JWST MIRI/LRS data combined with archival observations detect magnesium silicate clouds (likely Mg2SiO4) in HD 209458b at 1-10 mbar with ~0.1 micron particles using a new rule-based data reduction approach.
The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 Micron Spectrum of the Planetary-Mass Companion VHS 1256-1257 b
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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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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.