Sie befinden Sich nicht im Netzwerk der Universität Paderborn. Der Zugriff auf elektronische Ressourcen ist gegebenenfalls nur via VPN oder Shibboleth (DFN-AAI) möglich. mehr Informationen...
Carbon dioxide (CO
) is a key chemical species that is found in a wide range of planetary atmospheres. In the context of exoplanets, CO
is an indicator of the metal enrichment (that is, elements heavier than helium, also called 'metallicity')
, and thus the formation processes of the primary atmospheres of hot gas giants
. It is also one of the most promising species to detect in the secondary atmospheres of terrestrial exoplanets
. Previous photometric measurements of transiting planets with the Spitzer Space Telescope have given hints of the presence of CO
, but have not yielded definitive detections owing to the lack of unambiguous spectroscopic identification
. Here we present the detection of CO
in the atmosphere of the gas giant exoplanet WASP-39b from transmission spectroscopy observations obtained with JWST as part of the Early Release Science programme
. The data used in this study span 3.0-5.5 micrometres in wavelength and show a prominent CO
absorption feature at 4.3 micrometres (26-sigma significance). The overall spectrum is well matched by one-dimensional, ten-times solar metallicity models that assume radiative-convective-thermochemical equilibrium and have moderate cloud opacity. These models predict that the atmosphere should have water, carbon monoxide and hydrogen sulfide in addition to CO
, but little methane. Furthermore, we also tentatively detect a small absorption feature near 4.0 micrometres that is not reproduced by these models.