WEKO3
アイテム
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Petrology of the ALH-77003 chondrite (C3)
https://nipr.repo.nii.ac.jp/records/1378
https://nipr.repo.nii.ac.jp/records/1378f1f775c3-e3e6-4b13-aee8-77495063dcc0
名前 / ファイル | ライセンス | アクション |
---|---|---|
KJ00000012012.pdf (4.4 MB)
|
Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 1982-12-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Petrology of the ALH-77003 chondrite (C3) | |||||
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) |
Ikeda, Yukio
× Ikeda, Yukio |
|||||
著者所属(英) | ||||||
en | ||||||
Department of Earth Sciences, Ibaraki University | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The ALH-77003 chondrite (C3) is made up of fine-grained CAI's, amoeboid olivine inclusions, chondrules, devitrified glass fragments, mineral fragments and matrix. Their bulk chemical compositions and the constituent mineral compositions are presented in detail, and their origins are discussed. The fine-grained CAI's were formed from the materials rich in fassaitic pyroxenes by reactions with the surrounding gas at low temperatures. Amoeboid olivine inclusions are considered to have a cogenetic relationship with fine-grained CAI's and to have suffered the same reactions as the fine-grained CAI's FeO-rich chondrules (fSP type), devitrified glass fragments and matrix were formed from the solar nebula condensates at low temperatures whereas MgO-rich chondrules (mIP and mSP) types were formed from high temperature condensates. | |||||
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 25, p. 34-65, 発行日 1982-12 |