日本地球惑星科学連合2016年大会

講演情報

インターナショナルセッション(口頭発表)

セッション記号 P (宇宙惑星科学) » P-CG 宇宙惑星科学複合領域・一般

[P-CG10] Small Solar System Bodies: General and Mars Satellite Sample Return Mission

2016年5月23日(月) 09:00 〜 10:30 104 (1F)

コンビーナ:*中本 泰史(東京工業大学)、倉本 圭(北海道大学大学院理学院宇宙理学専攻)、渡邊 誠一郎(名古屋大学大学院環境学研究科地球環境科学専攻)、石黒 正晃(ソウル大学物理天文学科)、荒川 政彦(神戸大学大学院理学研究科)、安部 正真(宇宙航空研究開発機構宇宙科学研究所)、荒井 朋子(千葉工業大学惑星探査研究センター)、佐々木 晶(大阪大学大学院理学研究科宇宙地球科学専攻)、座長:荒川 政彦(神戸大学大学院理学研究科)

10:00 〜 10:30

[PCG10-16] The MMX mission

★招待講演

*藤本 正樹1 (1.宇宙航空研究開発機構・宇宙科学研究本部)

Martian Moons eXplorer (MMX) is the mission studied intensively by JAXA with the planned launch in 2022. It will explore the two moons of Mars, namely, Phobos and Deimos, and return samples from Phobos. The sampling will be done after detailed inspection of the moon from quasi-orbits around it is performed, while less detailed remote-sensing is planned for Deimos. The main objective of MMX is to understand the origin of the two Martian moons that remains controversial, with its goal being to reveal how small bodies at the outer-edge of the rocky-planet region behaved upon formation of the solar system. Mars is located at the outer-edge of the rocky-planet region, or at the gateway position to the snow line that demarcates the inner- and the outer-solar system. It is from beyond the snow line that water and volatiles were transported to the rocky planets. Without the across-the-snow-line transport, habitability is not an option for a rocky planet that was born dry inside the snow line. Small bodies, like those we find as primordial asteroids today, must have been the capsule for the transport, and thus, understanding the behavior of small bodies around the snow line during the formation of the solar system is one of the goals of planetary science as well as of MMX. In this talk, the mission scenario of MMX will be introduced and also discussed is the science strategy towards the mission goal via achieving its objectives.