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Habitable Zones of Land Planets: A Study with 1D EBM
https://jaxa.repo.nii.ac.jp/records/20289
https://jaxa.repo.nii.ac.jp/records/20289500ddc95-cb49-4e89-be50-fc3f29f39e9c
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 | Habitable Zones of Land Planets: A Study with 1D EBM | |||||
言語 | ||||||
言語 | eng | |||||
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 | |||||
著者 |
Takao, Yuya
× Takao, Yuya× Genda, Hidenori× Kodama, Takanori× Abe, Yutaka |
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著者所属 | ||||||
東京大学大学院理学系研究科地球惑星科学専攻 | ||||||
著者所属 | ||||||
東京大学大学院理学系研究科地球惑星科学専攻 | ||||||
著者所属 | ||||||
東京大学大学院理学系研究科地球惑星科学専攻 | ||||||
著者所属 | ||||||
東京大学大学院理学系研究科地球惑星科学専攻 | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Earth and Planetary Science, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Earth and Planetary Science, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Earth and Planetary Science, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Earth and Planetary Science, University of Tokyo | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | |||||
書誌情報 |
en : Proceedings of the 44th ISAS Lunar and Planetary Symposium 巻 44, 発行日 2011 |
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会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 44th ISAS Lunar and Planetary Symposium (August 1-3, 2011. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Planets with very little amount of water on their surface, called "land planets", have wider habitable zones than that of Earth-like "aqua planets" (Abe et al. (2011)). We investigated complete evaporation of liquid water on the ground of land planets using 1D energy balance model (EBM) with the transport of ground water. We found that the complete evaporation of ground water is controlled by the insolation and the latitude of dry edge, which is the boundary between the dry zone and the wet zone. Dry edge is determined by balance between the transport of water vapor in the atmosphere and liquid water on the ground. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: CD-ROM1枚 | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Note: One CD-ROM | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA12268968 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0065390004 |