Abstract
The mechanisms responsible for invisible gold enrichment driven by coupled dissolution-reprecipitation reaction (CDR) are debated. Here we report the micro- to nano-scale textures of arsenian pyrite in a high-grade (>10 g/t) gold ore from the Chang’an deposit to trace the gold enrichment process. Our study records a CDR-driven evolution of mineral growth from an As-rich, Au-poor pyrite core, with numerous fine arsenopyrite inclusions, to an inclusion-free, As-Au-rich oscillatory pyrite rim. The reaction occurred at ~260 °C under 4.7 to 5.8 pH and –36.6 to –32.9 logfO2 conditions. The elevated As but depleted S contents in the pyrite core indicate a combined elevation of S fugacity and solubility of Au. The coprecipitation of arsenopyrite inclusions in the core caused a depletion of S fugacity to –13.8 ~ –11.7, triggering Au enrichment in the rim. This non-unique process has the potential to explain the upgrade of invisible Au in arsenian sulfides, worldwide.
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Introduction
Gold in hydrothermal deposits occurs in a variety of forms including as native Au grains and invisible Au in arsenian sulfides1. Invisible Au consists of either disseminated atoms in the crystal lattice, nanoparticles, or decorates crystal defects in arsenian pyrite and arsenopyrite1,2,3,4,5,6,7. The extraordinary enrichment of visible Au, involving transportation, flocculation, and coarsening, has been well studied8,9,10,11,12, whereas that of invisible Au is debated due to the complex interaction of fluid physicochemical conditions and crystal growth processes. Incorporation of invisible Au into arsenian pyrite and arsenopyrite has commonly been suggested to be associated with growth kinetics of pyrite13,14, crystal defects induced by As incorporation4,15, and electrochemistry of crystal-fluid interfaces16,17,18. The liberation of invisible Au from arsenian sulfides has been attributed to a coupled dissolution-reprecipitation reaction (CDR)13,19,20,21,22,23. However, the mechanism of invisible Au enrichment driven by the CDR of arsenian pyrite are poorly understood. These puzzles are partly due to the lack of micro- to nanoscale data illustrating the mechanisms operating at the boundaries between Au-poor and Au-rich pyrite and between inclusions and host pyrite.
Here we present the micro- to nano-scale texture of arsenian pyrite in a high-grade ore (>10 g/t) from the Chang’an epizonal orogenic gold deposit (>30 t Au; Fig. 1a)24. Mineralogical and geochemical evidence and thermodynamic modeling are presented to trace the growth processes of pyrite and the fluctuation of physicochemical conditions driven by CDR.
This study depicts a detailed evolution of mineral growth from As-rich, Au-poor pyrite core with numerous inclusions of arsenopyrite, to an inclusion-free, As-Au-rich pyrite rim. Fluctuation of physicochemical conditions controlled the release, remobilization, and reprecipitation of invisible Au into the pyrite rim.
Geological setting
The Chang’an gold deposit occurs in the southern segment of the Cenozoic Ailaoshan Orogen, the youngest orogenic gold belt globally25, located along the southeastern margin of the Tibetan Plateau26,27,28 (Supplementary Fig. 1a). The main sedimentary units at Chang’an comprise an Ordovician turbidite package and Silurian dolostone (Fig. 1a; Supplementary Fig. 1b). The Ordovician turbidite package comprises a thick sequence of sandstone with minor thin layers of carbonaceous and calcareous sandstone, siltstone, mudstone, and conglomerate, among which the sandstone is the main host for the gold orebodies24,27. A series of ~35 Ma lamprophyre dikes and alkali-rich porphyry intrusions occur in the Chang’an gold deposit (Fig. 1a; Supplementary Fig. 1b)27. The gold orebodies which cross-cut the dikes are controlled by the NW–SE-trending Chang’an Fault (Fig. 1a; Supplementary Fig. 1b) and are discontinuous over 1.8 km along strike and 20–253 m down dip with an average grade of 4.54 g/t24. The crosscutting relationships the inferred stress field, and published paleomagnetic evidence, in combination, suggest that the Chang’an deposit most likely formed at ~23–21 Ma27,29,30. Geological characteristics at Chang’an include: (1) proximity to the major lithospheric-scale Ailaoshan shear zone, but ore zones hosted in second- or third-order Chang’an Fault; (2) gold-related alteration dominated by silicification, sericitization, sulfidation, and carbonation (Fig. 1b–d); and (3) lack of lateral metal zoning24,26,27. These features are compatible with those of orogenic gold deposits proposed by ref. 31, but differ from the extensional structures and ore textures of epithermal and Carlin-type gold deposits, as summarized by ref. 24.
