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SUBARU/IRCS infrared spectroscopy of the Pluto
https://jaxa.repo.nii.ac.jp/records/20693
https://jaxa.repo.nii.ac.jp/records/206937422bd5b-2a52-4cb2-95a3-9f0a05e2a6f5
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | SUBARU/IRCS infrared spectroscopy of the Pluto | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | すばる望遠鏡 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | IRCS | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 冥王星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 赤外線分光法 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | エタン | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | メタン | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 適応光学 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽系 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Subaru Telescope | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | IRCS | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Pluto | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | infrared spectroscopy | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | ethane | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | methane | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | adaptive optics | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | solar system | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
その他のタイトル | ||||||
その他のタイトル | 冥王星のSUBARU/IRCS赤外分光法 | |||||
著者 |
佐々木, 貴教
× 佐々木, 貴教× 中村, 良介× 石黒, 正晃× 木下, 大輔× Sasaki, Takanori× Nakamura, Ryosuke× Ishiguro, Masateru× Kinoshita, Daisuke |
|||||
著者所属 | ||||||
東京大学 大学院理学系研究科 | ||||||
著者所属 | ||||||
宇宙開発事業団 衛星総合システム本部 | ||||||
著者所属 | ||||||
宇宙科学研究所 固体惑星科学研究系 | ||||||
著者所属 | ||||||
総合研究大学院大学 数物科学研究科 | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
National Space Development Agency of Japan Office of Satellite Technology, Research and Applications | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science Planetary Science Division | ||||||
著者所属(英) | ||||||
en | ||||||
Graduate University for Advanced Studies School of Mathematical and Physical Science | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究本部 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS) | |||||
書誌情報 |
第36回月・惑星シンポジウム en : Proceedings of the 36th ISAS Lunar and Planetary Symposium p. 173-176, 発行日 2003-11 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | New spectrum of the Pluto is presented, covering the 2.8-4.1 micrometer wavelength range. The new data show prominent absorptions of ethane ice on surface of Pluto. The present results require the mass ratio of ethane to methane to be approximately 1:10, which is much higher than the value expected from the equilibrium condensation theory. Three processes are proposed to add this surplus ethane to Pluto's surface: 1) external reservoir, 2) internal reservoir, and 3) photolysis/radiolysis. The present study could provide important implications and constraints for evolutions of the edge of the solar system, such as Pluto, Charon, and EKBOs. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0046650044 |