日本地球惑星科学連合2024年大会

講演情報

[J] ポスター発表

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-CG44] 地球惑星科学におけるレオロジーと破壊・摩擦の物理

2024年5月27日(月) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:桑野 修(国立研究開発法人 海洋研究開発機構)、清水 以知子(京都大学大学院理学研究科地球惑星科学専攻)、田阪 美樹(静岡大学 )、東 真太郎(東京工業大学 理学院 地球惑星科学系)

17:15 〜 18:45

[SCG44-P07] 幌満で採取されたかんらん岩泥から作る実験用鉱物多結晶体合成法の開発:微細構造と化学組成

*小泉 早苗1平賀 岳彦1 (1.東京大学地震研究所)

キーワード:オリビン、幌満、湿式ジェットミル、放電プラズマ焼結、化学組成

Recent deformation experiments on synthetic olivine polycrystals have shown that the addition of Ca and Al, which distribute (segregate) to grain boundaries, to olivine aggregates promotes grain boundary diffusion and weakens the aggregates (Yabe and Hiraga 2020 JGR). This result indicates that "impurities" in natural rocks dominate the strength of the upper mantle. Although it would be ideal to conduct high-temperature deformation experiments using mantle rocks to analyze their mechanical properties, this is experimentally difficult due to the nature of the samples, such as mineral distribution, grain size, and porosity.
We have developed a method to synthesize highly dense, fine-grained synthetic olivine aggregates suitable for laboratory experiments to investigate the effect of impurities in the measurement of upper mantle properties. We used sedimentary mud in the peridotite quarry as raw material. The chemical composition of the mud was found to represent the composition of various types of olivine exposed in an area of 80 km2. Jet milling of the mud in aqueous solution was used to obtain submicron powders while avoiding contamination. Pressure-assisted spark plasma sintering was applied to synthesize fine-grained (~1µm) and dense (porosity <1%) upper mantle composites. The microstructure and chemical composition of the samples will be reported in this presentation.