JWST data on NGTS-10A b shows nightside CH4 depletion caused by day-to-night horizontal transport rather than vertical mixing or non-solar abundances.
(2019); Basilicata et al
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.EP 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
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.
Deep hydrocarbon chemistry and quenching in sub-Neptunes create PAH abundances peaking at 600 K, providing a first-principles explanation for the muted transmission spectra trend between 500-800 K.
citing papers explorer
-
Horizontal transport as a source of disequilibrium chemistry on the nightside of a hot exoplanet
JWST data on NGTS-10A b shows nightside CH4 depletion caused by day-to-night horizontal transport rather than vertical mixing or non-solar abundances.
-
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.
-
Sub-Neptunes as Soot Factories: Deep Atmosphere Hydrocarbon Formation and Quenching as the Origin of Sub-Neptune Aerosol Trends
Deep hydrocarbon chemistry and quenching in sub-Neptunes create PAH abundances peaking at 600 K, providing a first-principles explanation for the muted transmission spectra trend between 500-800 K.