隕石鉱物 Meteorite Minerals

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抄録

Meteorites are the most important sample to shed light on the origin of the solar system and planets. In these twenty years, the total number of meteoritic minerals has increased so much, up to about 200. The characteristic features of these minerals reflect on the formation conditions of meteorites. Especially, some minerals indicate the physical conditions at the formation of meteorites. Trace elements and isotopic compositions of meteoritic minerals have been also analyzed. From these data, the processes in the early solar system are reconstructed, such as condensation in the solar nebula, accretion, metamorphism, aqueous alteration, impact process and magmatism in the parent bodies.

収録刊行物

  • 鉱物学雜誌 = Journal of the Mineralogical Society of Japan

    鉱物学雜誌 = Journal of the Mineralogical Society of Japan 25(2), 49-60, 1996-04-01

    Japan Association of Mineralogical Sciences

参考文献:  78件中 1-78件 を表示

被引用文献:  2件中 1-2件 を表示

各種コード

  • NII論文ID(NAID)
    10008767950
  • NII書誌ID(NCID)
    AN00084868
  • 本文言語コード
    JPN
  • 資料種別
    REV
  • ISSN
    04541146
  • NDL 記事登録ID
    4226735
  • NDL 雑誌分類
    ZM46(科学技術--地球科学--岩石・鉱物・鉱床)
  • NDL 請求記号
    Z15-117
  • データ提供元
    CJP書誌  CJP引用  NDL  J-STAGE 
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