JWST NIRSpec PRISM transmission spectroscopy detects CH4, other hydrocarbons, and aerosols in WD 1856 b's atmosphere, with evidence for recent reheating and a carbon-enriched composition.
N.et al.Optical constants of organic tholins produced in a simulated Titanian atmo- sphere: From soft x-ray to microwave frequen- cies.Icarus60, 127–137 (1984)
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Aerosols and hydrocarbons in the atmosphere of a white dwarf planet
JWST NIRSpec PRISM transmission spectroscopy detects CH4, other hydrocarbons, and aerosols in WD 1856 b's atmosphere, with evidence for recent reheating and a carbon-enriched composition.