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

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 M p = 72.5 −5.1 +7.6 M Jup and a radius of R p = 1.03 ± 0.03 R Jup . 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 M BD / 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 T eff = 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.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2025-03-17
DOI
https://doi.org/10.1051/0004-6361/202453508
Citations
8
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
9.24

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article

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

E. Palle, Benjamin V. Rackham, B. -O. Demory, A. Shporer et al.
8 citations
Astronomy and Astrophysics
Stellar, planetary, and galactic studies
9.24
article

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

E. Palle, Benjamin V. Rackham, B. -O. Demory, A. Shporer, C. Stockdale, F. Murgas, D.R. Ciardi, E. L. Martín, M. Gillon, A. Burdanov, Daniel Sebastian, F. J. Pozuelos, K.A. Collins, T.W. Carmichael, K. Barkaoui, D. Queloz, J.M. Jenkins, J. de Wit, Adam J. Burgasser, S. Seager, Sebastián Zúñiga-Fernández, G. Ricker, Yasmin Davis, A. H. M. J. Triaud, Y. Gómez Maqueo Chew, S. B. Howell, M. J. Hooton, Fatemeh Davoudi, R.P. Schwarz, Colin Littlefield, Prajwal Niraula, Christopher A. Theissen, G. Srdoc, M. Timmermans, B. Rojas-Ayala, Tianjun Gan, A. Soubkiou, Emma Softich, G. Dransfield, Elsa Ducrot, A. Fukui, M. Stalport, Sarah J. Deveny, P.P. Pedersen, Joshua N. Winn, M. G. Scott, L. Florian
article en
8 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 M p = 72.5 −5.1 +7.6 M Jup and a radius of R p = 1.03 ± 0.03 R Jup . 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 M BD / 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 T eff = 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.

Astronomy and AstrophysicsVol. 696
University of Bern (CH), Cadi Ayyad University (MA), California Institute of Technology (US), Ames Research Center (US), Centre National de la Recherche Scientifique (FR), Planetary Science Institute (US), University of Hawaii System (US), University of Liège (BE), Universidad de La Laguna (ES), Universidad Autónoma de la Ciudad de México (MX), University of Tarapacá (CL), Princeton University (US), Université Paris Cité (FR), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris-Saclay (FR), NASA Exoplanet Science Institute (US), ETH Zurich (CH), University of California San Diego (US), Astrophysique, Instrumentation et Modélisation (FR), Cavendish Hospital (GB), Bay Area Environmental Research Institute (US), Center for Astrophysics Harvard & Smithsonian (US), CEA Paris-Saclay (FR), Instituto de Astrofísica de Canarias (ES), Tokyo Metropolitan Komaba High School (JP), Instituto de Astrofísica de Andalucía (ES), Ellinbank Observatory (AU), American Institute of Aeronautics and Astronautics (US), Massachusetts Institute of Technology (US), Université de Montréal (CA), The University of Tokyo (JP), University of Birmingham (GB), Universidad Nacional Autónoma de México (MX), Tsinghua University (CN)
National Science Foundation, National Aeronautics and Space Administration, California Institute of Technology, Space Telescope Science Institute, European Commission, Fonds De La Recherche Scientifique - FNRS, Fédération Wallonie-Bruxelles, Ministry of Science, ICT and Future Planning, Nuclear Safety and Security Commission, Korea Astronomy and Space Science Institute, European Southern Observatory, Ministerio de Ciencia e Innovación, Ministério da Ciência, Tecnologia, Inovações e Comunicações, Agencia Nacional de Investigación y Desarrollo, Ames Research Center, Science Mission Directorate, Science and Technology Facilities Council, Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture, Agencia Estatal de Investigación
Openalex Percentile: Top 2%
Stellar, planetary, and galactic studies
9.24
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