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

Abstract 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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Publication Details

Journal
The Astronomical Journal
Published
2024-10-10
DOI
https://doi.org/10.3847/1538-3881/ad6f07
Citations
14
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
4.64

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

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The Astronomical Journal
Stellar, planetary, and galactic studies
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article

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

Jon M. Jenkins, M. Gillon, F. J. Pozuelos, Zachory K. Berta-Thompson, Emmanuël Jehin, Rafael Brahm, Daniel Bayliss, Sebastián Zúñiga-Fernández, J. D. Hartman, X. Bonfıls, Karen A. Collins, Steve B. Howell, A. H. M. J. Triaud, Sara Seager, Marion Cointepas, Mathilde Timmermans, David Charbonneau, Elyar Sedaghati, Khalid Barkaoui, G. Ricker, P. P. Pedersen, Andrés Jordán, David Rapetti, M. J. Hooton, William C. Waalkes, Edward M. Bryant, Elise Furlan, G. Á. Bakos, Elsa Ducrot, Mélissa J. Hobson, R. Vanderspek, David R. Rodriguez, George Dransfield, Christopher J. Burke, J. M. Almenara, Joshua N. Winn
article en
14 citations

Abstract

Abstract 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).

The Astronomical JournalVol. 168(5)
National Aeronautics and Space Administration, Simons Foundation, California Institute of Technology, Space Telescope Science Institute, European Commission, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Fonds De La Recherche Scientifique - FNRS, Fédération Wallonie-Bruxelles, Nuclear Safety and Security Commission, Agencia Nacional de Investigación y Desarrollo, Ames Research Center, Science Mission Directorate, NASA Headquarters, Science and Technology Facilities Council, European Research Council, Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture, Agencia Estatal de Investigación, Astrophysics Division, Fondo Nacional de Desarrollo Científico y Tecnológico
Openalex Percentile: Top 5%
Stellar, planetary, and galactic studies
4.64
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