日本地球惑星科学連合2021年大会

講演情報

[E] 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-CG17] 宇宙・惑星探査の将来計画および関連する機器開発の展望

2021年6月3日(木) 15:30 〜 17:00 Ch.02 (Zoom会場02)

コンビーナ:小川 和律(宇宙航空研究開発機構)、尾崎 光紀(金沢大学理工研究域電子情報学系)、坂谷 尚哉(立教大学 理学部 物理学科)、吉岡 和夫(東京大学大学院新領域創成科学研究科)、座長:尾崎 光紀(金沢大学理工研究域電子情報学系)

15:30 〜 16:15

[PCG17-01] JAXAʼs Strategic Mars Exploration Program (JSMEP) for Understanding the Origin, Evolution, Inventory of Water on Mars

★Invited Papers

*臼井 寛裕1 (1.宇宙航空研究開発機構)

キーワード:火星、火星探査プログラム、水

The Mars-moon system is a promising target for exploration in the broad field of planetary science: e.g., geology, geochemistry, astrobiology, and comparative planetology. The international Mars science community has set a long-term goal toward achieving Mars sample return (MSR) and human exploration. MSR will address questions on the origin (e.g., source of building blocks), interior evolution (e.g., crust-mantle differentiation and mantle dynamics), the potential biological history (e.g., nature and extent of habitability and preservation of biosignature), and geologic history of Mars with an emphasis on the role of water. Previous Mars exploration missions have provided compelling evidence for the presence of liquid water during the earliest geologic era (Noachian: >~3.9 Ga) of Mars. Observations of dense valley networks, evaporites (e.g., gypsum) and hydrous minerals (e.g., clays) that are commonly formed by aqueous processes imply that, at some time in the past, Mars had an Earth-like active hydrological cycle with lakes, oceans, possibly also aquifers and groundwater, and had the potential for life.
According to the international trend for Mars exploration and potential significance for understanding the current and past surface/subsurface aqueous environments, JAXA plans a strategic Mars exploration program (JSMEP). JSMEP starts with a Martian moon’s sample return mission (MMX: Martian Moons Explorer) in 2024-2029, followed by a Mars orbiter (MO) in later 2020s and a Mars lander/rover (ML/R) mission in early 2030s. JSMEP’s goals are 1) to address questions of water on Mars [origin and delivery (MMX), distribution and inventory (MO), and chemical evolution (ML/R)], 2) to ensure the expansion of the areas of human activities by exploring the habitable subsurface world, and 3) to acquire key technologies including EDL (entry-descent-landing) with aerodynamic control, drilling and sampling on the surface, deep space telecommunication, transportation to/from the Mars orbit, and planetary protection.