WEKO3
アイテム
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Temperature constraint on formation mechanism of recent gullies on Mars
https://jaxa.repo.nii.ac.jp/records/20667
https://jaxa.repo.nii.ac.jp/records/20667da566f9d-f265-4c10-a686-43322dab7a15
Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Temperature constraint on formation mechanism of recent gullies on Mars | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 火星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 温度の制約 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 表面温度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 溝形成 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 水 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | モデル | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 熱拡散 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 火星大気 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Mars | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | temperature constraint | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | surface temperature | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | gully formation | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | water | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | model | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | thermal diffusion | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Martian atmosphere | |||||
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 | 火星表面の最近における溝の生成機構に対する温度制約 | |||||
著者 |
石井, 徹之
× 石井, 徹之× 佐々木, 晶× Ishii, Tetsuyuki× Sasaki, Sho |
|||||
著者所属 | ||||||
東京大学 大学院理学系研究科 | ||||||
著者所属 | ||||||
東京大学 大学院理学系研究科 | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo Graduate School of Science | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo Graduate School of 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. 69-72, 発行日 2003-11 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The observation of recent gullies related to a possibility of the existence of liquid water on present Mars has been concerned in recent years. Some models assume formation of gullies by liquid water but they cannot explain the absence of the features in the equator regions. Other models assume CO2 as a volatile associated with the formation of gullies. It is shown that a latitude of the boundary between regions with CO2 consolidation on poleward-facing slops and those without CO2 condensation is about a latitude of 30 deg. The result suggests a possibility of some correlation between the existence of CO2 and the formation of gullies. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0046650018 |