학술논문
Sulfur dioxide in the mid-infrared transmission spectrum of WASP-39b.
Document Type
article
Author
Taylor, Jake; Kirk, James; Bell, Taylor; Barstow, Joanna; Gao, Peter; Bean, Jacob; Blecic, Jasmina; Chubb, Katy; Crossfield, Ian; Jordan, Sean; Kitzmann, Daniel; Moran, Sarah; Morello, Giuseppe; Moses, Julianne; Welbanks, Luis; Yang, Jeehyun; Zhang, Xi; Ahrer, Eva-Maria; Bello-Arufe, Aaron; Brande, Jonathan; Casewell, S; Crouzet, Nicolas; Cubillos, Patricio; Demory, Brice-Olivier; Dyrek, Achrène; Flagg, Laura; Hu, Renyu; Inglis, Julie; Jones, Kathryn; Kreidberg, Laura; López-Morales, Mercedes; Lagage, Pierre-Olivier; Meier Valdés, Erik; Miguel, Yamila; Parmentier, Vivien; Piette, Anjali; Rackham, Benjamin; Radica, Michael; Redfield, Seth; Stevenson, Kevin; Wakeford, Hannah; Aggarwal, Keshav; Alam, Munazza; Batalha, Natalie; Batalha, Natasha; Benneke, Björn; Berta-Thompson, Zach; Brady, Ryan; Caceres, Claudio; Carter, Aarynn; Désert, Jean-Michel; Harrington, Joseph; Iro, Nicolas; Line, Michael; Lothringer, Joshua; MacDonald, Ryan; Mancini, Luigi; Molaverdikhani, Karan; Mukherjee, Sagnick; Nixon, Matthew; Oza, Apurva; Palle, Enric; Rustamkulov, Zafar; Sing, David; Steinrueck, Maria; Venot, Olivia; Wheatley, Peter; Yurchenko, Sergei; Powell, Diana; Feinstein, Adina; Lee, Elspeth; Zhang, Michael; Tsai, Shang-Min
Source
Nature. 626(8001)
Subject
Language
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 (