic, and have an oscillatory zoning or linear zoning, diagnostic of magmatic origin (Corfu et al., 2003). They are generally colorless or light brown and 80–270 μm long, with a length/width ratio of 1.1–2.6.
For sample ZK50901-1, a number of 20 spots were carried out on twenty zircons (Table 1). Only spot ZK50901-1-10 was excluded for its low (< 90%) concordance
Re contents and origin of ore metals
The Re–Os isotope system has been recognized as a possible geochemical tool for not only directly dating mineralization but also tracing the source of metals (Stein et al., 1997, Stein et al., 1998, Ruiz and Mathur, 1999, Wang et al., 2011a, Wang et al., 2011b, Li et al., 2007a, Li et al., 2014b). Comparing Re contents in molybdenite from various types of endogenous Mo deposits in China, Mao et al. (1999) recognized that Re in molybdenite varies in content from hundreds (a mantle source) to
Conclusions
Dating of the Xitian W–Sn polymetallic deposit in eastern Hunan Province using Re–Os molybdenite, Ar–Ar muscovite and LA-ICPMS U–Pb zircon techniques enables us to draw the following conclusions:
- 1)
Molybdenites in ore-bearing quartz veins of the Xitian deposit are characterized by a relatively variable Re content, 8.7–44.0 ppm, with an average of 30.5 ppm, indicating that the ore-forming materials were derived from the mixed mantle and crustal sources.
- 2)
LA-ICPMS zircon U–Pb dating yields a
Acknowledgements
This work was financially supported by the Public Scientific Research Project of Ministry of Land and Resources of China (201211024-03) and National Natural Science Foundation of China (Nos. 41576040, 40872080 & 41072081). The authors are indebted to Y. L. Sun, Y. Liu and G. Q. Hu for their help with sample analysis. Dr Susan Turner and two reviewers (Prof. J. W. Mao, and Dr. C.L. Guo) are thanked for science and English language improvements of the original and revised manuscripts. Special
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