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TOI-6508 b: A massive transiting brown dwarf orbiting a low-mass star

  • K. Barkaoui
  • , D. Sebastian
  • , S. Zúñiga-Fernández
  • , A. H.M.J. Triaud
  • , B. V. Rackham
  • , A. J. Burgasser
  • , T. W. Carmichael
  • , M. Gillon
  • , C. Theissen
  • , E. Softich
  • , B. Rojas-Ayala
  • , G. Srdoc
  • , A. Soubkiou
  • , A. Fukui
  • , M. Timmermans
  • , M. Stalport
  • , A. Burdanov
  • , D. R. Ciardi
  • , K. A. Collins
  • , Y. T. Davis
  • F. Davoudi, J. De Wit, B. O. Demory, S. Deveny, G. Dransfield, E. Ducrot, L. Florian, T. Gan, Y. Gómez Maqueo Chew, M. J. Hooton, S. B. Howell, J. M. Jenkins, C. Littlefield, E. L. Martín, F. Murgas, P. Niraula, E. Palle, P. P. Pedersen, F. J. Pozuelos, D. Queloz, G. Ricker, R. P. Schwarz, S. Seager, A. Shporer, M. G. Scott, C. Stockdale, J. Winn
  • University of Liege
  • Massachusetts Institute of Technology
  • Instituto de Astrofísica de Canarias
  • University of Birmingham
  • University of California at San Diego
  • University of Hawai'i at Mānoa
  • Kotizarovci Observatory
  • Cadi Ayyad University
  • The University of Tokyo
  • California Institute of Technology
  • Harvard-Smithsonian Center for Astrophysics
  • University of Bern
  • Bay Area Environmental Research Institute
  • NASA Ames Research Center
  • Paris Region Fellow
  • Université Paris-Saclay
  • Swiss Federal Institute of Technology Zurich
  • University of Montreal
  • Tsinghua University
  • Universidad Nacional Autónoma de México
  • University of Cambridge
  • University of La Laguna
  • Glorieta de la Astronomía S/n
  • Hazelwood Observatory
  • Princeton University

Research output: Contribution to journal › Article › peer-review

13 Scopus citations

Abstract

We report the discovery of a transiting brown dwarf orbiting a low-mass star, TOI-6508 b. Today, only ∼50 transiting brown dwarfs have been discovered. TOI-6508 b was first detected with data from the Transiting Exoplanet Survey Satellite (TESS) in Sectors 10, 37 and 63. Ground-based follow-up photometric data were collected with the SPECULOOS-South (Search for habitable Planets EClipsing ULtra-cOOl Stars) and LCOGT-1m telescopes, and RV measurements were obtained with the Near InfraRed Planet Searcher (NIRPS) spectrograph. We find that TOI-6508 b has a mass of Mp = 72.5-5.1+7.6 MJup and a radius of Rp = 1.03 ± 0.03 RJup. Our modeling shows that the data are consistent with an eccentric orbit of 19 day and an eccentricity of e = 0.28-0.08+0.09. TOI-6508 b has a mass ratio of MBD/M∗ = 0.40, makes it the second highest mass ratio brown dwarf that transits a low-mass star. The host has a mass of M∗ = 0.174 ± 0.004 M⊙, a radius of R∗ = 0.205 ± 0.006 R⊙, an effective temperature of Teff = 2930 ± 70 K, and a metallicity of [Fe/H] =-0.22 ± 0.08. This makes TOI-6508 b an interesting discovery that has come to light in a region still sparsely populated.

Original languageEnglish
Article numberA44
JournalAstronomy and Astrophysics
Volume696
DOIs
StatePublished - 1 Apr 2025

Keywords

  • Brown dwarfs
  • Stars: individual: TOI-6508

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