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Nature (London), 2023-02, Vol.614 (7949), p.649-652
2023
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Autor(en) / Beteiligte
Titel
Identification of carbon dioxide in an exoplanet atmosphere
Ist Teil von
  • Nature (London), 2023-02, Vol.614 (7949), p.649-652
Ort / Verlag
England: Nature Publishing Group
Erscheinungsjahr
2023
Beschreibungen/Notizen
  • 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.
Sprache
Englisch
Identifikatoren
ISSN: 0028-0836
eISSN: 1476-4687
DOI: 10.1038/s41586-022-05269-w
Titel-ID: cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_9946830
Format
Schlagworte
Life Sciences

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