Results
Pyrite texture and gold occurrence
The high-grade (>10 g/t) gold ores have a mineral assemblage of pyrite, arsenopyrite, galena, and sphalerite with minor native Au (Fig. 2a–f). The pyrite in the high-grade ores comprises commonly an As-rich core that contains fine-grained and numerous inclusions of arsenopyrite, sericite, galena, chalcopyrite, and native Au, and inclusion-free rim (Fig. 2a–f; Supplementary Fig. 2a–g). The pyrite rim is characterized by As oscillatory zoning (Fig. 2a–c). In localized domains, the oscillatory As zoning is dissected by As-poor pyrite domains associated with arsenopyrite inclusions (0.1–5 μm; Fig. 2b). The pyrites from proximal to distal quartz-ankerite veinlet show a decline in arsenopyrite inclusions and thickness of pyrite rim (Fig. 2a–c). The ToF-SIMS analysis of pyrite grains with core and rim textures shows that the inclusion-rich pyrite core has high As contents relative to its rim and that Au is concentrated in the As-depleted, inclusion-free pyrite rim (Fig. 3a, b).
Crystal relationship of fine-grained inclusions with host pyrite
The EBSD analysis reveals that the pyrite core and rim have similar crystallographic orientation (Fig. 3c–e). The analyzed pyrite has low-angle boundaries (<6° misorientation; Fig. 3e), which show no evidence of microfractures, indicating the coherent nature of the microstructure. The distribution of arsenopyrite inclusions is poorly correlated to the low-angle boundaries (white lines; Fig. 3e). Pole Figures. of the {100}, {110}, and {111} crystal faces of arsenopyrite inclusions and its host pyrite show similar preferred crystallographic orientation (Fig. 3f, g).
Geochemical composition of arsenopyrite
The EMPA shows that the fine-grained and anhedral arsenopyrite inclusions in the pyrite core have an atomic As concentration that range between 25.6% and 28.5% (median 27.7%; n = 40), with corresponding variations in S content of 37.7–42.3% (median 38.7%) and Fe content of 31.1–34.3% (median 33.6%; Supplementary Table 1). In contrast, the As, S, and Fe concentrations in coarse-grained and euhedral arsenopyrite intergrown with pyrite range from 26.4% to 30.6% (median 28.9%; n = 11), 36.1–41.1% (median 37.5%) and 33.2–33.8% (median 33.4%; Supplementary Table 1), respectively. There is an antithetic correlation between As and S (R2 = 0.95), indicating a coupled substitution within arsenopyrite, compatible with experimental studies32.
Nano-scale texture and elemental mapping of pyrite
The high-angle annular dark field-scanning TEM (HAADF-STEM) analysis of the TEM foil identified a bright pyrite core with several bright arsenopyrite sub-micrometer particles and relative dark rim with few sub-micrometer particles (Fig. 4a; Supplementary Fig. 2a). The SAED patterns and high-resolution TEM (HRTEM) images of the pyrite core and rim indicate that they have coherent crystal lattice (Fig. 4b, c), but that the pyrite core is characterized by abundant stacking faults relative to the pyrite rim, as shown by the HAADF-STEM image (Fig. 4a). The arsenopyrite particles with 50 nm to 1.5 μm diameter are located along the microfractures and/or voids of the pyrite core (Fig. 4a, c; Supplementary Fig. 2d–f) and host coherent crystal lattice with the pyrite core (Fig. 4d). The HAADF-STEM image and corresponding EDS maps show that the pyrite core has heterogenous Fe and As contents but that the pyrite surrounding a sericite inclusion has a high As content, but low Fe and S contents (Fig. 4e, f).
Discussion
Genesis of pyrite texture
The fine-grained and numerous arsenopyrite, galena, chalcopyrite, and native Au inclusions in arsenian pyrite from the Chang’an gold deposit can be attributed to post-crystallization exsolution of solid solution from metastable arsenian pyrite2,33 or fluid-mediated CDR20,21. If the former is correct, stacking faults in the high-As pyrite core would represent the lowest energy site for the nucleation of the arsenopyrite inclusions34. However, no systematic relationship between the high density of stacking faults in the high-As core and the location of the inclusions is recorded at Chang’an (Fig. 4a, c). Considering the sharp boundary between As-rich and As-poor pyrite, and truncation of the oscillatory zoning, a crystallographic relationship between the pyrite and arsenopyrite inclusions can be predicted from the pseudomorphic CDR model20. The EBSD and TEM data reveal a similar preferred crystallographic orientation and coherent grain boundaries between the arsenopyrite inclusions and the pyrite core (Figs. 3f–g, 4d; Supplementary Fig. 2b, c). This relationship supports the replacement of the As-bearing pyrite core by As-poor pyrite and arsenopyrite via a CDR reaction at Chang’an, as reported in other gold deposits worldwide13,14,21.
