JpGU-AGU Joint Meeting 2020

講演情報

[E] 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-IT26] 核ーマントルの相互作用と共進化

コンビーナ: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)、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)、土屋 卓久(愛媛大学地球深部ダイナミクス研究センター)

[SIT26-P01] Density of Fe3+-bearing magma at high pressure

坂 凛太郎1、*鈴木 昭夫1坂巻 竜也1 (1.東北大学大学院理学研究科地学専攻)

キーワード:マグマ、部分モル体積、密度、マントル、高圧力

Previous studies indicate the high concentration of Fe2O3 in the lower mantle. Even though the partial molar volume of Fe2O3 has become essential for discussing the magma in the deep mantle, there is no data of partial molar volume of Fe2O3 at high pressure and temperature. This study is aimed to obtain partial molar volume of Fe2O3 in silicate melts under high pressure. Fe3+-rich starting material was compressed by a Kawai-type multi-anvil apparatus at high pressure of above 4 GPa and high-temperature of above 1800 °C. We determined the third-order Birch-Murnaghan equation of state of melts from results of sink-float method. By combining the compression curves of melts and the equation of state of silicate melts proposed in Wakabayashi and Funamori (2013), partial molar volumes were yielded between 8 and 22 GPa and 1800 °C. These results indicate that compressibility of Fe2O3 is much higher than that of FeO within the range of 8 GPa to 22 GPa.