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Updated: Apr 20, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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小型の二重小惑星の起源としての回転分解

Kevin J Walsh1, Derek C Richardson, Patrick Michel

  • 1UMR 6202 Cassiopée, University of Nice-Sophia Antipolis, CNRS, Observatoire de la Côte d'Azur, BP 4229, 06304 Nice Cedex 4, France. kwalsh@oca.eu

Nature
|July 11, 2008
PubMed
まとめ

熱的なYORP効果は,小惑星が衛星を形成する方法を説明することができます. このメカニズムは,ゴミの堆積小惑星の回転を引き起こし,近軌道二次体を形成する質量を流す.

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