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Updated: Jun 28, 2025

Scattering And Absorption of Light in Planetary Regoliths
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太陽系の大惑星の軌道不安定をエンスタチット隕石を用いて年代測定

Chrysa Avdellidou1,2, Marco Delbo'1,2, David Nesvorný3

  • 1Laboratoire Lagrange, Centre National de la Recherche Scientifique, Observatoire de la Côte d'Azur, Université Côte d'Azur, 06304 Nice, France.

Science (New York, N.Y.)
|April 16, 2024
PubMed
まとめ

巨大惑星の軌道不安定は,太陽系形成の6000万年から1億年後に発生し,初期の惑星物質を小惑星帯に埋め込んだ. このタイミングは月形成の巨大衝突と 関連しているかもしれません

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