The atmosphere of TOI-1130b shows high metallicity, low C/O, and elevated mean molecular weight consistent with ex-situ formation beyond the water ice line.
A warm Neptune’s methane reveals core mass and vigorous atmospheric mixing
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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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JWST unveils a high mean molecular weight atmosphere for mini-Neptune TOI-1130b: Evidence for formation beyond the water ice line
The atmosphere of TOI-1130b shows high metallicity, low C/O, and elevated mean molecular weight consistent with ex-situ formation beyond the water ice line.
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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.