Observations of and its satellites by the Mars Imaging Camera (MIC) on Planet-B.
スポンサーリンク
概要
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We present the specifications of the Mars Imaging Camera (MIC) on the Planet-B spin-stabilized spacecraft, and key scientific objectives of MIC observations. A non-sun-synchronous orbit of Planet-B with a large eccentricity of about 0.87 around Mars provides the opportunities (1) to observe the same region of Mars at various times of day and various solar phase angles with spatial resolution of about 60 m from a distance of 150 km altitude (at periapsis), and (2) to monitor changes of global atmospheric conditions on Mars near an apoapsis of 15 Mars radii. In addition, (3) several encounters of Planet-B with each of the two Martian satellites are scheduled during the mission lifetime of two years from October 1999 to observe their shapes and surface structures with three color filters, centered on 450, 550, and 650 nm. (4) A search for hypothetical dust rings along the orbits of two satellites will be tried from the forward-scattering region of sunlight.
- 公益社団法人 日本地震学会、地球電磁気・地球惑星圏学会 、特定非営利活動法人 日本火山学会、日本測地学会、日本惑星科学会の論文
著者
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TOIGO Anthony
Division of Geological and Planetary Sciences, California Institute of Technology
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ABE Yutaka
Space and Planetary Science, University of Tokyo
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Inada Ai
The Graduate School Of Science And Technology Kobe University
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Sasaki Sho
Geological Institute University Of Tokyo
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Kurita Kei
Space And Planetary Science University Of Tokyo
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Hashimoto Tatsuaki
Institute Of Space And Astronautical Science
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Imamura Takeshi
Space And Planetary Science University Of Tokyo
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Akabane Tokuhide
Hida Observatory Kyoto University
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Nakamura Masato
Space And Planetary Science University Of Tokyo
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Mukai Tadashi
The Graduate School Of Sci. And Tech. Kobe Univ.:faculty Of Science Kobe University
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Ishimoto Hiroshi
The Graduate School Of Sci. And Tech. Kobe Univ.
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