日本地球惑星科学連合2021年大会

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[E] 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-IT16] Structure and Dynamics of Earth and Planetary Mantles

2021年6月4日(金) 13:45 〜 15:00 Ch.24 (Zoom会場24)

コンビーナ:中川 貴司(University of Leeds)、芳野 極(岡山大学惑星物質研究所)、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)、座長: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)

14:00 〜 14:15

[SIT16-02] ウォズリアイトの熔融温度に及ぼす高酸素分圧の影響

*山口 和貴1、川添 貴章1、井上 徹1 (1.広島大学)


キーワード:ウォズリアイト、高酸素分圧、3価の鉄イオン、急冷結晶、熔融

About 60% of the upper part of the Earth's mantle transition zone is composed of wadsleyite, which is the high-pressure phase of olivine. It is known that water and ferric iron are supplied to the mantle transition zone by subduction of the oceanic plates. A recent study revealed that ferric iron lowers melting temperature of bridgmanite, the major mineral in the lower mantle, in the MgO-FeO-Fe2O3-SiO2 system (Sinmyo et al., 2019). However, the effect of high oxygen fugacity on melting temperature of wadsleyite has not been studied so far. Therefore, in this study, we conducted experiments to clarify the effect of high oxygen fugacity on the melting temperature of (Mg0.9,Fe0.1)2SiO4 wadsleyite using a Kawai-type multi-anvil press. The experiments were performed twice at 13.5–16 GPa and 1500–1900 ℃ at oxygen fugacities buffered by Re-ReO2 and Mo-MoO2 oxygen fugacity buffers. As a result, quenched crystals were observed at high oxygen fugacity buffered by the Re-ReO2 buffer in both experiments while no quenched crystals were observed at low oxygen fugacity buffered by the Mo-MoO2 buffer. Wadsleyite with the (Mg0.9,Fe0.1)2SiO4 composition melts at about 2200 ℃ at low oxygen fugacity (Ohtani et al., 1998). Therefore, this result shows that the melting temperature of wadsleyite probably be lowered by at least about 700 ℃ due to the influence of high oxygen fugacity.