セッション詳細

[P-PS07]火星と火星圏の科学

2018年5月20日(日) 9:00 〜 10:30
201A 幕張メッセ国際会議場 2F
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、共同)、Sushil K Atreya (University of Michigan Ann Arbor)、座長:松岡 彩子、Sushil Atreya
Unprecedented progress in being made in our understanding of the planet Mars, especially because of new data from the US, European, Russian, and Asian missions to Mars. Eight spacecraft are currently 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 Lander is on track for launch in 2018, and Mars 2020, ExoMars and the Emirates Mars Mission in 2020. 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 or 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. Morphology and variable phenomena seen on the surface (RSLs, for example) indicate the red planet may possibly be still active, and require a clear understanding of its current geologic and atmospheric state, climate evolution and habitability. Thus, this session is planned to discuss 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 instrumentation and future mission plans are also encouraged for this session, as both the presenters and the audience would greatly benefit from ensuing discussions and feedbacks.

[PPS07-01]A coupled atmosphere–hydrosphere global climate model of early Mars: “cool and wet” scenario for the formation of water channels★招待講演

Kamada Arihiro1、*Kuroda Takeshi2,1、笠羽 康正1、Terada Naoki1、Nakagawa Hiromu1、Toriumi Katsushige1 (1.Dep. Geophysics, Graduate School of Science, Tohoku University、2.National Institute of Information and Communication Technology)

[PPS07-02]放射冷却が原始火星大気の流体力学的散逸に与える影響

*吉田 辰哉1、倉本 圭1 (1.北海道大学)

[PPS07-03]Wavenumber-frequency spectra in the Mars atmosphere: the 2 sols waves in low latitudes

*小郷原 一智1 (1.滋賀県立大学工学部)

[PPS07-04]Observation of secondary ions emitted from Phobos by the mass spectrum analyzer on Martian Moons eXploration (MMX)

*横田 勝一郎1、松岡 彩子2、寺田 直樹3、野村 麗子4、斎藤 義文2、加藤 大羽5 (1.大阪大学大学院・理学研究科、2.宇宙航空研究開発機構宇宙科学研究所、3.東北大学大学院・理学研究科、4.宇宙航空研究開発機構、5.東京大学大学院・理学系研究科)

[PPS07-05]回転原始火星大気による衛星前駆天体の捕獲と衛星軌道進化

*松岡 亮1、倉本 圭1 (1.北海道大学大学院理学院宇宙理学専攻)

[PPS07-06]High-resolution digital elevation models of Phobos derived from HiRISE stereo images

*逸見 良道1、宮本 英昭1 (1.東京大学)