日本地球惑星科学連合2024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-IT14] 地球深部科学

2024年5月31日(金) 09:00 〜 10:15 コンベンションホール (CH-B) (幕張メッセ国際会議場)

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)、石井 貴之(岡山大学惑星物質研究所)、飯塚 理子(早稲田大学教育学部理学科地球科学専修)、座長:飯塚 理子(早稲田大学教育学部理学科地球科学専修)、石井 貴之(岡山大学惑星物質研究所)、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)

10:00 〜 10:15

[SIT14-05] Ab Initio Calculations On The Mechanism Of The Iron Charge Disproportionation Reaction In Silicate Melts

*土屋 卓久1北口 一志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:第一原自由エネルギー計算、鉄の電荷不均化反応、マグマ・オーシャン

It is widely believed that during the growth of the proto-Earth, accretion of building blocks caused a large-scale melting and the formation of a magma ocean (MO) and the metallic core formed inside the MO through the segregation of liquid iron. The microscopic mechanisms of this process are however yet to be fully revealed so far. Recently, high-pressure experiments showed that the charge disproportionation (CD) reaction of ferous iron, 2Fe2+ = Fe3+ +Fe0, could occur in silicate melts under high pressure and temperature with producing metallic iron (Armstrong et al., 2019; Kuwahara et al., 2023), suggesting that the iron CD could be one of the mechanism of core formation in the MO. Theoretical calculations also reported that the ferric iron content increases with increasing the size of MO. The experiments however indicate an unrealistic strong pressure dependence, which implies almost all ferous iron in the MO changes to ferric at 50~60 GPa, and the computational analyses are obtained based imply on indirect analyses on the volume contrast between ferous and ferric iron in silicate melts without considering the iron CD reaction (Deng et al., 2020). Since the mechanisms of the iron CD in the MO remain largely unclear, we have performed free energy calculations of iron bearing silicate melts using the thermodynamic integration (TI) molecular dynamics (MD) method (Taniuchi and Tsuchiya, 2018) and investigated the stability of the iron CD reaction with changing pressure, temperature, and the composition of silicate melts. Results show that its stability may depend strongly on the temperature and iron concentration. The microscopic mechanisms of the reaction will be discussed.