Volatile chalcophile, siderophile and lithophile trace elements in lunar meteorite Yamato-82192

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type:P(論文)

Neutron activation analyses of Ag, Au, Bi, Cd, Co, Cs, Ga, In, Rb, Sb, Se, Te, Tl, U and Zn in whole-rock, melted and unmelted regolith samples of Yamato-82192 reveals a lunar highlands origin plus meteorite admixture, 2.4±0.8% Cl-equivalent for micrometeorites and ancient impact component. A small but real amount of mobile element loss occurred during the shock-melting episode that formed Y-82192. Differences in trace element and other trends indicate pronounced differences in the thermal histories of the parent regoliths of Allan Hills A81005 and Y-791197 and -82192 so that each must have been produced by a separate impact on the Moon.

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詳細情報 詳細情報について

  • CRID
    1050002212603156224
  • NII論文ID
    110000010242
  • NII書誌ID
    AA00733561
  • Web Site
    http://id.nii.ac.jp/1291/00002122/
  • 本文言語コード
    en
  • 資料種別
    departmental bulletin paper
  • データソース種別
    • IRDB
    • CiNii Articles

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