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Based on the well-established characteristic lunar and meteoritic ratios of FeO/MnO, (Cr)_2O_3/V and K/La, and the large-ion lithophile (LIL) element patterns, the Y-791197 meteorite is undoubtedly an anorthositic gabbro breccia of lunar highland origin. The similarity of chemical compositions of the Y-791197 and ALHA81005 meteorites suggests that both meteorites may have been ejected from the same lunar region. Based on the overall chemical abundances and the very low K_2O content, it is suggested that both meteorites originated from the far side of the moon. 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Chemistry of Yamato-791197 Antarctic meteorite: Evidence for its lunar highland origin
https://nipr.repo.nii.ac.jp/records/1954
https://nipr.repo.nii.ac.jp/records/1954eb29fcc8-8967-4a83-b3c9-b947634396c3
名前 / ファイル | ライセンス | アクション |
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KJ00000012508.pdf (1.2 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1986-07-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Chemistry of Yamato-791197 Antarctic meteorite: Evidence for its lunar highland origin | |||||
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 | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Fukuoka,Takaaki
× Fukuoka,Takaaki× Laul,J.C.× Smith,M.R.× Hughes,S.S.× Schmitt,R.A. |
|||||
著者所属(英) | ||||||
en | ||||||
Department of Chemistry, Faculty of Science, Gakushuin University/Chemical Technology Department, Battelle, Pacific Northwest Laboratories/Chemical Technology Department, Battelle, Pacific Northwest Laboratories/Department of Chemistry and Geology and the Radiation Center, Oregon State University/Department of Chemistry and Geology and the Radiation Center, Oregon State University | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We report chemical data for 33 major, minor and trace elements in one clast, two matrices and two bulk samples of the Yamato-791197 meteorite by instrumental neutron activation analysis (INAA). Based on the well-established characteristic lunar and meteoritic ratios of FeO/MnO, (Cr)_2O_3/V and K/La, and the large-ion lithophile (LIL) element patterns, the Y-791197 meteorite is undoubtedly an anorthositic gabbro breccia of lunar highland origin. The similarity of chemical compositions of the Y-791197 and ALHA81005 meteorites suggests that both meteorites may have been ejected from the same lunar region. Based on the overall chemical abundances and the very low K_2O content, it is suggested that both meteorites originated from the far side of the moon. The similar Ir/Ni/Au ratios of the Y-791197 and ALHA81005 meteorites suggest that they may be related to one and the same impact event. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA00733561 | |||||
書誌情報 |
Memoirs of National Institute of Polar Research. Special issue 巻 41, p. 84-95, 発行日 1986-07 |