日本地球惑星科学連合2014年大会

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インターナショナルセッション(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-IT03_29PO1] Structure and dynamics of Earth and Planetary deep interiors

2014年4月29日(火) 18:15 〜 19:30 3階ポスター会場 (3F)

コンビーナ:*田中 聡(海洋研究開発機構 地球内部ダイナミクス領域)、芳野 極(岡山大学地球物質科学研究センター)、亀山 真典(国立大学法人愛媛大学地球深部ダイナミクス研究センター)、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)、ヘルンランド ジョン(東京工業大学 地球生命研究所)

18:15 〜 19:30

[SIT03-P06] マグマオーシャン最深部における地球核へのカリウム分配量 -地球核の熱源への応用

*渡邉 虹水1大谷 栄治1鎌田 誠司1坂巻 竜也1宮原 正明2 (1.東北大学大学院理学研究科地学専攻、2.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:Potassium, magma ocean, high pressure, high temperature, Earth's core

Since the densities of the Earth's inner/outer cores are smaller than pure iron at the core conditions, the core has been thought to include light elements, such as H, C, S, O, Si (e.g., Poirier, 1994). Although the light element(s) in the core has not been decided yet, high-pressure experiments and cosmochemical estimations suggested that Si and O are plausible light elements. The energy causing the geodynamo is derived from the accretion energy at the early stage of the Earth, the latent heat of crystallization of the inner core, the gravitation energy associated with the exclusion of light materials from the inner core, and the radioactive decay of radioactive elements which are potentially present in the core. The Earth's core might contain long-lived radioactive elements such as U, Th, and K. In particular, potassium (K) is more depleted in the mantle than other volatile elements. Thus, potassium may be included in the core. In order to verify the amount of potassium in the core, we have performed potassium partitioning experiments under high pressure and temperature.
We studied partitioning of potassium between aluminosilicate (adularia, KAlSi3O8) and metal containing oxygen and silicon, and partitioning of potassium without light elements (Fe-O, Fe-Si, pure Fe) at pressures up to 50 GPa and 3500 K using a double-sided laser-heated diamond anvil cell. Our results for the pressure, temperature, and compositional effects on the partitioning coefficient of potassium, DK (i.e., the content of potassium in metal [wt%] divided by the content of potassium in silicate [wt%]), reveal that the temperature effect is slightly positive but weaker than that reported previously, whereas the pressure effect is negative and oxygen in metal increases the potassium content in metal, although silicon in metal has the opposite effect. According to the effects on potassium partitioning, we estimated that the amount of potassium in the core is less than 32 ppm and that it generates less than 0.14 TW heat in the core. This amount of heat is small compared with the heat flux at the core-mantle boundary (5-15 TW).