HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS
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Wang_2019_AJ_157_51.pdf
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Published version
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1.79 MB
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Author(s) • • • • • • • • •
Wang, Songhu
Jones, Matias
Shporer, Avi
Fulton, Benjamin J.
Paredes, Leonardo A.
Trifonov, Trifon
Kossakowski, Diana
Eastman, Jason
Redfield, Seth
Günther, Maximilian N.
Date Issued
January 2019
Journal
Astronomical Journal
Publisher
American Astronomical Society / IOP Publishing
Citation
Wang, Songhu et al. "HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS." Astronomical Journal 157, 2 (January 2019): 51 © 2019 American Astronomical Society
Version
Final published version
Abstract
We report the first confirmation of a hot Jupiter discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HD 202772A b. The transit signal was detected in the data from TESS Sector 1, and was confirmed to be of planetary origin through radial velocity (RV) measurements. HD 202772A b is orbiting a mildly evolved star with a period of 3.3 days. With an apparent magnitude of V = 8.3, the star is among the brightest and most massive known to host a hot Jupiter. Based on the 27 days of TESS photometry and RV data from the CHIRON, HARPS, and Tillinghast Reflector Echelle Spectrograph, the planet has a mass of and radius of , making it an inflated gas giant. HD 202772A b is a rare example of a transiting hot Jupiter around a quickly evolving star. It is also one of the most strongly irradiated hot Jupiters currently known.
MIT Department
Massachusetts Institute of Technology. Department of Physics
MIT Kavli Institute for Astrophysics and Space Research
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DOI of Published Version
https://doi.org/10.3847/1538-3881/aaf1b7