Retention of Surface Water on Tidally Locked Rocky Planets in the Venus Zone around M Dwarfs
Terrestrial planets within the Venus zone surrounding M-dwarf stars can retain surface ice caps on the perpetual dark side if atmospheric heat transport is inefficient, as suggested by previous global climate simulations. This condition is proposed to play a role in the potential regional habitabili...
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| Hauptverfasser: | , , |
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| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
IOP Publishing
2025-01-01
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| Schriftenreihe: | The Astrophysical Journal Letters |
| Schlagworte: | |
| Online-Zugang: | https://doi.org/10.3847/2041-8213/adda4b |
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