The heterogenous Fe distribution in the pyrite core (Fig. 4e, f) can be explained by an interaction between the ore fluids and pyrite. The deposition of pyrites that comprise cores and rims with contrasting trace element compositions in gold deposits has mostly been attributed to the involvement of multi-pulses of fluids35. At Chang’an, two different crystal defects 1 and 2 have been identified in the investigated pyrite with defects 1 that crosscut defects 2 (Fig. 4e). The elongated defects 1 are aligned perpendicular to crystal faces which implies that their formation is related to crystal growth, which is normal for growth-related stacking faults36. However, the high As zones are parallel to defects 1 and extend almost at right-angles across the boundary between the inclusion-rich core and inclusion-free rim of pyrite (Fig. 4e), indicating continuous precipitation of the As zone from the core to the rim. This phenomenon, together with lack of evidence for overlapping alteration and mineralization related to multi-pulse fluids in the gold ores (Fig. 1c), suggests that a single-pulse fluid was responsible for the CDR and pyrite textures at Chang’an.
Microenvironment for the CDR of arsenian pyrite
The As content of arsenopyrite and phase relationships of arsenian pyrite and arsenopyrite indicate that the formation temperature of euhedral arsenopyrite was mostly from 299 °C to 290 °C (median 294 °C) with two anomalous values of 350 °C and 325 °C, whereas temperatures of fine-grained and anhedral arsenopyrite inclusions within pyrite core are 272 °C to 256 °C (median 264 °C; Fig. 5a). The temperature of the CDR of arsenian pyrite can thus be better constrained at ~260 °C. The phase diagram in Fig. 5a shows that the S fugacity (fS2) of these fine-grained arsenopyrite inclusions is about –13.8 to –11.7, which is lower than those of euhedral arsenopyrite with values of –11.9 to –10.2 (except for two anomalous values; Fig. 5a).
Considering the 1.3–4.6 km emplacement depth of alkali-rich porphyries located <1.5 km from the Chang’an deposit based on the hornblende thermobarometer37, the CDR temperature of ~260 °C, and the epizonal mineralization types24, the modeled pressure was set at ~1 kbar. Based on the low sulfide content, sericite (muscovite)–ankerite alteration, and <6 wt% NaCl equiv salinities for typical orogenic gold deposits, we set the following of mΣS = 0.01, mK+ =; 0.005, mFe2+ = 0.0005, mCa(HCO3)- = 0.00005, and mCl- = 1. The pH and fO2 conditions of alteration and ore mineral precipitation are constrained by phase stability relationships using SUPCRT9238 and values of pH are calculated from mineral equilibria in the system K-Na-Ca-Fe-Cu-Al-O-H-S. The ankerite, sericite, and quartz alteration assemblages indicate a wide pH range, 4.7–5.8, of the ore fluids during mineral precipitation (Fig. 5b). Formation of mineral assemblages of pyrite-chalcopyrite-galena required logfO2 values between −36.6 and −32.9 (Fig. 5b).
Invisible Au enrichment and implications
The ore fluids infiltrated and reacted with the sandstone and its hosted pre-existing pyrite to form quartz-ankerite veinlets and alteration haloes with invisible Au-bearing arsenian pyrite at Chang’an (Fig. 6a, b). As noted above, the complex pyrite textures can be explained as pseudomorphic replacement of arsenian pyrite by fluid-mediated CDR. Considering the pyrite texture and the mineral assemblage, the relevant reactions are:
The syn-sedimentary and pre-existing different generations of pyrite generally have low As contents with mean values ranging from 620.8 ppm to 8931 ppm at Chang’an24. The cores of hydrothermal pyrite have elevated As contents with a mean value of 11,325 ppm24, and depleted S and Fe contents relative to pre-existing pyrite that was dissolved during the fluid-mediated CDR process (Fig. 4e, f). It resulted in an increase in S in the ore fluids, especially at fluid-crystal interfaces, and thus increased the solubility of gold as an Au(HS)2- complex19,39. The reaction may also cause an increase in O fugacity, as illustrated by a decreasing trend in δ34S values from pyrite core to pyrite rim24. The increase in O fugacity would have promoted residence of Au in the ore fluids as shown in Fig. 5b. The abundant crystal defects (e.g., stacking faults and dislocations) in the pyrite core can be attributed to either or both of the heterogeneous As incorporation into lattice crystal growth in pyrite6 and lattice deformation driven by stress and fluid pressure, or both36. The sericite and quartz were deposited along stacking faults in the pyrite core (Fig. 4a), indicative of a cogenetic relationship between them. The minor native Au overgrown with quartz wrapped in the pyrite core can be attributed to the deposition of Au and quartz from ore fluids due to local supersaturation in Au and Si13.
