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[E] ポスター発表
セッション記号 P (宇宙惑星科学) » P-CG 宇宙惑星科学複合領域・一般
[P-CG22] Shock responses of planetary materials elucidated from meteorites and dynamic compression experiments
2019年5月28日(火) 10:45 〜 12:15 ポスター会場 (幕張メッセ国際展示場 8ホール)
コンビーナ:関根 利守(Center for High Pressure Science and Technology Advanced Research)、奥地 拓生(岡山大学惑星物質研究所)
Impact phenomena had played essential roles in the process of planetary evolution. Recent analytical and experimental developments reveal a new prospective on the effects of shock-compression process for planetary materials. For deeper understanding of such shock effects, it is necessary to evaluate the detailed shock conditions from the observations of naturally-shocked planetary materials, and to compare them with the results on the planetary materials experienced a wide range of known shock conditions. Several metastable phases, that have not been known before, have recently been identified in shocked meteorites. They suggest that the shock state is often not in equilibrium and that it is more complicated process than ever thought. Experimental techniques including laser-driven shock compression and x-ray free electron laser diagnostics have been progressed to successfully simulate a wide range of shock conditions. The recent results indicate that shocked grains are fractured and rotated at relatively low pressures, and that they are subsequently transformed into denser phases or melts, or their mixtures at pressures of a few 100s GPa. Understanding of such shock dynamics requires another prospect, which is qualitatively different from the static high pressure and high temperature consensus. Therefore, it is timely to have an international symposium on dynamics of planetary materials.
*佐藤 友子1、丹下 慶範2、瀬戸 雄介3、関根 利守4,5、尾崎 典雅4、西川 豊人4、宮西 宏併4、松岡 健之4、兒玉 了祐4、富樫 格2、犬伏 雄一2、籔内 俊毅6、矢橋 牧名6 (1.広島大学、2.高輝度光科学研究センター、3.神戸大学、4.大阪大学、5.北京高压科学研究中心、6.理化学研究所)
*Narangoo Purevjav1、Takuo Okuchi1、Norimasa Ozaki2、Takayoshi Sano3、Yuhei Umeda2、Shintaro Morioka2、Nobuki Kamimura2 (1.Institute for Planetary Materials, Okayama University、2.Graduate School of Engineering, Osaka University、3.Institute of Laser Engineering, Osaka University)
*佐野 孝好1 (1.大阪大学レーザー科学研究所)
*Chi Pui Tang1、Pak Kin Leong1、Toshimori Sekine2,3 (1.State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology、2.Center for High Pressure Science and Technology Advanced Research (HPSTAR) Shanghai Laboratory of HPSTAR, Shanghai, P.R. China、3.Graduate School of Engineering, Osaka University)
*林 秀幸1、三河内 岳1、佐野 有司1、Bizzarro Martin2 (1.東京大学、2.コペンハーゲン大学)
*福井 敬也1、尾崎 典雅1,2、梅田 悠平1、宮西 宏併3、片桐 健登1、森岡 信太郎1、佐野 孝好3、兒玉 了佑1,2,3 (1.大阪大学大学院工学研究科、2.大阪大光科学センター、3.大阪大学レーザー科学研究所)