日本地球惑星科学連合2022年大会

講演情報

[E] ポスター発表

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-IT19] 地球深部科学

2022年5月30日(月) 11:00 〜 13:00 オンラインポスターZoom会場 (22) (Ch.22)

コンビーナ:太田 健二(東京工業大学理学院地球惑星科学系)、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)、飯塚 毅(東京大学)、コンビーナ:土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、座長:太田 健二(東京工業大学理学院地球惑星科学系)、土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、飯塚 毅(東京大学)、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)

11:00 〜 13:00

[SIT19-P09] 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境 毅2 (1.広島大学、2.愛媛大学)


キーワード:ウォズリアイト、マントル遷移層、酸素フガシティーバッファー、熔融温度、急冷結晶

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 11 times in the range of 13.7-16.6 GPa and 1300-1500 ℃ with controlled oxygen fugacity by Re-ReO2 or Mo-MoO2 buffer. As a result, quenched crystals were observed in the range of 1500-~1900 ℃ at high oxygen fugacity with controlled oxygen fugacity by Re-ReO2 buffer while no quenched crystals were observed at low oxygen fugacity with controlled oxygen fugacity by Mo-MoO2 buffer. Wadsleyite with the (Mg0.9,Fe0.1)2SiO4 composition melts at about 2300 ℃ at low oxygen fugacity (Ohtani et al., 1998). Therefore, this result shows that the melting temperature of wadsleyite is lowered by at least about 800 ℃ due to the influence of high oxygen fugacity.