Sulfur dioxide in the mid-infrared transmission spectrum of WASP-39b

Diana Powell, Adina D. Feinstein, Elspeth K.H. Lee, Michael Zhang, Shang Min Tsai, Jake Taylor, James Kirk, Taylor Bell, Joanna K. Barstow, Peter Gao, Jacob L. Bean, Jasmina Blecic, Katy L. Chubb, Ian J.M. Crossfield, Sean Jordan, Daniel Kitzmann, Sarah E. Moran, Giuseppe Morello, Julianne I. Moses, Luis WelbanksJeehyun Yang, Xi Zhang, Eva Maria Ahrer, Aaron Bello-Arufe, Jonathan Brande, S. L. Casewell, Nicolas Crouzet, Patricio E. Cubillos, Brice Olivier Demory, Achrène Dyrek, Laura Flagg, Renyu Hu, Julie Inglis, Kathryn D. Jones, Laura Kreidberg, Mercedes López-Morales, Pierre Olivier Lagage, Erik A. Meier Valdés, Yamila Miguel, Vivien Parmentier, Anjali A.A. Piette, Benjamin V. Rackham, Michael Radica, Seth Redfield, Kevin B. Stevenson, Hannah R. Wakeford, Keshav Aggarwal, Munazza K. Alam, Natalie M. Batalha, Natasha E. Batalha, Björn Benneke, Zach K. Berta-Thompson, Ryan P. Brady, Claudio Caceres, Aarynn L. Carter, Jean Michel Désert, Joseph Harrington, Nicolas Iro, Michael R. Line, Joshua D. Lothringer, Ryan J. MacDonald, Luigi Mancini, Karan Molaverdikhani, Sagnick Mukherjee, Matthew C. Nixon, Apurva V. Oza, Enric Palle, Zafar Rustamkulov, David K. Sing, Maria E. Steinrueck, Olivia Venot, Peter J. Wheatley, Sergei N. Yurchenko

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

The recent inference of sulfur dioxide (SO2) in the atmosphere of the hot (approximately 1,100 K), Saturn-mass exoplanet WASP-39b from near-infrared JWST observations1–3 suggests that photochemistry is a key process in high-temperature exoplanet atmospheres4. This is because of the low (<1 ppb) abundance of SO2 under thermochemical equilibrium compared with that produced from the photochemistry of H2O and H2S (1–10 ppm)4–9. However, the SO2 inference was made from a single, small molecular feature in the transmission spectrum of WASP-39b at 4.05 μm and, therefore, the detection of other SO2 absorption bands at different wavelengths is needed to better constrain the SO2 abundance. Here we report the detection of SO2 spectral features at 7.7 and 8.5 μm in the 5–12-μm transmission spectrum of WASP-39b measured by the JWST Mid-Infrared Instrument (MIRI) Low Resolution Spectrometer (LRS)10. Our observations suggest an abundance of SO2 of 0.5–25 ppm (1σ range), consistent with previous findings4. As well as SO2, we find broad water-vapour absorption features, as well as an unexplained decrease in the transit depth at wavelengths longer than 10 μm. Fitting the spectrum with a grid of atmospheric forward models, we derive an atmospheric heavy-element content (metallicity) for WASP-39b of approximately 7.1–8.0 times solar and demonstrate that photochemistry shapes the spectra of WASP-39b across a broad wavelength range.

Original languageEnglish (US)
Pages (from-to)979-983
Number of pages5
JournalNature
Volume626
Issue number8001
DOIs
StatePublished - Feb 29 2024
Externally publishedYes

ASJC Scopus subject areas

  • General

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