日本地球惑星科学連合2016年大会

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セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG19] Hydrogen in the Earth's interior from the crust to the core

2016年5月23日(月) 10:45 〜 12:15 201B (2F)

コンビーナ:*Mysen Bjorn(Geophysical Laboratory, Carnegie Inst. Washington)、大谷 栄治(東北大学大学院理学研究科地学専攻)、井上 徹(愛媛大学地球深部ダイナミクス研究センター)、座長:Bjorn Mysen(Geophysical Laboratory, Carnegie Inst. Washington)

12:00 〜 12:15

[SCG19-12] Hydrogen solubility into Fe-alloys under high pressure

*寺崎 英紀1柴崎 裕樹2肥後 祐司3 (1.大阪大学大学院理学研究科、2.東北大学大学院理学研究科、3.高輝度光科学研究センター)

キーワード:Hydrogen, Fe-alloy, core

Hydrogen, the most abundant element in the solar system, is known to incorporate into Fe and form FeHx above 3 GPa. The solubility of H in Fe is closely linked to light element in the terrestrial core and H reservoir in the planet interiors. In order to understand more realistic case of H in planet interiors, H solubility into Fe-alloys (such as Fe-Si, Fe-C, and Fe-S) needs to be clarified.
In this study, we have performed in situ X-ray diffraction measurements combined with Kawai-type multianvil press under high pressures and temperatures to study H solubility in FeSi and Fe3C. H solubility can be estimated from a volume expansion associated with hydrogen incorporation into metal. The lattice volumes and phase relations of FeSi-H and Fe3C–H systems were measured up to 19 GPa and 1973 K.
H starts to dissolve in FeSi and form FeSiHx (x=0.07-0.22) above 10 GPa, suggesting that presence of Si in metal increases the minimal pressure for H incorporation. H incorporation into Fe3C does not occur and H is unlikely to coexist with C in Fe-alloy up to 14 GPa (Terasaki et al. 2014). Therefore, hydrogenation pressures of Fe-alloys are different from that of pure Fe and more pressure is required for H incorporation into the Fe-alloy core.