日本地球惑星科学連合2022年大会

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-IT17] 地球型惑星内部での液体の特性とその役割

2022年5月30日(月) 11:00 〜 13:00 オンラインポスターZoom会場 (21) (Ch.21)

コンビーナ:坂巻 竜也(東北大学大学院理学研究科)、コンビーナ:中島 陽一(熊本大学大学院先導機構)、座長:坂巻 竜也(東北大学大学院理学研究科)、中島 陽一(熊本大学大学院先導機構)

11:00 〜 13:00

[SIT17-P02] 高圧下のマグマ中に存在するFe2O3の部分モル体積

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、Fe2O3、密度、部分モル体積、マントル

Density of magma is one of the most important properties to understand the magma behavior in the interior of the Earth. Considering the composition of Earth’s magma, iron is the heaviest component and has a strong influence on the melt density. Therefore, we need to investigate the behavior of iron and iron oxides in magmas under high pressure in order to discuss the magma density in the Earth’s mantle. Since the high concentration of Fe2O3 in the lower mantle has been proposed (e.g., McCammon, 2005), the generation of Fe2O3-bearing magma at the top of lower mantle has been implied (Nakajima et al., 2019). Although the partial molar volume of Fe2O3 in magma is essential to calculate the density of magma in the deep mantle, there is no data of the partial molar volume of Fe2O3 at high pressure and temperature. Here, we obtained the partial molar volume of Fe2O3 in silicate melts under high pressure based on high-pressure density measurement of the melts. Several Fe3+-rich starting material were prepared. For high-pressure generation, we used a Kawai-type multi-anvil apparatus installed at Tohoku University. We succeeded in measuring the density of Fe2O3-bearing magma based on sink-float method (Agee and Walker, 1988; Suzuki et al., 1995). Combining the obtained melt densities and partial molar volumes of other oxides calculated from Wakabayashi and Funamori (2013), the partial molar volumes of Fe2O3 at 8, 10 and 12 GPa were determined. Assuming that the thermal expansibility of Fe2O3 is constant regardless of pressure, the compression curve of Fe2O3 in magmas was derived. Although the compressibility of Fe2O3 is larger than FeO, it was not observed that the volume crossover between Fe2O3 and “2FeO+1/2O2”. It was indicated that the Fe2O3-bearing magma is about 0.1g/cm3 lighter than the FeO-bearing magma at the top of the lower mantle.