Transmission spectrum of WASP-94A b reveals morning limb cooler and cloudy versus evening limb hotter with H2O features, interpreted as cloud droplets forming on morning side and evaporating on evening side.
A New Sedimentation Model for Greater Cloud Diversity in Giant Exoplanets and Brown Dwarfs
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Clouds drive over 1000 K heating at depth in sub-Neptune atmospheres, producing molten mantle interfaces for most planets in the sample and increasing abundances of O2, SiH4, and SiO by at least 36 percent.
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Cloudy mornings and clear evenings on a gas giant exoplanet
Transmission spectrum of WASP-94A b reveals morning limb cooler and cloudy versus evening limb hotter with H2O features, interpreted as cloud droplets forming on morning side and evaporating on evening side.
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Impact of Clouds on the Atmosphere-Mantle Interface of Sub-Neptunes
Clouds drive over 1000 K heating at depth in sub-Neptune atmospheres, producing molten mantle interfaces for most planets in the sample and increasing abundances of O2, SiH4, and SiO by at least 36 percent.