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Climate Bistability at the Inner Edge of the Habitable Zone due to Runaway Greenhouse and Cloud Feedbacks

Understanding the climate dynamics at the inner edge of the habitable zone is crucial for predicting the habitability of rocky exoplanets. Previous studies using global climate models (GCMs) have indicated that planets receiving high stellar flux can exhibit climate bifurcations, leading to bistabil...

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Main Authors: Bowen Fan, Da Yang, Dorian S. Abbot
Format: Artigo
Language:Inglês
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
Subjects:
Exoplanets
Exoplanet atmospheres
Extrasolar rocky planets
Habitable planets
Atmospheric science
Planetary atmospheres
Online Access:https://doi.org/10.3847/2041-8213/ad7789
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