81P/2

J Kissel1, F R Krueger, J Silén

  • 1Max-Planck-Institut fur Aeronomie, Max-Planck-Strasse 2, D-37191 Katlenburg-Lindau, Germany.

Science (New York, N.Y.)
|June 19, 2004
PubMed
まとめ

彗星と恒星間塵の分析は,キノンの誘導体を含む有機物質を明らかにしています. 彗星の塵は水素と酸素を失い,窒素が豊富になるが,星間塵はこれらの元素を保持する.

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