Stellar radiation pressure markedly accelerates aerosol settling in hot exoplanets, reducing particle size and mass concentration, which steepens optical transmission slopes and increases near-infrared molecular feature amplitudes.
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Aerosol dynamics on hot exoplanets: the role of radiation pressure
Stellar radiation pressure markedly accelerates aerosol settling in hot exoplanets, reducing particle size and mass concentration, which steepens optical transmission slopes and increases near-infrared molecular feature amplitudes.