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惑星間塵の粒子の分子雲物質の識別

S Messenger1

  • 1McDonnell Center for the Space Sciences, Physics Department, Washington University, St. Louis, Missouri 63130-4899, USA. dbunny@howdy.wustl.edu

Nature
|May 9, 2000
PubMed
まとめ

脆弱な惑星間塵粒子のクラスター (IDP) は,他の原始的な太陽系物質よりも大きく,より一般的な水素と窒素の同位体異常を示しています. これらの発見は,恒星間分子雲の材料がクラスターのIDPに保存されていることを示唆しています.

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