The Astronomical Journal (Jan 2023)

TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf

  • Shubham Kanodia,
  • Suvrath Mahadevan,
  • Jessica Libby-Roberts,
  • Gudmundur Stefansson,
  • Caleb I. Cañas,
  • Anjali A. A. Piette,
  • Alan Boss,
  • Johanna Teske,
  • John Chambers,
  • Greg Zeimann,
  • Andrew Monson,
  • Paul Robertson,
  • Joe P. Ninan,
  • Andrea S. J. Lin,
  • Chad F. Bender,
  • William D. Cochran,
  • Scott A. Diddams,
  • Arvind F. Gupta,
  • Samuel Halverson,
  • Suzanne Hawley,
  • Henry A. Kobulnicky,
  • Andrew J. Metcalf,
  • Brock A. Parker,
  • Luke Powers,
  • Lawrence W. Ramsey,
  • Arpita Roy,
  • Christian Schwab,
  • Tera N. Swaby,
  • Ryan C. Terrien,
  • John Wisniewski

DOI
https://doi.org/10.3847/1538-3881/acabce
Journal volume & issue
Vol. 165, no. 3
p. 120

Abstract

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We present the discovery of TOI-5205b, a transiting Jovian planet orbiting a solar metallicity M4V star, which was discovered using Transiting Exoplanet Survey Satellite photometry and then confirmed using a combination of precise radial velocities, ground-based photometry, spectra, and speckle imaging. TOI-5205b has one of the highest mass ratios for M-dwarf planets, with a mass ratio of almost 0.3%, as it orbits a host star that is just 0.392 ± 0.015 M _⊙ . Its planetary radius is 1.03 ± 0.03 R _J , while the mass is 1.08 ± 0.06 M _J . Additionally, the large size of the planet orbiting a small star results in a transit depth of ∼7%, making it one of the deepest transits of a confirmed exoplanet orbiting a main-sequence star. The large transit depth makes TOI-5205b a compelling target to probe its atmospheric properties, as a means of tracing the potential formation pathways. While there have been radial-velocity-only discoveries of giant planets around mid-M dwarfs, this is the first transiting Jupiter with a mass measurement discovered around such a low-mass host star. The high mass of TOI-5205b stretches conventional theories of planet formation and disk scaling relations that cannot easily recreate the conditions required to form such planets.

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