电邮这篇文章 Impactor Type and Model of the Origin of the Zhamanshin Astrobleme, Kazakhstan
- 作者: Gornostaeva T.A.1, Mokhov A.V.1, Kartashov P.M.1, Bogatikov O.A.1
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隶属关系:
- Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM)
- 期: 卷 26, 编号 1 (2018)
- 页面: 82-95
- 栏目: Article
- URL: https://journals.rcsi.science/0869-5911/article/view/177572
- DOI: https://doi.org/10.1134/S0869591118010046
- ID: 177572
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详细
Fragments of heterogeneous cosmonegic substance (nickelphosphide Ni3P and ZnAl2) were found using high resolution analytical electron microscopic techniques, for the first time in samples from a large meteorite crater: the Zhamanshin astrobleme in Kazakstan. Inasmuch as such fragments cannot simultaneously occur in meteorite of any one type, we suggest that the impactor of the Zhamanshin crater was of comet nature.
作者简介
T. Gornostaeva
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM)
Email: avm@igem.ru
俄罗斯联邦, Staromonetny 35, Moscow, 109017
A. Mokhov
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM)
编辑信件的主要联系方式.
Email: avm@igem.ru
俄罗斯联邦, Staromonetny 35, Moscow, 109017
P. Kartashov
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM)
Email: avm@igem.ru
俄罗斯联邦, Staromonetny 35, Moscow, 109017
O. Bogatikov
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM)
Email: avm@igem.ru
俄罗斯联邦, Staromonetny 35, Moscow, 109017
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