Extremely Tenuous, Dusty Terrestrial Atmospheres Remain Stable against Global Collapse: An Argument for Arid Planet Habitability in the Trappist-1 System

The potential habitability of tidally locked planets orbiting M stars remains uncertain. However, recent observations with JWST and numerous theoretical studies investigating atmospheric evolution over time suggest that thick atmospheres (>1 bar) with abundant surface water are increasingly unlikely...

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Detalles Bibliográficos

Autores principales:	Victoria L. Hartwick, Melinda A. Kahre, Robert M. Haberle
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2025-01-01
Colección:	The Astrophysical Journal
Materias:	Exoplanet atmospheres Exoplanet atmospheric dynamics Habitable planets Habitable zone Planetary climates
Acceso en línea:	https://doi.org/10.3847/1538-4357/adf42f
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