セッション情報
[E] ポスター発表
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) 15:30 〜 17:00 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: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)
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.
*Reid Parsons1、Hideaki Miyamoto1 (1.University of Tokyo)
*神崎 友裕1、Reid Parsons1,2、逸見 良道1、宮本 英昭1 (1.東京大学、2.フィッチバーグ州立大学)
*吉村 義隆1、山岸 明彦2、佐藤 毅彦3、宮川 厚夫2、今井 栄一4、佐々木 聰5、小林 憲正6、癸生川 陽子6、岡田 朋華6、塩谷 圭吾3、薮田 ひかる7、長沼 毅7、三田 肇8、藤田 和央3、臼井 寛裕3 (1.玉川大学農学部、2.東京薬科大学、3.宇宙航空研究開発機構、4.長岡技術科学大学、5.東京工科大学、6.横浜国立大学、7.広島大学、8.福岡工業大学)
*Brian Hamilton Day1、Emily Law2 (1.NASA Solar System Exploration Research Virtual Institute, NASA Ames Research Center、2.NASA Jet Propulsion Laboratory, California Institute of Technology)
*小森 信男1 (1.東京学芸大学大学院連合学校教育学研究科)