日本地球惑星科学連合2021年大会

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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-IT15] 地球深部科学 - 核・マントルの相互作用と共進化

2021年6月4日(金) 10:45 〜 12:15 Ch.24 (Zoom会場24)

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

11:45 〜 12:00

[SIT15-05] Hf and W partitioning between liquid metal and liquid silicate and resultant core-mantle interaction signature on the 182W isotope of the Afar plume

*鈴木 勝彦1、賞雅 朝子2,1、土屋 卓久3、深海 雄介4、折橋 裕二5、新城 竜一6 (1.海洋研究開発機構・海底資源センター、2.日本エヌ・ユー・エス株式会社、3.愛媛大学・地球深部ダイナミクス研究センター、4.学習院大学・化学科、5.弘前大学・理工学部地球環境防災学科、6.琉球大学・理学部物質地球科学科)

キーワード:核-マントル相互作用、HfとWの分配、タングステン同位体

Low 182W/184W relative to the average value of modern mantle have been found in certain modern ocean island basalts such as the ones from Hawaii and Samoa (i.e, Rizo et al., 2019; Mundl-Petermeier et al., 2020). The most plausible process among the proposed models for such 182W variations is the one including the fractionation of Hf-W in core separation from the mantle due to the affinity of W to metal. This process leads to a low 182W of the metallic core, which may have contributed to the source of the ocean island basalt.
Here we report the evidence of the Hf-W fractionation under the lowermost mantle condition in core segregation in the early Earth. First-principles free energy calculations reveal that W is strongly partitioned into the liquid metal phase, while Hf remains in the molten silicate even at the core-mantle boundary P,T condition. Such Hf-W fractionation imparts a low 182W property to the core.
We present slightly negative 182W anomalies relative to the average present-day mantle for the Ethiopian basalts, which is closely related to the Afar mantle plume and non-resolvable 182W isotope for the Aden Bay MORB. The basalt samples were analyzed following the modified procedure from Takamasa et al. (2020). The low 182W isotope values indicated the Afar mantle plume generating the Ethiopian basalts were originated from the lowermost mantle and likely contained the core component with low 182W isotope values, which was likely to be diffused from the core (Yoshino et al., 2019).