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短周期彗星:原始物体还是碰撞碎片?

Farinella1, Davis

  • 1P. Farinella, Dipartimento di Matematica, Universita di Pisa, Via Buonarroti 2, 56127 Pisa, Italy. D. R. Davis, Planetary Science Institute, 620 North Sixth Avenue, Tucson, AZ 85705-8331, USA.

Science (New York, N.Y.)
|August 16, 1996
PubMed
概括

在Edgeworth-Kuiper带物体 (EKO) 之间的碰撞塑造了它们的群体,并产生了短周期彗星. 较小的EKO经常分解,影响彗星的形状和颜色等属性.

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