1. TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136
- Author
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Tianjun Gan, Abderahmane Soubkiou, Sharon X Wang, Zouhair Benkhaldoun, Shude Mao, Étienne Artigau, Pascal Fouqué, Luc Arnold, Steven Giacalone, Christopher A Theissen, Christian Aganze, Adam Burgasser, Karen A Collins, Avi Shporer, Khalid Barkaoui, Mourad Ghachoui, Steve B Howell, Claire Lamman, Olivier D S Demangeon, Artem Burdanov, Charles Cadieux, Jamila Chouqar, Kevin I Collins, Neil J Cook, Laetitia Delrez, Brice-Olivier Demory, René Doyon, Georgina Dransfield, Courtney D Dressing, Elsa Ducrot, Jiahao Fan, Lionel Garcia, Holden Gill, Michaël Gillon, Crystal L Gnilka, Yilen Gómez Maqueo Chew, Maximilian N Günther, Christopher E Henze, Chelsea X Huang, Emmanuel Jehin, Eric L N Jensen, Zitao Lin, Nadine Manset, James McCormac, Catriona A Murray, Prajwal Niraula, Peter P Pedersen, Francisco J Pozuelos, Didier Queloz, Benjamin V Rackham, Arjun B Savel, Nicole Schanche, Richard P Schwarz, Daniel Sebastian, Samantha Thompson, Mathilde Timmermans, Amaury H M J Triaud, Michael Vezie, Robert D Wells, Julien de Wit, George R Ricker, Roland Vanderspek, David W Latham, Sara Seager, Joshua N Winn, Jon M Jenkins, Canada-France-Hawaii Telescope Corporation (CFHT), National Research Council of Canada (NRC)-Centre National de la Recherche Scientifique (CNRS)-University of Hawai'i [Honolulu] (UH), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), and Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
- Subjects
Earth and Planetary Astrophysics (astro-ph.EP) ,planets and satellites: detection ,530 Physics ,520 Astronomy ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,000 Computer science, knowledge & systems ,500 Science ,Astrophysics - Solar and Stellar Astrophysics ,[SDU]Sciences of the Universe [physics] ,Space and Planetary Science ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,stars: individual: TIC 336128819 - TOI-2136 ,planetary systems ,Astrophysics::Galaxy Astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) ,Astrophysics - Earth and Planetary Astrophysics ,QB - Abstract
We present the discovery of TOI-2136b, a sub-Neptune planet transiting every 7.85 days a nearby M4.5V-type star, identified through photometric measurements from the TESS mission. The host star is located $33$ pc away with a radius of $R_{\ast} = 0.34\pm0.02\ R_{\odot}$, a mass of $0.34\pm0.02\ M_{\odot}$ and an effective temperature of $\rm 3342\pm100\ K$. We estimate its stellar rotation period to be $75\pm5$ days based on archival long-term photometry. We confirm and characterize the planet based on a series of ground-based multi-wavelength photometry, high-angular-resolution imaging observations, and precise radial velocities from CFHT/SPIRou. Our joint analysis reveals that the planet has a radius of $2.19\pm0.17\ R_{\oplus}$, and a mass measurement of $6.4\pm2.4\ M_{\oplus}$. The mass and radius of TOI2136b is consistent with a broad range of compositions, from water-ice to gas-dominated worlds. TOI-2136b falls close to the radius valley for low-mass stars predicted by the thermally driven atmospheric mass loss models, making it an interesting target for future studies of its interior structure and atmospheric properties., Comment: 19 pages, 15 figures, submitted to MNRAS
- Published
- 2022
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