Identification of carbon dioxide in an exoplanet atmosphere

Identification
DOI: 10.1038/s41586-022-05269-w Publication Date: 2022-09-02T10:05:52Z
AUTHORS (132)
ABSTRACT
Abstract Carbon dioxide (CO 2 ) is a key chemical species that found in wide range of planetary atmospheres. In the context exoplanets, CO an indicator metal enrichment (that is, elements heavier than helium, also called ‘metallicity’) 1–3 , and thus formation processes primary atmospheres hot gas giants 4–6 . It one most promising to detect secondary terrestrial exoplanets 7–9 Previous photometric measurements transiting planets with Spitzer Space Telescope have given hints presence but not yielded definitive detections owing lack unambiguous spectroscopic identification 10–12 Here we present detection atmosphere giant exoplanet WASP-39b from transmission spectroscopy observations obtained JWST as part Early Release Science programme 13,14 The data used this study span 3.0–5.5 micrometres wavelength show prominent absorption feature at 4.3 (26-sigma significance). overall spectrum well matched by one-dimensional, ten-times solar metallicity models assume radiative–convective–thermochemical equilibrium moderate cloud opacity. These predict should water, carbon monoxide hydrogen sulfide addition little methane. Furthermore, tentatively small near 4.0 reproduced these models.
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