Ore Geology Reviews

Volume 109, June 2019, Pages 545-563
Ore Geology Reviews

The nature and partitioning of invisible gold in the pyrite-fluid system

https://doi.org/10.1016/j.oregeorev.2019.04.024Get rights and content

Highlights

  • Au in sulfide-sulfate solutions is complexed with the HS, S3·- and S2·- ions.
  • In As-poor systems invisible gold in pyrite is present as Au(0) and Au(I).
  • Au(I) in pyrite occurs as chemisorbed S-Au-Sn moieties similar to those in the fluid.
  • Au(I) uptake by pyrite from fluid is enhanced with decreasing temperature.
  • Au(I) pyrite/fluid partition coefficients allow predictions of gold tenors in pyrite ore.

Abstract

The most characteristic feature of hydrothermal deposits of gold is its intimate association with pyrite. Microscopically visible gold occurs in pyrite ore as metal particles of >0.1 µm in size, together with so called “invisible” gold, undetectable by conventional microscopic methods. The chemical, redox and structural state of this invisible gold and the mechanisms of its incorporation into pyrite remain both inconsistent and controversial since the dawn of economic geology. To clarify these issues, we performed laboratory experiments to simulate interactions of gold-bearing sulfur-rich hydrothermal fluids with arsenic-free pyrite at temperatures from 350 to 450 °C and pressures from 400 to 700 bar, typical of the formation conditions of many types of gold deposits. Gold solubility was measured in these fluids as a function of sulfur speciation and acidity. Gold redox and structural state in pyrite was characterized by high-energy resolution fluorescence-detected x-ray absorption spectroscopy (HERFD-XAS), together with more traditional analytical techniques such as scanning electron microscopy (SEM), x-ray diffraction (XRD), electron probe micro analysis (EPMA), laser ablation inductively coupled plasma mass spectrometry (LA-ICPMS), and inductively coupled plasma atomic emission spectrometry (ICP-AES). Results show that dissolved Au in sulfide-sulfate solutions forms complexes with hydrogen sulfide, and tri- and di-sulfur radical ions whose amounts depend mostly on the fluid pH and total sulfur concentration. Invisible gold in pyrite occurs as Au metal submicron- to nano-sized particles and chemically bound Au(I) in the form of (poly)sulfide clusters composed on S-Au-S linear units, similar to those in aqueous complexes. Our findings contest the common belief that Au(I) substitutes for Fe and/or S in the structure of As-poor pyrite. The partition coefficient of Au(I) between pyrite and the fluid, Dpy/fl, is determined to be 0.15 ± 0.07 at 450 °C in a wide range of Au fluid phase concentrations (10–1000 ppm), but much higher Dpy/fl values, between 10 and 50, are found at 350 °C. These Au partitioning trends coupled with the new data on Au molecular environment in pyrite suggest a control of Au(I) incorporation in the mineral by a chemisorption step. Extrapolated to Au contents of hydrothermal fluids of the Earth’s crust which are typically below 1 ppm, our Dpy/fl values reproduce fairly well the natural Au tenors in As-poor pyrites (∼0.1–1 ppm Au), which are 100–1000 times lower than those typically observed in arsenian pyrites and arsenopyrites (10–1000 ppm Au at As tenors of 0.01–10 wt%). Our results thus indirectly highlight a key role played by arsenic in gold enrichment in As-bearing iron sulfide ore, a role that yet remains to be fully understood and quantified.

