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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Autors principals:	Yueyun Ouyang, Feng Ding, Jun Yang
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2025-01-01
Col·lecció:	The Astrophysical Journal Letters
Matèries:	Exoplanet atmospheres Extrasolar rocky planets Land-atmosphere interactions Water vapor Surface ices
Accés en línia:	https://doi.org/10.3847/2041-8213/adda4b
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