M N Fomenkova1, J F Kerridge, K Marti

  • 1Space Research Institute, Academy of Sciences, Moscow, Russia.

Science (New York, N.Y.)
|October 9, 1992
PubMed
まとめ

彗星P/ハレー彗星からの彗星塵の粒子は,マグネシウムや鉄に富んだ粒子を含め,異常な組成を示しています. これらの発見は,平衡の凝縮だけでなく,水性変化と二次的プロセスによる形成を示唆しています.

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