日本地球惑星科学連合2018年大会

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[EE] 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-IT22] 核-マントルの相互作用と共進化

2018年5月23日(水) 13:45 〜 15:15 国際会議室(IC) (幕張メッセ国際会議場 2F)

コンビーナ:飯塚 毅(東京大学)、渋谷 秀敏(熊本大学大学院先端科学研究部基礎科学部門地球環境科学分野)、土屋 卓久(愛媛大学地球深部ダイナミクス研究センター、共同)、太田 健二(東京工業大学大学院理工学研究科地球惑星科学専攻)、座長:太田 健二飯塚 毅

13:45 〜 14:00

[SIT22-25] Composition of the outermost outer core estimated from thermoelastic properties of liquid Fe alloys

*市川 浩樹1土屋 卓久2 (1.東京工業大学 地球生命研究所、2.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:外核組成、外核最上部層、軽元素

The Earth's core is thought to include substantially large amounts of light elements (LEs), which account for observed density deficits of ~10% for the liquid outer core and ~5% for the solid inner core. Although studies have been made on candidate LEs such as oxygen, silicon, carbon, nitrogen, sulfur, and hydrogen, there is no established compositional model of the core so far due to technical difficulties in experiments and a lack of observational data. However, recent reports of low-velocity anomalies (VP=0.03-0.1 km/s) observed at the outermost 100-300 km of the outer core give another new constraint on the composition of the core. Due to the gravitational stability, such a layer should have a lower density than the ambient outer core liquid. Therefore, it seems reasonable to assume that the outermost layer consists of the LE-rich liquid. However, the sole LE incorporation leads to the increase of VP of the liquid iron due to the reduction of its density. Therefore, complicated processes such as exchanges of two LE species might be responsible. The dynamically stable and chemically distinct topmost LE layer can be created either by the interaction at the CMB, the incomplete mixing of core merging, or the residue from crystallization.


Here, we show integrative analyses of the compositional model of the Earth’s outer core based on the ab initio thermoelasticity and diffusivity of iron-nickel-LE alloy liquids in order to restrict the both compositions of the outermost layer and the entire outer core.