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  1. 極地研刊行誌
  2. 英文誌
  3. 南極隕石
  4. Proceedings of the NIPR Symposium on Antarctic Meteorites (ISSN 0914-5621)
  5. No.8 (Mar. 1995)

Geochemistry and origin of achondritic inclusions in Yamato-75097, -793241 and -794046 chondrites

https://doi.org/10.15094/00004681
https://doi.org/10.15094/00004681
437f449a-0d63-4f75-a336-261c609a60a4
名前 / ファイル ライセンス アクション
KJ00000036487.pdf KJ00000036487 (2.3 MB)
license.icon
Item type 紀要論文(ELS) / Departmental Bulletin Paper(1)
公開日 1995-03-01
タイトル
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 10.15094/00004681
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) Mittlefehldt,David W.

× Mittlefehldt,David W.

WEKO 8024

en Mittlefehldt,David W.

Search repository
Lindstrom,Marilyn M.

× Lindstrom,Marilyn M.

WEKO 46862

en Lindstrom,Marilyn M.

Search repository
Wang,Ming-Sheng

× Wang,Ming-Sheng

WEKO 46863

en Wang,Ming-Sheng

Search repository
Lipschutz,Michael E.

× Lipschutz,Michael E.

WEKO 46864

en Lipschutz,Michael E.

Search repository
著者所属(英)
en
C23,Lockheed Engineering and Sciences Co./SN2,Planetary Materials Branch, NASA-Johnson Space Center/Department of Chemistry, Purdue University/Department of Chemistry, Purdue University
抄録(英)
内容記述タイプ Other
内容記述 We have performed instrumental and radiochemical neutron activation analyses of the host L6 chondrite and five splits of the Yamato (Y)-75097 achondritic inclusion, and achondritic inclusions from the Y-793241 (L6) and Y-794046 (H5) chondrites. The troctolitic inclusions from Y-75097 and Y-793241 show numerous compositional similarities, including low Sc contents, fractionated siderophile element patterns at low abundances, and commonly (though not always) depleted trivalent REE abundances but with Eu at near chondritic levels. The REE, however, are highly variable in the Y-75097 inclusion due to variations in modal merrillite. The lack of pyroxene in these inclusions is best explained by assuming the protolith was non-chondritic in bulk composition. However, it is not clear that nebular processes could produce a pyroxene-poor protolith. The siderophile element patterns in these inclusions can be modeled as residual metal left after partial melting of the Fe-FeS system. The Y-794046 inclusion is compositionally and mineralogically different from the other inclusions. Abundances of refractory through moderately volatile lithophile elements are unfractionated relative to mean H chondrites. Similarly, abundances of refractory through moderately volatile siderophile elements are in H chondritic relative proportions, but at ∿10% the abundance of mean H chondrites. This cosmochemical signature is most simply modeled as a result of impact melting of an H chondrite target, with loss of ∿90% of the immiscible Fe-FeS melt.
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 8, p. 251-271, 発行日 1995-03
出版者
出版者 National Institute of Polar Research
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