流体矿物钛同位素分馏:对矿床影响的计算和经验结果

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Geochimica et Cosmochimica Acta Pub Date : 2024-12-15 DOI:10.1016/j.gca.2024.12.007
Christopher Emproto, Ryan Mathur, Mingguang Sun, Adam C. Simon, Linda Godfrey
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引用次数: 0

摘要

钛(Ti)在地质流体中通常表现出低流动性,这是由于普通(Fe-)Ti氧化物矿物的水溶性较低。因此,地质系统中Ti同位素(δ49/47Ti,用δ49Ti表示)的变化主要归因于岩浆分异。因此,流体-矿物分选的潜力受到的关注较少。然而,在自然系统和实验室研究中观察到,富含配体的液体能够调动钛。由于热液矿化通常与能够运输大量金属的富配体盐水有关,因此Ti同位素可能有助于理解复杂热液系统中的矿化和蚀变。本文通过对地质系统和相关实验条件下理论存在的各种钛配位配合物的计算建模,以及各种含钛结晶相的计算分馏因子,研究平衡流体-矿物钛同位素分馏的基本机制。这些结果表明,我们的模型Ti配合物和具有6配位Ti的相之间的平衡流体-矿物Ti同位素交换通常会导致流体中重Ti同位素的富集。由于具有6配位Ti的矿物(如磁铁矿和钛铁矿)是固体地球中最重要的Ti储集层,因此可以推广陆相岩石与流体之间的Ti同位素平衡,使流体富集重Ti同位素。我们还进行了磁铁矿- 左尖晶石浸出实验,以研究这一阶段的流体矿物钛同位素分馏。不同酸强度、浸出温度和与HCl和HF反应时间的矿物浸出实验定性地支持了这样的预测:在流体-矿物相互作用过程中,流体相将富集重钛同位素,并与富钛磁铁矿接近平衡。此外,浸出数据还表明,当Ti交换受到限制时,流体中较轻的Ti同位素会略微富集,这可能是由于动力学效应。因此,来自自然系统的磁铁矿可能在与流体平衡的再生矿物替换过程中失去重钛同位素,或者可能在动力学分馏过程中失去轻钛同位素,导致矿物δ49Ti值不能充分解释岩浆分馏或矿物间分馏。这些结果是对热液矿物系统中可能影响钛同位素分馏的流体-矿物相互作用的第一次观察,Ti同位素应进一步研究,作为了解矿床水中金属运输和示踪蚀变的潜在方法。
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Fluid-mineral titanium isotope fractionation: Computational and empirical results with implications for mineral deposits
Titanium (Ti) typically exhibits low mobility in geologic fluids due to the low aqueous solubility of common (Fe-)Ti oxide minerals. Consequently, Ti isotope variations (δ49/47Ti, given as δ49Ti) in geologic systems are primarily attributed to magmatic differentiation. Thus, the potential for fluid-mineral fractionation has received less attention. However, ligand-rich fluids are capable of mobilizing Ti as observed in natural systems and laboratory studies. As hydrothermal ore mineralization is commonly associated with ligand-rich brines capable of transporting significant quantities of metals, Ti isotopes may aid in understanding mineralization and alteration in complex hydrothermal systems. Here we present data from computational modeling of various Ti coordination complexes theorized to exist in geologic systems and/or under relevant experimental conditions as well as computed fractionation factors for various Ti-bearing crystalline phases to investigate the basic mechanics of equilibrium fluid-mineral Ti isotope fractionation. These results indicate that equilibrium fluid-mineral Ti isotope exchange between our modeled Ti complexes and phases with 6-coordinated Ti is predicted to generally lead to enrichment of heavy Ti isotopes in the fluid. Because minerals with 6-coordinated Ti (such as magnetite and ilmenite) are the most important reservoirs of Ti in the solid Earth, Ti isotope equilibration between terrestrial rocks and fluids can be generalized to enrich the fluid in heavy Ti isotopes. We also performed magnetite-ülvospinel leaching experiments to investigate fluid-mineral Ti isotope fractionation in this phase. Mineral leaching experiments varying acid strength, leaching temperature, and reaction time with HCl and HF qualitatively support the prediction that the fluid phase will become enriched in heavy Ti isotopes during fluid-mineral interactions that approach equilibrium with Ti-rich magnetite. Additionally, the leaching data also suggest that the fluid becomes slightly enriched in lighter Ti isotopes when Ti exchange is limited—potentially due to kinetic effects. Therefore, magnetite from natural systems may be depleted in heavy Ti isotopes during regenerative mineral replacement involving equilibration with fluids or may possibly become depleted in light Ti isotopes under a kinetic fractionation regime—leading to mineral δ49Ti values that are insufficiently explained by magmatic differentiation or inter-mineral fractionation. These results are a first look at fluid-mineral interactions that may affect Ti isotope fractionation in hydrothermal mineral systems, and Ti isotopes should be further studied as a potential method of understanding aqueous metal transport and tracing alteration in mineral deposits.
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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.
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