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Updated: May 3, 2026

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巨大な太陽系外惑星の大気の安定性限界

Tommi T Koskinen1, Alan D Aylward, Steve Miller

  • 1Atmospheric Physics Laboratory, Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK. tommi@apl.ucl.ac.uk

Nature
|December 8, 2007
PubMed
まとめ

惑星の大気は不安定になり,木星のような系外惑星の場合は0.16au以内で水力学的に脱出する. この大気からの脱出は,分子水素の熱解離によって引き起こされ,冷却機構を停止させます.

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