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Planet Hunters Tess I: TOI 813, a subgiant hosting a transiting Saturn-sized planet on an 84-day orbit

  • N. L. Eisner*
  • , O. Barragán
  • , S. Aigrain
  • , C. Lintott
  • , G. Miller
  • , N. Zicher
  • , T. S. Boyajian
  • , C. Briceño
  • , E. M. Bryant
  • , J. L. Christiansen
  • , A. D. Feinstein
  • , L. M. Flor-Torres
  • , M. Fridlund
  • , D. Gandolfi
  • , J. Gilbert
  • , N. Guerrero
  • , J. M. Jenkins
  • , K. Jones
  • , M. H. Kristiansen
  • , A. Vanderburg
  • N. Law, A. R. López-Sánchez, A. W. Mann, E. J. Safron, M. E. Schwamb, K. G. Stassun, H. P. Osborn, J. Wang, A. Zic, C. Ziegler, F. Barnet, S. J. Bean, D. M. Bundy, Z. Chetnik, J. L. Dawson, J. Garstone, A. G. Stenner, M. Huten, S. Larish, L. D. Melanson, T. Mitchell, C. Moore, K. Peltsch, D. J. Rogers, C. Schuster, D. S. Smith, D. J. Simister, C. Tanner, I. Terentev, A. Tsymbal
*Corresponding author for this work

    Research output: Contribution to journalReview articlepeer-review

    47 Citations (Scopus)

    Abstract

    We report on the discovery and validation of TOI 813 b (TIC55525572b), 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* = 1.94 R, M = 1.32 M). 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 MJup (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+0.0027-0.0031 d, a planet radius of 6.71 ± 0.38 R and a semimajor axis of 0.423+0031-0.037 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.

    Original languageEnglish
    Pages (from-to)750-763
    Number of pages14
    JournalMonthly Notices of the Royal Astronomical Society
    Volume494
    Issue number1
    DOIs
    Publication statusPublished - 1 May 2020

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