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Detailed mapping and statistical analysis of Noachian and post-Noachian valley networks: implications to the history of martian surface environment
https://jaxa.repo.nii.ac.jp/records/20346
https://jaxa.repo.nii.ac.jp/records/2034647cf830a-8e26-4ae5-8b06-34b844e64a23
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 | Detailed mapping and statistical analysis of Noachian and post-Noachian valley networks: implications to the history of martian surface environment | |||||
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 |
山口, 優夢
× 山口, 優夢× 宮本, 英昭× Yamaguchi, Yuumu× Miyamoto, Hideaki |
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著者所属 | ||||||
東京大学総合研究博物館 | ||||||
著者所属 | ||||||
東京大学総合研究博物館 | ||||||
著者所属(英) | ||||||
en | ||||||
Univerisity Museum, University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Univerisity Museum, 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本部 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
月・惑星シンポジウム en : Proceedings of the ISAS lunar and planetary symposium 巻 42, p. 8-11, 発行日 2009-08 |
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会議概要(会議名, 開催地, 会期, 主催者等) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 第42回 月・惑星シンポジウム(2009年8月5-7日, 宇宙航空研究開発機構宇宙科学研究本部) | |||||
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 | The 42nd ISAS Lunar and Planetary Symposium (August 5-7, 2009. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), Sagamihara, Kanagawa Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Using THEMIS-IR and Viking images and MOLA topography data, we mapped clusters of valley networks, which dissect Noachian and post-Noachian terrains, and thus are representative of Noachian and more geologically recent surface environments. In the Naktong Vallis and surrounding region, 36 major Noachian valley network systems, whose total length is greater than 66,000 sq km, were mapped, characterized, and compiled. Drainage areas range from 9,000 to 210,000 km2 and the drainage densities from 0.07 to 0.63. We find strong correlation between the mean slopes and the drainage densities in this Noachian terrain, indicating that the drainage density was likely controlled by the overall slope of the precipitation area at the time of valley network formation. We also map post-Noachian valley networks, which dissect the flanks of Uranius, Ceraunius, and Hecates Tholi and Hadriaca and Apollinaris Paterae. The correlation between drainage densities and mean slopes does not exist in every case, indicating that the valley network formational process varied locally. For example, whereas local precipitation may have been more influential in valley network formation on the flanks of Hadriaca and Apollinaris Paterae, other processes may have been more dominant in the dissection of the flanks of Uranius, Ceraunius, and Hecates Tholi. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
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 | Physical characteristics: Original contains color illustrations | |||||
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: AA0064739002 |