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Updated: May 13, 2026

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主環の粘着性の広がりによる土星の月子の最近の形成

Sébastien Charnoz1, Julien Salmon, Aurélien Crida

  • 1Laboratoire AIM, Université Paris Diderot/CEA/CNRS, 91191 Gif sur Yvette, France. charnoz@cea.fr

Nature
|June 11, 2010
PubMed
まとめ

予想より若い土星の小さな衛星は,おそらくそのリングから形成された. シミュレーションでは,ロシュの限界を超えて広がる粘性指輪がこれらの衛星を作り,主環とF環を形作っていることが示されています.

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