Gold in sulfide fluids revisited

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Geochimica et Cosmochimica Acta Pub Date : 2024-08-31 DOI:10.1016/j.gca.2024.08.022
Boris R. Tagirov, Nikolay N. Akinfiev, Mariia E. Tarnopolskaia, Irina Yu. Nikolaeva, Irina Yu. Zlivko, Valentina A. Volchenkova, Luydmila A. Koroleva, Alexander V. Zotov
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Abstract

Gold solubility was measured at temperatures of 350, 400, 450, and 490 °C and pressures of 500 and 1000 bar in an ’oxidized sulfide’ system, as a function of pHT (2 – 10) and sulfur concentration (m(Stotal) = 0.03 – 1.2 [mol·(kg H2O)-1]). In this system, sulfur primarily exists as H2S, H2SO3, H2SO4, their dissociation products, and radical species such as S2- and S3-. The complexes Au(HS)2-, Au2S22-, AuHS(aq), AuHS(H2S)3(aq), and AuOH(aq) were identified as the primary gold species in the experimental fluids, varying with pH and m(Stotal). The solubility constants for Au(HS)2-, a critical (hydro)sulfide complex, align excellently with literature for ’reduced sulfide’ fluids, where sulfur predominantly exists in the 2- oxidation state. New experimental data from the ’oxidized sulfide’ system were regressed along with reliable literature data from ’reduced sulfide’ systems to calculate standard thermodynamic properties and parameters of the Helgeson-Kirkham-Flowers (HKF) model. The solubility constants for charged complexes, Au(HS)2- and Au2S22-, increase sharply with temperature, whereas those for neutral species, AuHS(aq) and AuHS(H2S)3(aq), show a pronounced peak near 300 °C. These (hydro)sulfide complexes account for gold solubility ranging from a few tens of ppb to a few tens of ppm in natural sulfide fluids, depending on the fluid pH. Thermodynamic calculations also indicate that, in addition to (hydro)sulfide species and the hydroxide complex, AuCl2- significantly contributes to Au mobility in high-temperature acidic chloride fluids. Based on new experimental data and prior studies using solubility and X-ray absorption spectroscopy methods, other gold complexes including mixed Au-HS-Cl, Au-HS-S3- species, and complexes with alkali metal cations, are deemed redundant. Above 250 °C, the influence of chloride salts on gold solubility can be accurately modeled using a simple extended Debye-Hückel equation with the term bγ·I = 0. The Setchenov coefficient bn = 0 suffices for calculating the activity coefficients of neutral species. This streamlined thermodynamic model aligns closely with earlier experimental work by Terry Seward and his team, effectively describing the state of Au in all types of natural fluids where Au exists in the 1+ oxidation state, under any set of P-T-f(O2)-f(S2)-compositional parameters.
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硫化物流体中的金再探
在温度为 350、400、450 和 490 °C,压力为 500 和 1000 bar 的 "氧化硫 "体系中,测量了金的溶解度与 pHT(2 - 10)和硫浓度(m(Stotal) = 0.03 - 1.2 [mol-(kg H2O)-1])的函数关系。在这个体系中,硫主要以 H2S、H2SO3、H2SO4、它们的解离产物以及 S2- 和 S3- 等自由基的形式存在。复合物 Au(HS)2-、Au2S22-、AuHS(aq)、AuHS(H2S)3(aq) 和 AuOH(aq) 被确定为实验流体中的主要金物种,它们随 pH 值和 m(Stotal) 的变化而变化。Au(HS)2-是一种临界(氢)硫化物复合物,其溶解常数与 "还原硫化物 "流体的文献资料非常吻合,在 "还原硫化物 "流体中,硫主要以 2- 氧化态存在。来自 "氧化硫 "体系的新实验数据与来自 "还原硫 "体系的可靠文献数据进行了回归,以计算标准热力学性质和赫尔格森-柯克姆-弗劳尔斯(HKF)模型的参数。带电络合物 Au(HS)2- 和 Au2S22- 的溶解常数随温度的升高而急剧增大,而中性物质 AuHS(aq) 和 AuHS(H2S)3(aq) 的溶解常数则在 300 °C 附近出现一个明显的峰值。在天然硫化物流体中,根据流体 pH 值的不同,金在这些(氢)硫化物络合物中的溶解度从几十 ppb 到几十 ppm 不等。热力学计算还表明,除了(氢)硫化物物种和氢氧化物络合物之外,AuCl2- 对高温酸性氯化物流体中金的流动性也有很大的影响。根据新的实验数据以及之前使用溶解度和 X 射线吸收光谱方法进行的研究,其他金络合物(包括混合 Au-HS-Cl、Au-HS-S3- 物种以及与碱金属阳离子的络合物)被认为是多余的。在 250 °C 以上,氯盐对金溶解度的影响可以用一个简单的扩展德拜-胡克尔方程(bγ-I = 0)来精确模拟。这个简化的热力学模型与 Terry Seward 及其团队早期的实验工作非常吻合,在任何一组 P-T-f(O2)-f(S2)-组成参数下,都能有效地描述金在 1+ 氧化态存在的各类天然流体中的状态。
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
期刊最新文献
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