日本地球惑星科学連合2015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-IT03] Structure and dynamics of Earth and Planetary deep interiors

2015年5月25日(月) 16:15 〜 18:00 106 (1F)

コンビーナ:*芳野 極(岡山大学地球物質科学研究センター)、田中 聡(海洋研究開発機構 地球深部ダイナミクス研究分野)、趙 大鵬(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)、亀山 真典(国立大学法人愛媛大学地球深部ダイナミクス研究センター)、John Hernlund(Earth-Life Science Institute, Tokyo Institute of Technology)、座長:芳野 極(岡山大学地球物質科学研究センター)、中島 陽一(理化学研究所放射光科学総合研究センター)

17:00 〜 17:15

[SIT03-11] First principles study on the phase stability and elasticity of potassium-host hexagonal aluminous phases

*河合 研志1土屋 卓久2 (1.Department of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo、2.Geodynamics Research Center, Ehime University)

キーワード:High pressure, Pottasium, Lower mantle, Aluminous phase

In order to understand the fate of the potassium-bearing phase subducted into the deep Earth's interior, we have studied the high-pressure stability and elasticity of KMg2Al5SiO12 hexagonal aluminous phase (K-Hex) by means of the density functional computation method. The K-Hex phase is found to be mechanically stable up to 150 GPa and also energetically more stable than the calcium-ferrite (K-CF) type structure up to 150 GPa. In addition, calculations indicate that when the spinel composition coexists with the K-hollandite (K-Hol) phase, the K-Hex phase becomes more stable than the K-Hol phase at pressures above ~27 GPa. This suggests that the hexagonal aluminous phase be a potential host of the incompatible large-ion elements such as potassium in the lower mantle, especially in the subducted basaltic Mg and Al rich composition. Finally, seismic velocities of the K-Hex phase are found slower than Mg-perovskite (pv) in the lower mantle pressures, while its density is larger than Mg-pv over 70 GPa.