日本地球惑星科学連合2024年大会

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セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT15] Mass and energy transport properties and processes in the crust and the mantle

2024年5月30日(木) 09:00 〜 10:15 301B (幕張メッセ国際会議場)

コンビーナ:Mysen Bjorn(Geophysical Laboratory, Carnegie Inst. Washington)、大谷 栄治(東北大学大学院理学研究科地学専攻)、高橋 菜緒子(東京大学大学院理学系研究科)、Codillo Emmanuel(Carnegie Institution for Science)、座長:Mysen Bjorn(Geophysical Laboratory, Carnegie Inst. Washington)、大谷 栄治(東北大学大学院理学研究科地学専攻)



09:15 〜 09:30

[SIT15-02] Experimental investigation of tungsten speciation in hydrothermal fluids under subduction-zone conditions

*高橋 菜緒子1中村 美千彦2鍵 裕之1 (1.東京大学大学院理学系研究科、2.東北大学大学院理学研究科)

キーワード:タングステン、流体、ダイヤモンドアンビルセル、ラマン分光法

Tungsten(W) is recognized as a critical raw material essential for increasing economic demand and applications in green technology. W is an incompatible and fluid mobile element in the Earth’s crust and mantle, and its stable isotopes serve as tracers to decipher geological processes. Despite its importance, the mechanisms controlling W transport in the Earth’s crust and upper mantle remain uncertain, requiring a fundamental understanding of W speciation in hydrothermal solutions. Early solubility experiments have suggested that W(VI) primarily dissolves as simple monomers [WO4]2- and [HWO4]- and their alkali ion pairs[1]. This view of W speciation contrasts with the prevailing view that W(VI) forms large polynuclear metal-oxygen anions under ambient conditions. Recent in-situ Raman spectroscopic analyses using a fused-silica capillary tube have suggested the persistence of polyanions in acidic to neutral solutions up to 400 °C and 60 MPa [2]. However, the speciation of W(VI) at deep crustal pressures and temperatures has not yet been explored. In this study, we performed in situ Raman spectroscopic measurements of W-dissolved hydrothermal solutions up to 750 °C and 1.2 GPa using an externally-heated hydrothermal diamond anvil cell. In the WO3–H2O system, the Raman spectra of tungsten oxide-saturated fluids showed no detectable W=O stretching band from monomeric tungstate species [WO4]2- appearing at ~930 cm-1. Instead, the Raman bands centered at ~950 cm-1 and ~975 cm-1, which are typically assigned to tungsten polyanions, were respectively detected above 500 °C and 600 °C. These findings indicate that polymeric tungsten species are dominant in high-pressure and high-temperature fluids, challenging existing thermodynamic modeling of electrolyte fluids. In the Na2WO4–H2O±HCl systems at constant concentration, the initial pH of solutions primarily controls tungsten speciation at elevated pressures and temperatures, which is in broad agreement with the previous studies. In addition, we observed that polymeric tungsten species that appeared at ~950 cm-1 became more pronounced in acidic to alkaline solutions with increasing pressures and temperatures. Consequently, our results suggest that tungsten polyclusters govern tungsten hydrothermal transport in the Earth’s deep crust and upper mantle and may be potential precursors in mineralizing fluids.

References: [1] Wood (1992) Geochim. Cosmochim. Acta, 56, 1827–1836. [2] Carocci et al. (2022) Geochim. Cosmochim. Acta, 317, 306–324.