日本地球惑星科学連合2018年大会

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[EE] 口頭発表

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-IT22] 核-マントルの相互作用と共進化

2018年5月23日(水) 10:45 〜 12:15 国際会議室(IC) (幕張メッセ国際会議場 2F)

コンビーナ:飯塚 毅(東京大学)、渋谷 秀敏(熊本大学大学院先端科学研究部基礎科学部門地球環境科学分野)、土屋 卓久(愛媛大学地球深部ダイナミクス研究センター、共同)、太田 健二(東京工業大学大学院理工学研究科地球惑星科学専攻)、座長:角野 浩史舘野 繁彦飯塚 毅

11:15 〜 11:30

[SIT22-21] He and Ar partitioning between liquid iron and molten silicate at high pressure

Zhihua Xiong1、*Taku Tsuchiya1 (1.Geodynamics Research Center, Ehime University)

キーワード:Noble gas partitioning, Ab initio Calculation, Earth's core

The Earth’s core has been suggested as a potential reservoir of noble gases, which can remove the difficulties of their long-term maintenance in the mantle. The fundamental process controlling noble gas sequestering into the core is their partitioning between liquid iron and molten silicate. Unfortunately, limited measurements have only been conducted so far. Experiments conducted by Matsuda et al. [1993] up to 10 GPa showed that the partitioning coefficients of noble gases decrease with pressure, denying the core to be a noble gas reservoir. In contrast, Bouhifd et al. [2013] reported that the helium partitioning coefficient becomes more constant (~10-2) at P > 10 GPa, suggesting that some helium could be dissolved into the core. However, it is unclear whether this tendency is applicable to other noble gases.

Here we investigate the helium and argon partitioning between liquid iron and molten silicate using the ab initio molecular dynamics method combined with thermodynamics integration technique [Taniuchi and Tsuchiya, 2018]. The partitioning coefficients are computed from the Gibbs free energy changes associated with their exchange reactions. Although more detailed studies on several factors including temperature, pressure, and composition are required, our results in the moment suggest possible partitioning of helium and argon into liquid metal at high pressure. We will try to explain the behaviors from the electronic and structural points of view.