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Origin of isotopic fractionation of terrestrial xenon
https://doi.org/10.15094/00004465
https://doi.org/10.15094/00004465fdf2c869-f8e4-41b2-86c4-e9d814f6439c
名前 / ファイル | ライセンス | アクション |
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KJ00000036271 (990.0 kB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1988-03-01 | |||||
タイトル | ||||||
タイトル | Origin of isotopic fractionation of terrestrial xenon | |||||
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 | 10.15094/00004465 | |||||
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) |
Igarashi,George
× Igarashi,George× Ozima,Minoru |
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著者所属(英) | ||||||
en | ||||||
Geophysical Institute, Faculty of Science, University of Tokyo/Geophysical Institute, Faculty of Science, University of Tokyo | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | By taking account of a size distribution of planetesimals, we show that noble gases gravitationally trapped by planetesimals in the solar nebula can explain the isotopic fractionation of terrestrial Xe relative to Xe in primitive meteorites, leaving Kr and other lighter noble gases almost unfractionated. However, this model is not successful in explaining noble gas elemental abundances in the Earth. | |||||
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 1, p. 315-320, 発行日 1988-03 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |