The Astronomical Journal (Jan 2025)

Searching for GEMS: TOI-5688 A b, a Low-density Giant Orbiting a High-metallicity Early M-dwarf

  • Varghese Reji,
  • Shubham Kanodia,
  • Joe P. Ninan,
  • Caleb I. Cañas,
  • Jessica Libby-Roberts,
  • Andrea S. J. Lin,
  • Arvind F. Gupta,
  • Tera N. Swaby,
  • Alexander Larsen,
  • Henry A. Kobulnicky,
  • Philip I. Choi,
  • Nez Evans,
  • Sage Santomenna,
  • Isabelle Winnick,
  • Larry Yu,
  • Jaime A. Alvarado-Montes,
  • Chad F. Bender,
  • Lia Marta Bernabó,
  • Cullen H. Blake,
  • William D. Cochran,
  • Scott A. Diddams,
  • Samuel Halverson,
  • Te Han,
  • Fred Hearty,
  • Sarah E. Logsdon,
  • Suvrath Mahadevan,
  • Michael W. McElwain,
  • Andrew Monson,
  • Paul Robertson,
  • Devendra K. Ojha,
  • Arpita Roy,
  • Christian Schwab,
  • Gudmundur Stefansson,
  • Jason Wright

DOI
https://doi.org/10.3847/1538-3881/ada7ea
Journal volume & issue
Vol. 169, no. 3
p. 187

Abstract

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We present the discovery of a low-density planet orbiting the high-metallicity early M-dwarf TOI-5688 A b. This planet was characterized as part of the search for transiting giant planets ( R ≳ 8 R _⊕ ) through the Searching for Giant Exoplanets around M-dwarf Stars (GEMS) survey. The planet was discovered with the Transiting Exoplanet Survey Satellite, and characterized with ground-based transits from Red Buttes Observatory, the Table Mountain Observatory of Pomona College, and radial velocity (RV) measurements with the Habitable-Zone Planet Finder on the 10 m Hobby Eberly Telescope and NEID on the WIYN 3.5 m telescope. From the joint fit of transit and RV data, we measure a planetary mass and radius of 124 ± 24 M _⊕ (0.39 ± 0.07 M _J ) and 10.4 ± 0.7 R _⊕ (0.92 ± 0.06 R _J ), respectively. The spectroscopic and photometric analysis of the host star TOI-5688 A shows that it is a metal-rich ([Fe/H] = 0.47 ± 0.16 dex) M2V star, favoring the core-accretion formation pathway as the likely formation scenario for this planet. Additionally, Gaia astrometry suggests the presence of a wide-separation binary companion, TOI-5688 B, which has a projected separation of ~5″ (1110 au) and is an M4V, making TOI-5688 A b part of the growing number of GEMS in wide-separation binary systems.

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