HAADF-STEM images show that arsenopyrite inclusions grew along microfractures of the pyrite core (Fig. 4c), suggesting that the fine-grained arsenopyrite inclusions precipitated later than its formation. The equation for reaction 2 demonstrates that the deposition of arsenopyrite inclusions in pores within the pyrite core would have consumed the Fe, As, and S and thus result in a decrease in S fugacity. This inference is supported by the decreased S fugacity of –13.8 to –11.7 for the precipitation of arsenopyrite inclusions formed by the CDR, which is lower than that of the euhedral arsenopyrite and intergrown pyrite that were precipitated directly from the ore fluids (–11.9 to –10.2; Fig. 5a). The interpreted decrease in S fugacity would have triggered the deposition of invisible Au in the oscillatory As-zoned pyrite rims (Fig. 6c). Gold in the pyrite rims is dominantly in solid-solution, indicating that the ore fluid was still undersaturated with Au after the precipitation of the arsenopyrite inclusions. The incorporation of Au in pyrite rims with Au-As zoning (reaction 3) can be attributed to processes operating at the mineral surfaces and the growth rate of pyrite, as reported in other cases worldwide4,14,40,41.
This study records a detailed process of mineral growth, fluctuation of physicochemical conditions, and final Au incorporation into pyrite rims associated with the CDR at the micro- to nano-scale. At the ore scale, there is a decline in the concentration of arsenopyrite inclusions, thickness of pyrite rims, and thus gold concentration, from proximal to distal quartz-ankerite veinlets (Fig. 2a–c, f), which can be attributed to a decline in ore fluid: rock ratios. High fluid-rock ratios are likely a pivotal factor for upgrade of invisible Au during CDR reactions, as supported by the thermodynamic modeling by ref. 42. The pyrite textures at Chang’an are similar to those of Sunrise Dam21 and Kanowna Belle gold deposits43 in Western Australia and Konkera gold deposit in West Africa44, suggesting that the process of Au release, remobilization, and re-enrichment noted above is not unique.
Methods
Geological sampling
The high-grade (>10 g/t) gold ores (CA18-1) are hosted in the sandstone, which is cut by a series of sub-parallel centimeter-scale quartz-sulfide veinlets associated with sericite alteration haloes (Fig. 1c, d). The sample CA18-1 was collected from the 1532 m level and the location has been marked in Fig. 1a and Supplementary Fig. 1b.
Scanning electron microscope (SEM) and electron backscattered diffraction (EBSD) analyses
Thin sections and polished mounts of studied samples were examined under an optical microscope and SEM to determine mineral textures and paragenesis. Analyses of SEM were carried out in the Key Laboratory of Deep-Earth Dynamics, Institute of Geology, Chinese Academy of Geological Sciences, using a FEI Nova NanoSEM 450. The backscattered electron (BSE) imaging was taken under an operating voltage of 15–20 KV and the working distance of 13.5 mm. Crystallographic orientation analysis was carried out using an EBSD detector installed at a field emission SEM system at the SEM-EBSD Laboratory, School of Earth Sciences, China University of Geosciences (Wuhan). Working conditions were as follows: 20 kV accelerating voltage, 0.1–0.3 spot size, working distance of 20 mm, 70° sample tilt angle, and low-vacuum mode of 20 Pa. Diffraction patterns were collected and indexed with an automatic mapping mode using the Aztec 4.0 software from the Oxford Instruments.
TESCAN integrated mineral analyzer (TIMA) and electron probe microanalysis (EMPA)
Alteration types and crosscutting relationships were analyzed using TIMA at the Guangzhou Tuoyan Analytical Technology Co., Ltd. An acceleration voltage of 25 kV and a beam current of 8.24 nA were used with working distance of 15 mm. Pixel spacing and dot spacing were 3 μm and 9 μm, respectively. The samples were scanned using TIMA liberation analysis module. Major element components of arsenopyrite were analyzed at Craton Science and Technology Co., LTD, Beijing, using a JXA-8230 electron microprobe. Working conditions include a voltage of 15 kV, beam current of 2 × 10–8 A, spot size of 1 μm, and detection limit of 0.01%. Analytical results were reduced using the ZAF (Z, atomic number; A, absorption; F, fluorescence) correction routines.
