日本地球惑星科学連合2014年大会

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セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS02_28AM1] Mars

2014年4月28日(月) 09:00 〜 10:45 418 (4F)

コンビーナ:*佐藤 毅彦(宇宙航空研究開発機構・宇宙科学研究本部)、石渡 正樹(北海道大学大学院理学院宇宙理学専攻)、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)、高橋 芳幸(惑星科学研究センター)、佐々木 晶(大阪大学大学院理学研究科宇宙地球科学専攻)、宮本 英昭(東京大学総合研究博物館)、座長:石渡 正樹(北海道大学大学院理学院宇宙理学専攻)

10:30 〜 10:45

[PPS02-05] Development of a dust imager for Mars landing mission

*佐藤 毅彦1小郷原 一智2はしもと じょーじ3三浦 和彦4間野 高明5 (1.Japan Aerospace Exploration Agency、2.University of Shiga Prefecture、3.Okayama University、4.Tokyo University of Science、5.National Institute for Materials Science)

キーワード:Mars, dust, imager, landing, mission

We report progress in developing a dust imager for future Mars landing missions. As Martian dust is a key element of its environment and a potential hazard for human exploration, it is essential to know what is Martian dust and how it works. However, little is known about the Martian dust due primarily to lack of measurements. Direct imaging would greatly increase our knowledge about the Martian dust (previously, an Atomic-Force Microscope onboard Phoenix acquired just one image).The dust imager under development is not a microscope but a "bare" imaging sensor of which pixels are fine pitched. After exposing the sensor to the air with dust for a while, we illuminate the sensor with a parallel beam so that shadows of particles on the sensor are directly imaged. In this way, the imager does not need a focusing mechanism and is expected to be very light-weighted and robust. Although the status is still the laboratory-experiment level, this small tool would greatly contribute to the Mars science and exploration.