*Yamada Iori1, Hidenori Terasaki2, Asaka Kamiya1, Keisuke Nishida3, Yuki Shibazaki4, Tatsuya Sakamaki4, Yuji Higo5, Yoshinori Tange5, Tadashi Kondo2 (1.Osaka University, 2.Graduate School of Science, Osaka University, 3.Graduate School of Science, Tokyo University, 4.Graduate School of Science, Tohoku University, 5.Japan Synchrotron Radiation Research Institute)
Session information
[EE] Poster
S (Solid Earth Sciences) » S-IT Science of the Earth's Interior & Tectonophysics
[S-IT18] Planetary cores: Structure, formation, and evolution
Mon. May 21, 2018 10:45 AM - 12:15 PM Poster Hall (International Exhibition Hall7, Makuhari Messe)
convener:Hidenori Terasaki(Graduate School of Science, Osaka University), Eiji Ohtani(Department of Earth and Planetary Materials Science, Graduate School of Science, Tohoku University), William F McDonough (共同), George Helffrich(Earth-Life Science Institute, Tokyo Institute of Technology)
There are fundamental links between the formation and evolution of planets and their satellites to that of their cores. Defining the physical and chemical properties of the cores of these terrestrial bodies are fundamental for understanding their internal structures and thermal profile. Recent advances in experimental and theoretical studies provide new insights and applications to the Earth's cores and other terrestrial bodies. Future exploration missions will obtain data on the internal structure of terrestrial planets (e.g., Mars and Mercury) and planet-satellite systems. We anticipate presentations on recent advances on the physical and chemical properties of cores and discussions regarding the latest views of their formation and evolution. We welcome contributions from mineral/rock physics, geophysics, geochemistry, geodynamics, and planetary science.
*Hidenori Terasaki1, Attilio Rivoldini2, Yuta Shimoyama1, Keisuke Nishida3, Satoru Urakawa4, Fuyuka Kurokawa1, Yusaku Takubo1, Yuki Shibazaki5, Tatsuya Sakamaki5, Akihiko Machida6, Yuji Higo7, Tadashi Kondo1 (1.Graduate School of Science, Osaka University, 2.Royal observatory of Belgium, 3.Graduate School of Science, The University of Tokyo, 4.Graduate School of Natural science and technology, Okayama University, 5.Graduate School of Science, Tohoku University, 6.QST, 7.JASRI)
Takaaki Katsura1, *Hiroaki TOH2 (1.Division of Earth and Planetary Sciences, Graduate School of Science, Kyoto University, 2.Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University)
*Chao Liu1, Takashi Yoshino1 (1.Institute for Planetary Materials, Okayama University)
*George Helffrich1, Guillaume Morard3, Kei Hirose1,2, Satoshi Kaneshima4 (1.Earth-Life Science Institute, Tokyo Institute of Technology, 2.Department of Earth and Planetary Science, University of Tokyo, 3.IMPMC, Universite Pierre et Marie Curie - Paris 6, 4.Department of Earth and Planetary Sciences, University of Kyushu)
Takashi Fujikawa1, *Tatsuhiro Sakaiya1, Hidenori Terasaki1, Tadashi Kondo1, Keisuke Shigemori2 (1.Graduate School of Science, Osaka University, 2.Institute of Laser Engineering, Osaka University)