*Takehiro Hirose1, Takazo Shibuya2 (1.Kochi Institute for Core Sample Research, Japan Agency for Marine-Earth Science and Technology, 2.JAMSTEC)
Session information
[JJ] Poster
M (Multidisciplinary and Interdisciplinary) » M-IS Intersection
[M-IS18] Aqua planetology
Tue. May 22, 2018 10:45 AM - 12:15 PM Poster Hall (International Exhibition Hall7, Makuhari Messe)
convener:Yasuhito Sekine(Department of Earth and Planetary Science, University of Tokyo), Tomohiro Usui(Earth-Life Science Institute, Tokyo Institute of Technology), Hidenori Genda(東京工業大学 地球生命研究所, 共同), Takazo Shibuya(Japan Agency for Marine-Earth Science and Technology)
This proposed session covers a wide range of topics related to aqua planetology, including chemical reactions involving water on planetary bodies, water-rock reactions within planetesimals, distribution of water in the early Solar system and the origin of water on terrestrial planets, hydrological and biogeochemical processes on Earth, geochemical cycles and habitability on Mars and icy moons, exploration of water in the solar system, and theory to understand how to build a habitable aqua planet.
*Kaho Harada1, Takashi Nakagawa2, Manabu Morishige2 (1.Keio University, 2.Japan Agancy for Marine-Earth Science and Technology)
*Yuhki Matsuoka1, Ikuo Katayama1 (1.Department of Earth and Planetary Systems Science, Hiroshima University)
*Hiromu Nakagawa1, Naoki Terada1, Shohei Aoki1, Takeshi Kuroda2, Yasumasa Kasaba1 (1.Planetary Atmosphere Physics Laboratory, Department of Geophysics, Graduate School of Science, Tohoku University, 2.National Institute of Information and Communications Technology)
*Hiroki Shozaki1, Hitoshi Hasegawa1 (1.Faculty of Science and Technology, Kochi University)
*Keisuke Fukushi1, Yasuhito Sekine2 (1.Institute of Nature & Environmental Technology, Kanazawa University, 2.Department of Earth & Planetary Science, The University of Tokyo)
*Takufumi Chida1, Yasuhito Sekine1, Keisuke Fukushi2, Haruna Matsumiya2, Tsetsgee Solongo2, Noriko Hasebe2, Davaadorj Davaasuren3 (1.Department of Earth and Planetary Science, University of Tokyo, 2.Institute of Nature and Environmental Technology, Kanazawa University, 3.National University of Mongolia)
*Maya Nakamura1, Yasuhito Sekine1, Keisuke Fukushi2, Takazo Shibuya3, Noriko Hasebe2, Jaahanaa Davaadorj4, Yoshio Takahashi1 (1.Department of Earth and Planetary Science, The University of Tokyo, 2.Institute of Nature & Environmental Technology, Kanazawa University, 3.Japan Agency for Marine-Earth Science and Technology, 4.Department of Geography, National University of Mongolia)
*Takazo Shibuya1, Sakiko Kikuchi1, Mariko Abe1, Yasuhito Sekine2 (1.Japan Agency for Marine-Earth Science and Technology, 2.University of Tokyo)
*Hiroyuki Kurokawa1, Bethany L Ehlmann2,3, Eleonora Ammannito4, Maria Cristina De Sanctis5, Mathieu G. A. Lapotre6, Tomohiro Usui1, Nathaniel T. Stein2, Thomas Prettyman7, Andrea Raponi5, Mauro Ciarniello5 (1.Earth-Life Science Institute, Tokyo Institute of Technology, 2.California Institute of Technology, 3.Jet Propulsion Laboratory, 4.Agenzia Spaziale Italiana, 5.Institute for Space Astrophysics and Planetology, National Institute for Astrophysics, 6.Harvard University, 7.Planetary Science Institute)
Hoki Ka1, *Tomoki Nakamura1, Moe Matsuoka1, Yuma Enokido1, Yuya Sato1, Masakuni Yamanobe1 (1.Department of Earth and Planetary Materials Sciences, Faculty of Science, Tohoku University)
*Yasuhito Sekine1, Kenya Kodama1, Takamichi Kobayashi2, Seiji Obata1, Yu Chang1, Nanako O. Ogawa3, Yoshinori Takano3, Naohiko Ohkouchi3, Koichiro Saiki1, Toshimori Sekine4 (1.University of Tokyo, 2.National Institute for Materials Science, 3.JAMSTEC, 4.Center for High Pressure Science and Technology Advanced Research)