Introduction

The most characteristic feature of hydrothermal deposits of gold is its intimate association with iron sulfide minerals, pyrite and arsenopyrite, in which Au concentrations may reach 100–1000 ppm, i.e. almost million times the Au average crustal abundance. Gold affinity for these minerals has been recognized since the first half of the 20th century (e.g., Goldschmidt, 1937). Both ‘visible’ native gold (i.e., optically detectable particles >0.1–1 μm) in physical association with pyrite, and ‘invisible’ (i.e., optically undetectable) gold, possibly incorporated into the mineral structure, occur (e.g., Boyle, 1969, Cathelineau et al., 1989, Cook and Chryssoulis, 1990; references therein). Invisible gold, also termed refractory gold, is not only difficult to identify, but also hard to recover from ore (e.g., Yang et al., 1998, Adams, 2005, Marsden and House, 2009). Such refractory gold poses problems both for accurate estimates of the gold distribution and endowment of a deposit and for efficient extraction of the metal from iron sulfide ore. Resolving these issues requires knowledge of the nature, distribution and mechanisms of incorporation of invisible gold in pyrite, which all yet remain enigmatic. The present study was designed in an attempt to better understand the gold-pyrite relationships, using a novel integrated experimental, spectroscopic and modeling approach.
The literature on Au-bearing pyrite over the four last decades is full of discussions about the chemical and redox state of invisible gold. Based on a variety of analytical techniques such as scanning electron microscopy (SEM), high resolution transmission electron microscopy (HRTEM), secondary ion mass spectrometry (SIMS), laser ablation inductively coupled plasma mass spectrometry (LA-ICPMS), electron probe microanalyzer (EPMA), Mössbauer spectroscopy (MBS), proton induced x-ray emission (PIXE), x-ray photoelectron spectrometry (XPS), x-ray absorption spectroscopy (XAS), atom probe microscopy (APM), atomic force microscopy (AFM), tunneling spectroscopy (STS), coupled with analyses of elemental distribution and inter-element correlations, most studies agree that invisible gold occurs in two major chemical states: an elemental form as nanometer-size particles of Au(0) or alloys with some other trace metals (e.g., Bi, Te, Ag), and a chemically bound form (e.g., Marion et al., 1986, Arehart et al., 1993, Scaini et al., 1998, Friedl et al., 1995, Fleet and Mumin, 1997, Genkin et al., 1998, Den Besten et al., 1999, Simon et al., 1999, Tauson, 1999, Cabri et al., 2000, Palenik et al., 2004, Reich et al., 2005, 2006, Reich et al., 2010, Mikhlin et al., 2011, Deditius et al., 2011, Fougerouse et al., 2016, Trigub et al., 2017a). However, despite significant recent advances in analytical and microscopic methods listed above, the nature of this latter type of gold and factors controlling its incorporation in pyrite remain both inconsistent and controversial. For example, the redox state of chemically bound gold varies from Au3+ to Au1−, and its coordination number from 2 to 6, according to different authors (e.g., see Cabri et al., 2000 for review); such large variations make it difficult to attribute to Au an exact structural position in pyrite and to identify the nature of coordinating atoms (e.g., Au, Fe, S). The situation is further complicated by the presence of other minor and trace elements (Cu, Sb, Ni, Co, Ag, Bi, Se, Te) and, in particular, of arsenic with which gold is systematically correlated in arsenian pyrite (e.g., Reich et al., 2005). These elements, often present in far greater concentrations (>0.1–1.0 wt%) than Au (typically < 0.01–0.1 wt%), greatly complicate the assessment, using inter-element correlations, of the Au oxidation state and atomic substitutions in pyrite. The use of direct redox-sensitive spectroscopic methods such as X-ray photoelectron, X-ray absorption or Mössbauer spectroscopy is often limited by low concentrations, poor selectivity for Au in the presence of As and other elements, and a lack of adequate standards.
As a result of these limitations, the mechanisms of Au incorporation in hydrothermal pyrite and arsenopyrite and the role of arsenic and other elements played in this process still remain hypothetical. For example, some earlier studies invoked gold transport by the fluid phase in the form of Au-As-S (Sb, Se, Te) aqueous complexes and their co-precipitation with ferrous iron (Boyle, 1969, Boiron et al., 1989). Other studies suggested chemisorption of dissolved Au as Au-S(As) complexes at As-rich, Fe-deficient sites (Mao, 1991, Fleet and Mumin, 1997, Cepedal et al., 2008), electrochemically driven adsorption of negatively charged AuHS2- complexes on semiconducting As-pyrite and arsenopyrite surfaces (Mironov et al., 1981, Möller and Kersten, 1994, Widler and Seward, 2002), or Au3+ and Au+ precipitation on sulfide surfaces due to Au reduction (Bancroft and Hyland, 1990, Scaini et al., 1998, Maddox et al., 1998, Mikhlin et al., 2011). However, these hypotheses are mostly based on low-temperature experiments (<100 °C), some of them involving Au aqueous complexes (AuCl4-, AuCN2Br23-), which are unlikely at hydrothermal conditions (e.g., see Pokrovski et al., 2014 for a review of Au speciation in hydrothermal fluids). These limitations complicate the extrapolation of the results of such experiments to the far greater temperatures of Au-bearing pyrite formation in nature (>150–200 °C). Different isomorphic substitution models of Au in the pyrite structure were also proposed, including coupled substitutions of As3+ + Au+ for 2 Fe2+, As3+ + Au3+ for 3 Fe2+ (Deditius et al., 2008), Cu+ + Au3+ for 2 Fe2+ (Chouinard et al., 2005), or Au+ + S2− for Fe2+ + HS (Tauson, 1999), but analytical methods capable of unambiguously supporting these models are lacking. Note that the geometry of the available structural sites in pyrite composed of Fe(S6) octahedrons and S(Fe3S) distorted tetrahedrons (Le Pape et al., 2018) is not favorable for an energetically stable incorporation of both Au+ and Au3+ ions that have linear and square planar coordination geometries in most inorganic and organometallic compounds (e.g., Cotton and Wilkinson, 1988). Furthermore, common precipitation mechanisms of As and Au due to fluid reduction and/or cooling, or coupled As-Au redox reactions on the pre-existing (arseno)pyrite have also been considered (e.g., Heinrich and Eadington, 1986, Pokrovski et al., 2002), but they remain qualitative owing to the complexity of the fluid composition and evolution in hydrothermal systems and the interplay of multiple factors controlling mineral solubility such as temperature (T), pressure (P), redox, acidity (pH), and fluid composition (Pokrovski et al., 2014).
It follows from this brief overview that a deeper understanding of the gold-pyrite(-arsenic) relationships in hydrothermal systems awaits experimental studies at pertinent laboratory-controlled conditions, coupled with Au-selective in situ spectroscopic techniques. In the recent years, advances in synchrotron-based high-resolution X-ray absorption/fluorescence spectroscopy (e.g., Proux et al., 2017, Manceau et al., 2018, Le Pape et al., 2018; references therein) have provided an unprecedented gain both in sensitivity (metal detection limits <1 ppm) and selectivity (ability to isolate the trace metal fluorescence signal in a complex mineral/organic matrix), now enabling to directly “see” invisible gold in iron sulfide minerals. In this study, we designed hydrothermal experiments aimed at investigating the Au-pyrite interactions in model S-bearing fluid-pyrite systems at temperatures (350–450 °C) and pressures (400–700 bar) typical of those of various types of gold deposits, as a function of gold and sulfur speciation in the fluid phase. The Au-bearing pyrites resulting from such experiments were investigated by high-resolution X-ray absorption spectroscopy (HR-XAS) coupled with more “traditional” methods (EPMA, SEM, XRD, LA-ICPMS, ICP-AES) to reveal the state of invisible gold in pyrite and to derive pyrite-fluid partition coefficients for chemically bound Au. The results allow predictions of invisible Au contents in ore, and more reliable identification of the factors leading to Au enrichment in iron sulfide minerals. Although the present work deals with As-free systems, the results also help indirectly assess the role of arsenic, thus providing the foundation for future experimental and analytical studies on far more complex As-bearing systems.

