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Surface Dynamics on Small Bodies: Electrostatic versus Gravitational Fields
https://jaxa.repo.nii.ac.jp/records/7359
https://jaxa.repo.nii.ac.jp/records/7359ca4b93ca-bc01-4f9e-a829-2eee1c534b14
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 | Surface Dynamics on Small Bodies: Electrostatic versus Gravitational Fields | |||||
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 |
矢野, 創
× 矢野, 創× Bellerose, Julie× Yano, Hajime |
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著者所属 | ||||||
宇宙航空研究開発機構月・惑星探査プログラムグループ | ||||||
著者所属 | ||||||
宇宙航空研究開発機構月・惑星探査プログラムグループ : 宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属(英) | ||||||
en | ||||||
JAXA Space Exploration Center, Japan Aerospace Exploration Agency (JAXA)(JSPEC) | ||||||
著者所属(英) | ||||||
en | ||||||
JAXA Space Exploration Center, Japan Aerospace Exploration Agency (JAXA)(JSPEC) : Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | ||||||
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 |
アストロダイナミクスシンポジウム講演後刷り集 en : Proceedings of 19th workshop on JAXA Astrodynamics and Flight Mechanics 巻 2009, p. 334-337, 発行日 2010-03 |
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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 | アストロダイナミクスシンポジウム (2009年7月30-31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 | Workshop on JAXA Astrodynamics and Flight Mechanics, 2009 (July 30-31, 2009. Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA)), Sagamihara, Kanagawa Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | There has been evidence of dust levitation in space, first on the Moon. At asteroid Eros, dust craters, or ponds, have been observed by the Near Earth Asteroid Rendezvous mission (NEAR) in 2001, suggesting the presence of electrostatic forces able to alter the regolith distribution. Since then, work has been done to simulate and partially reproduce the phenomena observed. More recently, observations from the Hayabusa spacecraft validate predictions on particle sizes due to solar interaction. In future missions to these bodies, we hope for additional close approaches, touchdowns and mobile landers. Thus local gravity and dust properties become a greater concern for the success of the mission. As an asteroid rotates, it induces charging cycles from photoemission of electrons and collection of solar wind electrons and ions. Hence, the local surface of the small body goes from positive to strongly negative potential. However, to date, there is still little known about the coupling between electrostatic force and the low gravitational attraction on small bodies. In this paper, we revisit the modeling and theory of dust levitation for Near Earth Asteroids, and we give a measure of relative importance of the electrostatic and the gravitational fields. | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11567475 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064734054 |