An Eccentric Massive Jupiter Orbiting a Subgiant on a 9.5-day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images
We report the discovery of TOI-172 b from the Transiting Exoplanet Survey Satellite (TESS) mission, a massive hot Jupiter transiting a slightly evolved G star with a 9.48-day orbital period. This is the first planet to be confirmed from analysis of only the TESS full frame images, because the host s...
Similar Items
-
EVIDENCE FOR THE TIDAL DESTRUCTION OF HOT JUPITERS BY SUBGIANT STARS
by: Winn, Joshua Nathan, et al.
Published: (2014) -
TOI-1994b: A Low-mass Eccentric Brown Dwarf Transiting A Subgiant Star
by: Emma Page, et al.
Published: (2024-01-01) -
oMEGACat. IV. Constraining the Ages of Omega Centauri Subgiant Branch Stars with HST and MUSE
by: C. Clontz, et al.
Published: (2024-01-01) -
Asteroseismic Study of the Subgiant HD 82074
by: Villar, Victoria Ashley
Published: (2015) -
A Hot Saturn Orbiting an Oscillating Late Subgiant Discovered by TESS
by: Crossfield, Ian, et al.
Published: (2020)