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The Shape and Interior Structure of the South Pole-Aitken Basin from KAGUYA Selenodesy Data
https://jaxa.repo.nii.ac.jp/records/20295
https://jaxa.repo.nii.ac.jp/records/2029569b11fdd-e444-4dfc-b093-72082c06b73f
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 | The Shape and Interior Structure of the South Pole-Aitken Basin from KAGUYA Selenodesy Data | |||||
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 |
佐々木, 晶
× 佐々木, 晶× 石原, 吉明× 松本, 晃治× 花田, 英夫× 荒木, 博志× 野田, 寛大× 岩田, 隆浩× 並木, 則行× Sasaki, Sho× Ishihara, Yoshiaki× Goossens, Sander× Matsumoto, Koji× Hanada, Hideo× Araki, Hiroshi× Noda, Hirotomo× Iwata, Takahiro× Namiki, Noriyuki |
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著者所属 | ||||||
国立天文台RISE月探査プロジェクト | ||||||
著者所属 | ||||||
国立天文台RISE月探査プロジェクト | ||||||
著者所属 | ||||||
国立天文台RISE月探査プロジェクト | ||||||
著者所属 | ||||||
国立天文台RISE月探査プロジェクト | ||||||
著者所属 | ||||||
国立天文台RISE月探査プロジェクト | ||||||
著者所属 | ||||||
国立天文台RISE月探査プロジェクト | ||||||
著者所属 | ||||||
国立天文台RISE月探査プロジェクト | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) | ||||||
著者所属 | ||||||
千葉工業大学惑星探査研究センター | ||||||
著者所属(英) | ||||||
en | ||||||
RISE Project, National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
RISE Project, National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
RISE Project, National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
RISE Project, National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
RISE Project, National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
RISE Project, National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
RISE Project, National Astronomical Observatory of Japan | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | ||||||
著者所属(英) | ||||||
en | ||||||
Planetary Exploration Research Center, Chiba Institute of Technology | ||||||
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 | The South Pole-Aitken basin (SPA) is the largest (2500km in diameter), deepest and presumably oldest impact basin in the solar system. SPA was characterized by an ellipse with axes 2400 by 2050 km, but more precise topography and gravity data are necessary to discuss the structure of SPA on the lunar farside. We use topography and gravity data obtained by KAGUYA(SELENE). The direction of an ellipse denoting the depression is similar to the previous result. The region with the thinnest crust is offset southward from the center of SPA. We analyzed interior structure of small basins in and around SPA. We interpret that a positive gravity anomaly corresponds to a Moho uplift. A distinct Moho uplift beneath Schrodinger corresponds to the presence of olivine at the central peak rings. | |||||
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: AA0065390010 |