日本地球惑星科学連合2018年大会

講演情報

[EE] Evening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-IT20] Structure and Dynamics of Earth and Planetary Mantles

2018年5月21日(月) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 7ホール)

コンビーナ: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)、中川 貴司(海洋研究開発機構数理科学・先端技術研究分野)

[SIT20-P09] Coupled substitution of Fe3+ and H+ for Si in wadsleyite

*川添 貴章1 (1.広島大学大学院理学研究科地球惑星システム学専攻)

キーワード:ウォズリアイト、水、水素、三価のFe、Si

Wadsleyite is the most abundant mineral in the upper part of the mantle transition zone (MTZ) and can incorporate up to 3 wt% water in its crystal structure. Incorporation of water (or hydrogen) in wadsleyite influences its elasticity, atomic diffusivity, creep strength, crystallographic preferred orientation, grain-growth kinetics and electrical conductivity. Moreover, water affects phase boundaries relevant to wadsleyite. Consequently, determination of the substitution mechanisms of hydrogen in wadsleyite is fundamentally important to addressing the effects of water on the above properties of the upper MTZ. The major substitution mechanism of hydrogen in Fe-free hydrous wadsleyite is protonation of oxygen having no bonding to Si (non-silicate oxygen, O1). Recently, coupled substitution of Fe3+ and H+ for Si was proposed as a new protonation mechanism in Fe-bearing hydrous wadsleyite (Bolfan-Casanova et al. 2012; Smyth et al. 2014; Kawazoe et al. 2016). I will review the previous studies and introduce experimental evidence to support the coupled substitution of Fe3+ and H+ for Si in wadsleyite.