Time-of-flight secondary ion mass spectrometry (ToF-SIMS) microanalysis
The ToF-SIMS of arsenian pyrite was performed using the IONTOF M6 instrument in the John de Laeter Centre at Curtin University, Australia. The instrument was operated in Fast Imaging mode with a 60 kV Bi3++ primary ion source at a pulsed current of 0.2 pA. Negative ions were collected using Delayed Extraction mode for the mass analyzer at a cycle time of 50 µs. SIMS maps were collected over a 350 × 350 µm field of view with 1024 × 1024 pixels in each frame (342 nm pixel size). To remove surface contamination and increase the ionization rate, the field of view was pre-sputtered with a Cs+ ion source (2 kV, 70 nA) over a 500 × 500 µm area for 60 s. Analysis time was 50 min where 60 frames were collected over the analyzed region.
Transmission electron microscopy (TEM) observation and analyses
Two regions of interest cutting the boundaries of Au-poor pyrite core and Au-rich pyrite rim were extracted using Focused ion beam (FIB) micro-sampling on a Zeiss Auriga Compact instrument at the Institute of Geology and Geophysics, Beijing, China. The steps that select the sites of interest (Supplementary Fig. 3a, e), cut and remove the foil from its excavation site (Supplementary Fig. 3b, c, f, g), and mount the foil on the Cu-grid (Supplementary Fig. 3d, h) in the preparation of site-specific TEM foils are shown in Supplementary Fig. 3. The TEM analyses for nano-scale mineral texture and elemental mapping by the Energy Dispersive Spectrometer (EDS) were performed at Electron Microscopy Center of GIGCAS, using a Thermofisher FEI Talos F200S microscope. A Ceta 16 M camera and TEM image analysis software (Thermo Fisher Scientific) were used to capture and analyze the TEM images, resepctively. A 10 μm selective area aperture under the microscope mode in the TEM system was used to record the selected area electron diffraction (SAED) patterns. The scanning transmission electron microscopy (STEM) system was used to record the EDS spectra and elemental maps and the EDS quantifications were performed at a beam current of 1 nA using the Thermo Fisher Scientific software either with or without standards. The uncertainty of Fe and S were <0.5%.
Data availability
Source data that support the findings of this study are available in figshare with the identifier https://doi.org/10.6084/m9.figshare.25471537.v145.
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Acknowledgements
We appreciate Editors Joe Aslin and Holly Stein for handling, and Drs. Evan Hastie and Sabina Strmic Palinkas for providing constructive comments and suggestions on the manuscript. We thank mine geologists in the Chang’an gold deposit for their kind help during our fieldwork and sampling permissions, Prof. Chang Xu and Dr. Dapeng Wen at the China University of Geosciences (Wuhan) for their comprehensive help with the EBSD analyses of pyrite. This work was supported by the National Natural Science Foundation of China (42125203, 42102107, 42372110), the “Deep-time Digital Earth” Science and Technology Leading Talents Team Funds from the Central Universities for the Frontiers Science Center for Deep-time Digital Earth, China University of Geosciences (Beijing) (2652023001), and the 111 Project of the Ministry of Science and Technology (BP0719021). The IONTOF M6 ToF-SIMS at the John de Laeter Centre, Curtin University was funded by the Australian Research Council LIEF program (LE190100053).
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Conceptualization: L.Y., Q.F.W. and J.D. SEM, EBSD, and EPMA work: L.Y. and H.J.L. FIB and TEM work: L.Y. and H.Y.X. ToF-SIMS work: R.X.W. and W.R. Thermodynamic modeling: H.J.L. Data analysis: L.Y., Q.F.W., H.Y.X., and D.F. Writing—original draft: L.Y., Q.F.W., J.D. and D.G. Writing—review & editing: all authors.
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Communications Earth and Environment thanks Evan Hastie, Sabina Strmić Palinkaš, and [name] for their contribution to the peer review of this work. Primary Handling Editors: Holly Stein and Joe Aslin. A peer review file is available.
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Yang, L., Wang, Q., Fougerouse, D. et al. Release and re-enrichment of invisible gold in arsenian pyrite promoted by coupled dissolution-reprecipitation reactions. Commun Earth Environ 5, 241 (2024). https://doi.org/10.1038/s43247-024-01408-5
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DOI: https://doi.org/10.1038/s43247-024-01408-5
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