The Astronomical Journal (Jan 2024)

TOI 762 A b and TIC 46432937 b: Two Giant Planets Transiting M-dwarf Stars

  • Joel D. Hartman,
  • Daniel Bayliss,
  • Rafael Brahm,
  • Edward M. Bryant,
  • Andrés Jordán,
  • Gáspár Á. Bakos,
  • Melissa J. Hobson,
  • Elyar Sedaghati,
  • Xavier Bonfils,
  • Marion Cointepas,
  • Jose Manuel Almenara,
  • Khalid Barkaoui,
  • Mathilde Timmermans,
  • George Dransfield,
  • Elsa Ducrot,
  • Sebastián Zúñiga-Fernández,
  • Matthew J. Hooton,
  • Peter Pihlmann Pedersen,
  • Francisco J. Pozuelos,
  • Amaury H. M. J. Triaud,
  • Michaël Gillon,
  • Emmanuel Jehin,
  • William C. Waalkes,
  • Zachory K. Berta-Thompson,
  • Steve B. Howell,
  • Elise Furlan,
  • George R. Ricker,
  • Roland Vanderspek,
  • Sara Seager,
  • Joshua N. Winn,
  • Jon M. Jenkins,
  • David Rapetti,
  • Karen A. Collins,
  • David Charbonneau,
  • Christopher J. Burke,
  • David R. Rodriguez

DOI
https://doi.org/10.3847/1538-3881/ad6f07
Journal volume & issue
Vol. 168, no. 5
p. 202

Abstract

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We present the discovery of TOI 762 A b and TIC 46432937 b, two giant planets transiting M-dwarf stars. Transits of both systems were first detected from observations by the NASA TESS mission, and the transiting objects are confirmed as planets through high-precision radial velocity observations carried out with Very Large Telescope/ESPRESSO. TOI 762 A b is a warm sub-Saturn with a mass of 0.251 ± 0.042 M _J , a radius of 0.744 ± 0.017 R _J , and an orbital period of 3.4717 days. It transits a mid-M-dwarf star with a mass of 0.442 ± 0.025 M _☉ and a radius of 0.4250 ± 0.0091 R _☉ . The star TOI 762 A has a resolved binary star companion, TOI 762 B, that is separated from TOI 762 A by 3.″2 (∼319 au) and has an estimated mass of 0.227 ± 0.010 M _☉ . The planet TIC 46432937 b is a warm super-Jupiter with a mass of 3.20 ± 0.11 M _J and radius of 1.188 ± 0.030 R _J . The planet’s orbital period is P = 1.4404 days, and it undergoes grazing transits of its early M-dwarf host star, which has a mass of 0.563 ± 0.029 M _☉ and a radius of 0.5299 ± 0.0091 R _☉ . TIC 46432937 b is one of the highest-mass planets found to date transiting an M-dwarf star. TIC 46432937 b is also a promising target for atmospheric observations, having the highest transmission spectroscopy metric or emission spectroscopy metric value of any known warm super-Jupiter (mass greater than 3.0 M _J , equilibrium temperature below 1000 K).

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