日本地球惑星科学連合2019年大会

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[E] 口頭発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS04] 火星と火星圏の科学

2019年5月26日(日) 09:00 〜 10:30 A02 (東京ベイ幕張ホール)

コンビーナ:宮本 英昭(東京大学)、臼井 寛裕(東京工業大学地球生命研究所)、松岡 彩子(宇宙航空研究開発機構 宇宙科学研究所 太陽系科学研究系)、Sushil K Atreya(University of Michigan Ann Arbor)、座長:Sushil Atreya

In view of unprecedented advances in our understanding of Mars, primarily due to new and ongoing observations of the planet with a number of spacecraft missions of the US, Europe and Asia, we propose a session on Mars. Mars is an object of intense scrutiny. Currently, eight spacecraft are operating at Mars, with six in orbit (Odyssey, MRO, MAVEN, Mars Express, Mangalyaan and TGO) and two on the surface (MSL-Curiosity and MER-Opportunity), the largest number ever at any given time. In addition, InSight is on track to land on Mars in November 2018, and several spacecraft are in various stages of implementation with launches scheduled for 2020 (Mars 2020, ExoMars 2020, Emirates Mars Mission Hope, Chinese Mars Mission and the Japanese Mars Terahertz Microsatellite), 2022 (ISRO's Mangalyaan 2), and 2024 (JAXA's MMX mission to explore Phobos, Deimos, and Mars). All this is a clear demonstration of public's strong fascination with and commitment to Mars exploration and the resulting scientific bonanza. Synergistic investigations with ongoing and already completed missions along with modeling studies and earth-based observations are gradually revealing the nature of Earth's most closely resembling planet that took on a different evolutionary track than our home planet. Morphology and variable phenomena seen on the surface (RSLs, e.g.) and in the atmosphere (methane) indicate that Mars is possibly currently active. Available data are providing a better understanding of Mars' present geologic and atmospheric state, climate evolution, and habitability. Thus, the scope of this session will be the recent results from a broad spectrum of Mars studies encompassing the interior, surface, atmosphere, plasma environment, and the Mars system including its two satellites. Abstracts on modelling, instrumentation and future mission plans are also encouraged.

09:45 〜 10:00

*Lihui Chai1Weixing Wan1Yong Wei1Tielong Zhang2Willi Exner3Markus Fraenz4Eduard Dubinin4Moritz Feyerabend3Uwe Motschmann3Yingjuan Ma5J. S. Halekas6 (1.Institute of Geology and Geophysics Chinese Academy of Sciences、2.Space Research Institute, Austrian Academy of Sciences, Graz, Austria、3.Institute for Theoretical Physics, TU Braunschweig, Braunschweig, Germany、4.Max Planck Institute for Solar System Research, Goettingen, Germany、5.Institute of Geophysics and Planetary Physics, University of California, Los Angeles, Los Angeles, CA, USA、6.Department of Physics and Astronomy, University of Iowa, Iowa City, IA, USA)

10:15 〜 10:30

*笠羽 康正1豊岡 雅士2青木 翔平3Mahieux Arnaud3,4中川 広務2岩渕 弘信2 (1.東北大学 惑星プラズマ・大気研究センター、2.東北大学 理学研究科 地球物理学専攻、3.Planetary Aeronomy, Belgian Institute for Space Aeronomy, Belgium 、4.University of Texas at Austin, USA )

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