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-IT18] Planetary cores: Structure, formation, and evolution

2018年5月21日(月) 13:45 〜 15:15 A11 (東京ベイ幕張ホール)

コンビーナ:寺崎 英紀(大阪大学大学院理学研究科)、大谷 栄治(東北大学大学院理学研究科地学専攻)、William F McDonough (共同)、George Helffrich(Earth-Life Science Institute, Tokyo Institute of Technology)、座長:寺崎 英紀McDonough William(University of Maryland / Tohoku University)

14:30 〜 14:45

[SIT18-04] Elastic wave velocity of Fe-Si alloy at high pressure

*坂巻 竜也1寺崎 英紀2柴崎 裕樹1戸邉 宙1下山 裕太2肥後 祐司3鈴木 昭夫1 (1.東北大学大学院理学研究科、2.大阪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:鉄-珪素合金、弾性波速度、高圧

As an approach to understanding planetary cores, a determination of the elastic property of iron-alloys is powerful. Here, we report both of elastic velocity and density of Fe-Si alloy up to 6 GPa and 1873 K using ultrasonic technique combining with synchrotron x-ray at BL04B1 of SPring-8. In this experiment, Fe-10at%Si system showed three phases (bcc, fcc, bcc+fcc) depending on pressure and temperature conditions. This indicated that a stability field of fcc phase is large compared to ambient condition. Based on the velocity measurements, negative temperature effect on the velocity was found clearly. The phase transition from bcc to fcc around 6 GPa and 1000 K caused small changes in properties: the density and velocity (Vp) jump are 1.2% and 0.8%, respectively. Comparing with pure-iron (bcc), the bcc-Fe-Si is 10% faster at the same density. These knowledges can help us to analyze new planetary observations in the near future.