Genesis of the Kangshan Au-polymetallic deposit, Xiong’ershan District, North China Craton: Constraints from fluid inclusions and C-H-O-S-Pb isotopes
Graphical abstract
Introduction
The Xiong’ershan District (XD), in the middle of the Eastern Qinling Metallogenic Belt (EQMB), lies on the southern margin of the North China Craton (NCC). The XD is an important Au-producing area of China (Mao et al., 2002). To date, two types of Au-polymetallic deposit have been described in the XD: magmatic-hydrothermal and orogenic deposits, distinguished mainly by H-O-S-Pb isotopic compositions, ore-forming fluids, and mineralization ages. Magmatic-hydrothermal deposits are considered to have formed during a craton-destruction event in the Early Cretaceous ( Mao et al., 2002, Han et al., 2007, Gao et al., 2011, Zhai et al., 2012, Li et al., 2013b, Tang et al., 2013, Tang, 2014, Zhu et al., 2015, Tian et al., 2017, Zhang et al., 2018, Zhang et al., 2019), while orogenic deposits generally formed during the Triassic, apparently in association with the collision between the NCC and Yangtze Craton (YC) (Chen et al., 2004, Chen et al., 2006, Chen et al., 2008, Tang, 2014, Zhou et al., 2018a).
The Kangshan Au-polymetallic deposit is hosted in Neoarchean Taihua Group metamorphic rocks and Mesoproterozoic Xiong’er Group volcanic rocks. Controversy remains concerning the genesis of the Kangshan deposit: whether it is a magmatic-hydrothermal deposit (Fan et al., 1994a) or an orogenic Au deposit (Wang et al., 2001). Fan et al. (1994a) considered that the ore-forming fluids were magmatic-hydrothermal fluids, with ore-forming materials being derived from the Taihua Group; Wang et al. (2001) considered that the ore-forming fluids were metamorphic-hydrothermal fluids, with the ore-forming materials being derived from subducting slabs. Study of the Kangshan deposit continues with the aim of clarifying these issues.
Here we present new fluid inclusion and C-H-O-S-Pb isotopic data for the Kangshan Au-polymetallic deposit, which we use to trace the sources of ore-forming fluids and materials, and clarify the origins of the deposit.
Section snippets
Regional geology
The EQMB lies on the southern margin of the NCC (Fig. 1A) and has a complex multi-stage orogenic history (Meng and Zhang, 2000, Zhang et al., 2001, Dong et al., 2011). Strata in the EQMB comprise the Neoarchean Taihua, Mesoproterozoic Xiong’er and Guandaokou, and Neoproterozoic Luanchuan groups (Fig. 1B). The Taihua Group (2.8–2.6 Ga) comprises mainly metamorphic rocks, including gneiss, marble, quartzite, and amphibolite (Kröner et al., 1988, Xue et al., 1996). The Xiong’er Group (1.8–1.4 Ga)
Strata
The Kangshan deposit lies in the southwestern XD (Fig. 1B). Strata in the ore area include the Neoarchean Taihua and Mesoproterozoic Xiong’er groups, with some Quaternary strata distributed in valleys (Fig. 2). Au-polymetallic mineralization is hosted in the Neoarchean Taihua and Mesoproterozoic Xiong’er groups.
Structures
Faults are widely distributed in the Kangshan deposit, the largest of which is the Sanmen-Lingtai Fault (Fig. 2), which is the northernmost fault of the Machaoying Fault Zone. It is
Samples
Samples were collected from tunnels and outcrops in the Kangshan deposit. Doubly polished thin-sections (0.2 mm thick) were made from auriferous quartz veins and altered wall-rocks for petrographic study of compositions, textures, structures, and spatial distributions of minerals. Fluid inclusions microthermometric and vapor-phase laser Raman spectroscopic analyses were undertaken on 12 and 6 typical sections, respectively. Isotopic analyses were undertaken on 9 sulfide samples for S isotopes
Petrography
Fluid inclusions are widely developed in quartz veins of each ore-forming stage. Most are isolated or randomly clustered primary inclusions, with fairly regular shapes (polygonal, oval, or semicircular) in a size range of 3–15 μm (Fig. 8). Secondary and pseudo-secondary inclusions occur as intergranular arrays or aligned along microfractures in transgranular crystal trails (Roedder, 1984, Lu et al., 2004). Here we focus on the primary inclusions (Fig. 8), of which there are four types in the
Source and evolution of the ore-forming fluids
δD and δ18Ofluid values of quartz veins from the different hydrothermal stages are shown in Fig. 12, where Stage 1 values plot in or near the magmatic field. δ18Ofluid values gradually decrease over the later stages, suggesting a continuous influx of meteoric water during ore-formation.
δ13CPDB and δ18OSMOW values of ankerite formed in Stage 2-2 are shown in Fig. 13, where δ13CPDB values (-4.89‰ to -3.67‰) plot within the range of magmatic and mantle C (from -5‰ to -2‰, Taylor, 1986), suggesting
Conclusions
- (1)
Ore-forming fluids of the Kangshan Au-polymetallic deposit were formed in a moderate-low temperature, NaCl-H2O-CO2 magmatic-related system. Fluid immiscibility was the main process involved in Au precipitation, and fluid mixing in Pb-Zn-Ag precipitation.
- (2)
Mineral C-H-O isotopic compositions indicate that the ore-forming fluids were derived mainly from magmatic fluids; S-Pb isotopic compositions indicate that the ore-forming materials may have originated from the magmas and host rocks.
- (3)
Geological
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
This work was financially supported by the National Key R & D Program of China (Grant No. 2016YFC0600109), and the State Key Laboratory of Lithospheric Evolution, IGGCAS (SKL-Z201905). We are indebted to all the geologists and staffs of the Kangshan Gold Mine for their hospitable assistance. We grated the kind help of He Zhang from the CUGB on the fluid inclusions microthermometric measurements, Mu Liu from the BRIUG on the Pb isotopic analysis. We appreciate Liangliang Huang for assistance of
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