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Section snippets

Experimental strategy and conditions

The primary goal of this exploratory experimental study was to investigate the state of gold incorporated into pyrite under conditions pertinent to natural hydrothermal systems forming gold deposits. Gold incorporation in pyrite is expected to occur via i) exchange of an Au-bearing aqueous fluid with already existing sulfide minerals, and/or ii) simultaneous precipitation of gold and pyrite (and other metals) from an aqueous fluid, driven by changes in T, P or fluid composition. Such

Batch-reactor experiments

Gold concentrations measured in quenched solutions from batch-reactor experiments at 450 °C and 700 bar are reported in Table 1. The dissolved Au concentrations vary from ∼100 ppm (in acidic solutions) to almost 3000 ppm (in alkaline solutions). A reasonable quantification limit for aqueous Au in our experimental systems is about 100–150 ppm, which is due to intrinsic uncertainties of the batch-reactor technique such as incomplete recovery of Au precipitated on the reactor walls after the

Interpretation of gold solubility and speciation in sulfur-bearing fluids

The interpretation of Au solubility measured in our experimental sulfate-sulfide systems in terms of Au aqueous complexes is primarily based on knowledge of sulfur speciation itself, which has been a subject of recent systematic research in similar systems at elevated temperatures and pressures using in situ spectroscopic methods (Pokrovski and Dubrovinsky, 2011, Jacquemet et al., 2014, Barré et al., 2017, Pokrovski and Dubessy, 2015, Pokrovski et al., 2015). These direct spectroscopic data,

Concluding remarks

The key points of this study are the following:
A combination of experimental, analytical and modeling approaches used in this work enables new insight into one of the oldest enigmas of Ore Deposit Research, the nature of invisible gold in pyrite. We show that gold is incorporated from hydrothermal fluids into As-poor pyrite both as native metal, Au(0) in the form of nano- and submicron particles, and as chemically bound gold of a nominal redox state of +1, Au(I).
High-resolution XANES

Acknowledgments

This work was funded by the French National Research Agency (grants RadicalS – ANR-16-CE31-0017 and SOUMET – ANR-2011-Blanc SIMI 5-6 009), the Institut des Sciences de l’Univers of the Centre National de la Recherche Scientifique (grants OrPy-CESSUR and AsOrPy-CESSUR), and the Institut Carnot ISIFoR (grant OrPet). We acknowledge the European Synchrotron Radiation Facility (ESRF) for providing access to beamtime and infrastructure. DFT calculations were performed using HPC resources from CALMIP

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