Nondestructive characterization of Antarctic micrometeorites collected at the Dome Fuji Station by synchrotron radiation X-ray fluorescence analysis
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The bulk trace element composition (Ca, Ti, Cr, Mn, Ni Cu, Zn, Ge, Se, Rb, Sr, Y, Zr, Mo) of eighty-three Antarctic micrometeorites was nondestructively analyzed using synchrotron radiation X-ray fluorescence analysis (SR-XRF), and these elements were characterized in terms of their abundance ratio relative to Murchison matrix composition. The relationship between heating history and chemical composition is also examined. We found a complementary relationship among I-type, S-type and unmelted AMMs in the micrometeorites' elemental abundance, which is consistent with the hypothesis that I-type and S-type spherules were separated from chondritic meteoroids.
収録刊行物
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- Antarctic meteorite research
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Antarctic meteorite research 13 302-310, 2000-03
National Institute of Polar Research
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詳細情報 詳細情報について
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- CRID
- 1390572174722262016
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- NII論文ID
- 120005506925
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- NII書誌ID
- AA11182426
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- Web Site
- http://id.nii.ac.jp/1291/00005984/
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- IRDB
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