Planet Hunters TESS I: TOI 813, a subgiant hosting a transiting Saturn-sized planet on an 84-day orbit
Nora L. Eisner, Oscar Barragán, S. Aigrain, Chris Lintott, G. E. Miller, N. Zicher, Tabetha S. Boyajian, César Briceño, Edward M. Bryant, Jessie L. Christiansen, Adina D. Feinstein, Lauren Melissa Flor Torres, M. Fridlund, D. Gandolfi, James Gilbert, Natalia Guerrero, Jon M. Jenkins, K. Jones, Martti H. Kristiansen, Andrew Vanderburg, Nicholas M. Law, Á. R. López-Sánchez, Andrew W. Mann, Emily Safron, Megan E. Schwamb, Keivan G. Stassun, H. P. Osborn, J. Wang, Andrew Zic, Carl Ziegler, F Barnet, S J Bean, D M Bundy, Z. Chetnik, J L Dawson, J. Garstone, Andrés Stenner, Marc Huten, S. Larish, L D Melanson, Terence N. Mitchell, C. J. Moore, K Peltsch, David J. Rogers, C. Schuster, D. Steve Smith, Dean Joseph Simister, Christopher Tanner, Ivan A. Terentev, A. Tsymbal
Abstract
ABSTRACT We report on the discovery and validation of TOI 813 b (TIC 55525572 b), a transiting exoplanet identified by citizen scientists in data from NASA’s Transiting Exoplanet Survey Satellite (TESS) and the first planet discovered by the Planet Hunters TESS project. The host star is a bright (V = 10.3 mag) subgiant ($R_\star =1.94\, R_\odot$, $M_\star =1.32\, M_\odot$). It was observed almost continuously by TESS during its first year of operations, during which time four individual transit events were detected. The candidate passed all the standard light curve-based vetting checks, and ground-based follow-up spectroscopy and speckle imaging enabled us to place an upper limit of $2\, M_{\rm Jup}$ (99 per cent confidence) on the mass of the companion, and to statistically validate its planetary nature. Detailed modelling of the transits yields a period of $83.8911 _{ - 0.0031 } ^ { + 0.0027 }$ d, a planet radius of 6.71 ± 0.38 R⊕ and a semimajor axis of $0.423 _{ - 0.037 } ^ { + 0.031 }$ AU. The planet’s orbital period combined with the evolved nature of the host star places this object in a relatively underexplored region of parameter space. We estimate that TOI 813 b induces a reflex motion in its host star with a semi-amplitude of ∼6 m s−1, making this a promising system to measure the mass of a relatively long-period transiting planet.