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Petrology of silicate inclusions in the Miles IIE iron
https://doi.org/10.15094/00004706
https://doi.org/10.15094/0000470673673726-7ee7-45e7-ae6a-d564446f2222
名前 / ファイル | ライセンス | アクション |
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KJ00000036512 (3.1 MB)
|
Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1996-03-01 | |||||
タイトル | ||||||
タイトル | Petrology of silicate inclusions in the Miles IIE iron | |||||
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 | 10.15094/00004706 | |||||
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) |
Ikeda,Yukio
× Ikeda,Yukio× Prinz, Martin |
|||||
著者所属(英) | ||||||
en | ||||||
Department of Earth Sciences, Ibaraki University/Department of Earth and Planetary Sciences, Amerian Museum of Natural History | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The Miles IIE iron contains many silicate inclusions with gabbroic and cryptocrystalline textures. The gabbroic inclusions consist of inverted pigeonite, orthopyroxene, high-Ca pyroxene, olivine, sodic plagioclase, antiperthite, K-feldspar, tridymite, granitic glass, chromite, rutile, armalcolite, ilmenite, whitlockite, chlorapatite, troilite, schreibersite, taenite, and kamacite. They are the crystallization products of silicate melts which were produced by equilibrium or impact partial melting of an H chondritic precursor, and the degree of melting was variable, but about 25% on the average. Partial melting probably took place in a regolithic breccia on an H chondritic parent body. The melts experienced reduction during their crystallization. The cryptocrystalline inclusions consist mainly of cryptocrystalline albite and alkali feldspar, and sometimes have phenocrystic clinopyroxene, needles of orthopyroxene, and/or whitlockite-predominant nodules. Some nodules include P-bearing magnesian olivine, sodalite, and rutile, and these nodules appear to have separated as P_2O_5-rich melts from the albite-rich melt by liquid immiscibility. The inclusions cooled rapidly, resulting in their cryptocrystalline textures. | |||||
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 9, p. 143-173, 発行日 1996-03 |
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出版者 | ||||||
出版者 | National Institute of Polar Research |