Elsevier

Ore Geology Reviews

Volume 127, December 2020, 103815
Ore Geology Reviews

Genesis of the Kangshan Au-polymetallic deposit, Xiong’ershan District, North China Craton: Constraints from fluid inclusions and C-H-O-S-Pb isotopes

https://doi.org/10.1016/j.oregeorev.2020.103815Get rights and content

Highlights

  • The ore-forming materials and fluids of the Kangshan deposit might be magmatic source.

  • The Kangshan deposit is a moderate-low temperature hydrothermal Au-polymetallic deposit.

  • The Kangshan deposit may formed in an extensional setting related to craton destruction.

Abstract

The Kangshan Au-polymetallic deposit, in the Xiong’ershan District of China, lies on the southern margin of the North China Craton. The orebodies are hosted in (E)NE–(W)SW-trending brittle faults formed during the Mesozoic, which crosscut Neoarchean metamorphic rocks and Mesoproterozoic volcanic rocks. The ore-forming process can be divided into three stages: a quartz ± pyrite stage (Stage 1), a quartz-polymetallic sulfide stage (Stage 2), and a quartz-calcite stage (Stage 3). Stage 2 includes two substages: a quartz-pyrite-chalcopyrite-electrum substage (Stage 2-1; the main Au mineralization stage) and a galena-sphalerite-pyrite-ankerite-Ag-bearing tetrahedrite ± chalcopyrite ± electrum substage (Stage 2-2; the main Pb-Zn-Ag mineralization stage). Four types of fluid inclusions have been identified in the Kangshan deposit: three-phase CO2-rich inclusions, two-phase aqueous inclusions, one-phase vapor inclusions and one-phase aqueous inclusions. Inclusion microthermometric, laser Raman, and C-H-O-S-Pb isotope analyses were undertaken to clarify the properties of the ore-forming fluids, sources of these fluids and ore-forming materials, and mineral precipitation mechanisms. Laser Raman spectroscopic analysis indicate that the ore-forming fluids were formed in a NaCl-H2O-CO2 system. Inclusion homogenization temperatures and salinities are 130 °C–359 °C, and 0.53–11.46 wt% NaCl equivalent (eqv.), respectively. δ18Ofluid values calculated from the δ18OSMOW and δD values of the inclusions in auriferous quartz veins are 1.0–9.0‰ and -92‰ to -67‰, respectively. δ13CPDB and δ18OSMOW values of ankerite are -4.89‰ to -3.67‰ and 12.0‰–13.9‰, respectively. Fluid C-H-O isotopic compositions indicate that the ore-forming fluids originated mainly from magmas, with minor addition of meteoric water. δ34S values of the ore sulfides are 4.8‰–7.4‰; 206Pb/204Pb, 207Pb/204Pb, and 208Pb/204Pb ratios of the ore sulfides are 17.625–17.889, 15.543–15.620, and 38.389–38.740, respectively. S-Pb isotopic compositions indicate that the ore-forming materials of the deposit originated from granitic magmas and host rocks. The Kangshan Au-polymetallic deposit is a medium–low-temperature hydrothermal deposit. Its mineralization may be related toEarly Cretaceous granite formed in an extensional tectonic setting caused by craton destruction on the southern margin of the North China Craton.

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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