The Astrophysical Journal Letters (Jan 2023)

TOI-3235 b: A Transiting Giant Planet around an M4 Dwarf Star

  • Melissa J. Hobson,
  • Andrés Jordán,
  • E. M. Bryant,
  • R. Brahm,
  • D. Bayliss,
  • J. D. Hartman,
  • G. Á. Bakos,
  • Th. Henning,
  • Jose Manuel Almenara,
  • Khalid Barkaoui,
  • Zouhair Benkhaldoun,
  • Xavier Bonfils,
  • François Bouchy,
  • David Charbonneau,
  • Marion Cointepas,
  • Karen A. Collins,
  • Jason D. Eastman,
  • Mourad Ghachoui,
  • Michaël Gillon,
  • Robert F. Goeke,
  • Keith Horne,
  • Jonathan M. Irwin,
  • Emmanuel Jehin,
  • Jon M. Jenkins,
  • David W. Latham,
  • Dan Moldovan,
  • Felipe Murgas,
  • Francisco J. Pozuelos,
  • George R. Ricker,
  • Richard P. Schwarz,
  • S. Seager,
  • Gregor Srdoc,
  • Stephanie Striegel,
  • Mathilde Timmermans,
  • Andrew Vanderburg,
  • Roland Vanderspek,
  • Joshua N. Winn

DOI
https://doi.org/10.3847/2041-8213/acbd9a
Journal volume & issue
Vol. 946, no. 1
p. L4

Abstract

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We present the discovery of TOI-3235 b, a short-period Jupiter orbiting an M dwarf with a stellar mass close to the critical mass at which stars transition from partially to fully convective. TOI-3235 b was first identified as a candidate from TESS photometry and confirmed with radial velocities from ESPRESSO and ground-based photometry from HATSouth, MEarth-South, TRAPPIST-South, LCOGT, and ExTrA. We find that the planet has a mass of 0.665 ± 0.025 M _J and a radius of 1.017 ± 0.044 R _J . It orbits close to its host star, with an orbital period of 2.5926 days but has an equilibrium temperature of ≈ 604 K, well below the expected threshold for radius inflation of hot Jupiters. The host star has a mass of 0.3939 ± 0.0030 M _☉ , a radius of 0.3697 ± 0.0018 R _☉ , an effective temperature of 3389 K, and a J -band magnitude of 11.706 ± 0.025. Current planet formation models do not predict the existence of gas giants such as TOI-3235 b around such low-mass stars. With a high transmission spectroscopy metric, TOI-3235 b is one of the best-suited giants orbiting M dwarfs for atmospheric characterization.

Keywords