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Updated: Jul 14, 2026

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超新星が60Feを原惑星円盤に注入した後の証拠

Martin Bizzarro1, David Ulfbeck, Anne Trinquier

  • 1Geological Institute, University of Copenhagen, Øster Voldgade 10, DK-1350, Denmark. bizzarro@geol.ku.dk

Science (New York, N.Y.)
|May 26, 2007
PubMed
まとめ

初期の太陽系惑星系は,鉄-60 (60Fe) がなく形成され,その後の注入を示しています. この発見は,太陽が巨大な恒星群の中で形成され,初期の太陽系の構成と形成環境に影響を与えたことを示唆しています.

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