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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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Auteurs principaux: Bowen Fan, Da Yang, Dorian S. Abbot
Format: Artigo
Langue:Inglês
Publié: IOP Publishing 2024-01-01
Collection:The Astrophysical Journal Letters
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Accès en ligne:https://doi.org/10.3847/2041-8213/ad7789
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