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Formulation of planetary migration
https://jaxa.repo.nii.ac.jp/records/20502
https://jaxa.repo.nii.ac.jp/records/205027f0d2018-d117-4516-abdb-95bace779e14
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Formulation of planetary migration | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 惑星進化 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 惑星移動 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽系 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 太陽系進化 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 海王星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 角運動量 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 原始惑星 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 原始惑星系円盤 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 運動量輸送 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 惑星重力 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | planetary evolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | planetary migration | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | solar system | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | solar system evolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | Neptune | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | angular momentum | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | protoplanet | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | protoplanetary disk | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | momentum transfer | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | planetary gravitation | |||||
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 |
高橋, 啓介
× 高橋, 啓介× 小林, 浩× 渡邊, 誠一郎× Takahashi, Keisuke× Kobayashi, Hiroshi× Watanabe, Seiichiro |
|||||
著者所属 | ||||||
名古屋大学 大学院環境学研究科 | ||||||
著者所属 | ||||||
名古屋大学 大学院環境学研究科 | ||||||
著者所属 | ||||||
名古屋大学 大学院環境学研究科 | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya University Graduate School of Environmental Studies | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya University Graduate School of Environmental Studies | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya University Graduate School of Environmental Studies | ||||||
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39回月・惑星シンポジウム en : Proceedings of the 39th ISAS Lunar and Planetary Symposium p. 154-157, 発行日 2006-08-07 |
|||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Solar system has experienced planetary migration in its formation stage. Especially, Neptune has an evidence of outward migration in the 3:2 mean motion resonance in the Kuiper belt objects. In the point of view of planetary formation theory, outer ice giant planet needs planetary migration to shortening its growth time. Several simulations about planetary migration has done, and some results indicate that planet can migrate outward when disk has enough mass, but there are few works to understand the basic mechanism. In our work, we would like to focus attention on the mass flux that step over the planet to formulate the planetary migration. That kind of mass flux works as a fuel of migration. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0063505040 |