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Penetration of the solar wind after dissipation of the solar nebula: Origin of Venusian Ar by off-disk implantation of the solar wind
https://doi.org/10.15094/00004494
https://doi.org/10.15094/00004494c199196b-d6ae-424a-86ec-15005c7a515a
名前 / ファイル | ライセンス | アクション |
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KJ00000036300 (1.1 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1989-10-01 | |||||
タイトル | ||||||
タイトル | Penetration of the solar wind after dissipation of the solar nebula: Origin of Venusian Ar by off-disk implantation of the solar wind | |||||
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_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ID登録 | ||||||
ID登録 | 10.15094/00004494 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Sasaki, Sho
× Sasaki, Sho |
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著者所属(英) | ||||||
en | ||||||
Lunar and Planetary Laboratory, University of Arizona | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Implantation of the ancent solar wind is a possible noble gas source for Venus and gas-rich meteorites. During the stage of planetary accretion, dust grains re-emitted by planetesimal collisions could be targets of the solar wind implantation. The present study shows that such off-disk implantation can play an important role in noble gas capture; our results explain not only the ^<36>Ar amount in the Venusian atmosphere but also the fact that the ^<36>Ar abundance in Venus is 70 times as much as that in the Earth, assuming that gravitational scattering by the proto-Venus should enhance the orbital inclination of target materials. This mechanism may also have played a role in the origin of gas-rich meteorites. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA10784627 | |||||
書誌情報 |
Proceedings of the NIPR Symposium on Antarctic Meteorites 巻 2, p. 326-334, 発行日 1989-10 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |