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Updated: Dec 16, 2025

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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熱いネプチューンの砂漠の残った惑星の核

David J Armstrong1,2, Théo A Lopez3, Vardan Adibekyan4

  • 1Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK. d.j.armstrong@warwick.ac.uk.

Nature
|July 3, 2020
PubMed
まとめ

TOI-849bは,海王星より小さい密度の高い系外惑星で,ガスの巨星の残った核である可能性が高い. 惑星の進化の洞察を提示する 大気の大量の損失を示唆しています

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