The Astrophysical Journal Letters (Jan 2023)

Detection of Carbon Monoxide’s 4.6 Micron Fundamental Band Structure in WASP-39b’s Atmosphere with JWST NIRSpec G395H

  • David Grant,
  • Joshua D. Lothringer,
  • Hannah R. Wakeford,
  • Munazza K. Alam,
  • Lili Alderson,
  • Jacob L. Bean,
  • Björn Benneke,
  • Jean-Michel Désert,
  • Tansu Daylan,
  • Laura Flagg,
  • Renyu Hu,
  • Julie Inglis,
  • James Kirk,
  • Laura Kreidberg,
  • Mercedes López-Morales,
  • Luigi Mancini,
  • Thomas Mikal-Evans,
  • Karan Molaverdikhani,
  • Enric Palle,
  • Benjamin V. Rackham,
  • Seth Redfield,
  • Kevin B. Stevenson,
  • Jeff A. Valenti,
  • Nicole L. Wallack,
  • Keshav Aggarwal,
  • Eva-Maria Ahrer,
  • Ian J. M. Crossfield,
  • Nicolas Crouzet,
  • Nicolas Iro,
  • Nikolay K. Nikolov,
  • Peter J. Wheatley,
  • JWST Transiting Exoplanet Community ERS team

DOI
https://doi.org/10.3847/2041-8213/acd544
Journal volume & issue
Vol. 949, no. 1
p. L15

Abstract

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Carbon monoxide (CO) is predicted to be the dominant carbon-bearing molecule in giant planet atmospheres and, along with water, is important for discerning the oxygen and therefore carbon-to-oxygen ratio of these planets. The fundamental absorption mode of CO has a broad, double-branched structure composed of many individual absorption lines from 4.3 to 5.1 μ m, which can now be spectroscopically measured with JWST. Here we present a technique for detecting the rotational sub-band structure of CO at medium resolution with the NIRSpec G395H instrument. We use a single transit observation of the hot Jupiter WASP-39b from the JWST Transiting Exoplanet Community Early Release Science (JTEC ERS) program at the native resolution of the instrument ( R ∼ 2700) to resolve the CO absorption structure. We robustly detect absorption by CO, with an increase in transit depth of 264 ± 68 ppm, in agreement with the predicted CO contribution from the best-fit model at low resolution. This detection confirms our theoretical expectations that CO is the dominant carbon-bearing molecule in WASP-39b’s atmosphere and further supports the conclusions of low C/O and supersolar metallicities presented in the JTEC ERS papers for WASP-39b.

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