日本地球惑星科学連合2021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-IT21] 固体地球科学と材料科学の融合が切り拓く新展開

2021年6月3日(木) 13:45 〜 15:15 Ch.24 (Zoom会場24)

コンビーナ:河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)、土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、野村 龍一(京都大学)、大村 訓史(広島工業大学)、座長:河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)、野村 龍一(京都大学)

14:20 〜 14:35

[SIT21-03] 第一原理電子状態計算を用いた沈み込む海洋プレート中の蛇紋石の構造モデリング

*土屋 旬1、井上 紗綾子1 (1.愛媛大学地球深部ダイナミクス研究センター)

キーワード:第一原理計算、蛇紋石

Serpentine is hydrous phyllosilicate known to be formed in the mantle wedge by a reaction between mantle peridotit and upwelling water released by the decomposition of hydrous minerals in the subducting slab [e.g. Schmidt and Poli,1998]. Partially serpentinized peridotite may be a significant reservoir of water in the mantle wedge and the dehydration of serpentine is considered to have an important contribution to the generation of arc magmatism. This was also extensively investigated in connection with intermediate and deep earthquakes [e.g. Irifune et al. , 1996].
In order to investigate the transporting processes of water into the Earth’s interior, the thermodynamic stabilities and the elastic properties of antigorite should be clarified. Antigorite is the high-temperature polymorph of serpentine and thus the relevant phase in the subduction zone. This phase has been reported to show polysomatism depending on the pressure and temperature conditions. Previous TEM study reported that m value (m = number of SiO4 tetrahedra in a wavelength along the a axis) increases/decreases with pressure/temperature [e.g. Wunder et al. 2001]. However, there is no sufficient structural and thermodynamic corroboration regarding the stable polysome of antigorite along the pressure and temperature conditions of the subducting oceanic plate.
In the present study, we investigated the structure and elasticity of antigorite with several different m values by ab intio calculation and discuss the stable polysome of antigorite in the subducting oceanic plate.