TESS Giants Transiting Giants. I: A Noninflated Hot Jupiter Orbiting a Massive Subgiant
Name
Saunders_2022_AJ_163_53.pdf
Description
Published version
Size
6.77 MB
Format
Adobe PDF
Checksum (MD5)
7dd753a60bb0cdf55243295da815b69d
Author(s)
Seager, Sara
Date Issued
2022
Journal
Astronomical Journal
Publisher
American Astronomical Society
Citation
Seager, Sara. 2022. "TESS Giants Transiting Giants. I: A Noninflated Hot Jupiter Orbiting a Massive Subgiant." Astronomical Journal, 163 (2).
Version
Final published version
Abstract
While the population of confirmed exoplanets continues to grow, the sample of confirmed transiting planets around evolved stars is still limited. We present the discovery and confirmation of a hot Jupiter orbiting TOI-2184 (TIC 176956893), a massive evolved subgiant (M⋆ = 1.53 ± 0.12 M⊙, R⋆ = 2.90 ± 0.14 R⊙) in the Transiting Exoplanet Survey Satellite (TESS) Southern Continuous Viewing Zone. The planet was flagged as a false positive by the TESS Quick-Look Pipeline due to periodic systematics introducing a spurious depth difference between even and odd transits. Using a new pipeline to remove background scattered light in TESS Full Frame Image data, we combine space-based TESS photometry, ground-based photometry, and ground-based radial velocity measurements to report a planet radius of Rp = 1.017 ± 0.051 RJ and mass of Mp = 0.65 ± 0.16 MJ. For a planet so close to its star, the mass and radius of TOI-2184b are unusually well matched to those of Jupiter. We find that the radius of TOI-2184b is smaller than theoretically predicted based on its mass and incident flux, providing a valuable new constraint on the timescale of post-main-sequence planet inflation. The discovery of TOI-2184b demonstrates the feasibility of detecting planets around faint (TESS magnitude > 12) post-main-sequence stars and suggests that many more similar systems are waiting to be detected in the TESS FFIs, whose confirmation may elucidate the final stages of planetary system evolution.
MIT Department
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Terms of Use
Creative Commons Attribution 4.0 International license
Persistent DSpace Link
DOI of Published Version
https://doi.org/10.3847/1538-3881/AC38A1
