planets and satellites: detection; stars: individual: TOI-2406; techniques: photometric; Astrophysics - Earth and Planetary Astrophysics
Abstract :
[en] Context. Large sub-Neptunes are uncommon around the coolest stars in the Galaxy and are rarer still around those that are metal-poor. However, owing to the large planet-to-star radius ratio, these planets are highly suitable for atmospheric study via transmission spectroscopy in the infrared, such as with JWST. Aims: Here we report the discovery and validation of a sub-Neptune orbiting the thick-disk, mid-M dwarf star TOI-2406. The star's low metallicity and the relatively large size and short period of the planet make TOI-2406 b an unusual outcome of planet formation, and its characterisation provides an important observational constraint for formation models. Methods: We first infer properties of the host star by analysing the star's near-infrared spectrum, spectral energy distribution, and Gaia parallax. We use multi-band photometry to confirm that the transit event is on-target and achromatic, and we statistically validate the TESS signal as a transiting exoplanet. We then determine physical properties of the planet through global transit modelling of the TESS and ground-based time-series data. Results: We determine the host to be a metal-poor M4 V star, located at a distance of 56 pc, with properties Teff = 3100 ± 75 K, M* = 0.162 ± 0.008M⊙, R* = 0.202 ± 0.011R⊙, and [Fe∕H] = −0.38 ± 0.07, and a member of the thick disk. The planet is a relatively large sub-Neptune for the M-dwarf planet population, with Rp = 2.94 ± 0.17R⊕ and P= 3.077 d, producing transits of 2% depth. We note the orbit has a non-zero eccentricity to 3σ, prompting questions about the dynamical history of the system. Conclusions: This system is an interesting outcome of planet formation and presents a benchmark for large-planet formation around metal-poor, low-mass stars. The system warrants further study, in particular radial velocity follow-up to determine the planet mass and constrain possible bound companions. Furthermore, TOI-2406 b is a good target for future atmospheric study through transmission spectroscopy. Although the planet's mass remains to be constrained, we estimate the S/N using amass-radius relationship, ranking the system fifth in the population of large sub-Neptunes, with TOI-2406 b having a much lower equilibrium temperature than other spectroscopically accessible members of this population.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Wells, R. D.; Center for Space and Habitability, University of Bern, Gesellschaftsstrasse 6, 3012, Bern, Switzerland
Rackham, B. V.; Department of Earth, Atmospheric and Planetary Science, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA, 02139, USA ; Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
Schanche, N.; Center for Space and Habitability, University of Bern, Gesellschaftsstrasse 6, 3012, Bern, Switzerland
Petrucci, R.; Universidad Nacional de Córdoba - Observatorio Astronómico de Córdoba, Laprida 854, X5000BGR, Córdoba, Argentina ; Consejo Nacional de Investigaciones Cientf́icas y Técnicas (CONICET), Buenos Aires, Argentina
Gómez Maqueo Chew, Y.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 70-264, CDMX, 04510, México
Demory, B.-O.; Center for Space and Habitability, University of Bern, Gesellschaftsstrasse 6, 3012, Bern, Switzerland
Burgasser, A. J.; Center for Astrophysics and Space Science, University of California San Diego, La Jolla, CA 92093, USA
Burn, R.; Max Planck Institute for Astronomy (MPIA), Koenigstuhl 17, 69117, Heidelberg, Germany
Pozuelos Romero, Francisco José ; Astrobiology Research Unit, Université de Liège, Allée du 6 Août 19C, 4000, Liège, Belgium ; Space Sciences, Technologies and Astrophysics Research (STAR) Institute, Universitďe Liège, Allée du 6 Août 19C, 4000, Liège, Belgium
Günther, M. N.; Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA ; Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
Sabin, L.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Schroffenegger, U.; Center for Space and Habitability, University of Bern, Gesellschaftsstrasse 6, 3012, Bern, Switzerland
Gómez-Muñoz, M. A.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Stassun, K. G.; Department of Physics & Astronomy, Vanderbilt University, 6301 Stevenson Center Ln., Nashville, TN 37235, USA
Van Grootel, Valérie ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Howell, S. B.; NASA Ames Research Center, Moffett Field, CA 94035, USA
Sebastian, Daniel ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Exotic
Triaud, A. H. M. J.; School of Physics & Astronomy, University of Birmingham, Edgbaston, Birmimgham, B15 2TT, UK
Apai, D.; Steward Observatory, The University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USA ; Lunar and Planetary Laboratory, The University of Arizona, 1639 E. University Boulevard, Tucson, AZ 85721, USA
Plauchu-Frayn, I.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Guerrero, C. A.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Guillén, P. F.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Landa, A.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Melgoza, G.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Montalvo, F.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Serrano, H.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Riesgo, H.; Universidad Nacional Autónoma de México, Instituto de Astronomía, AP 106, Ensenada, 22800, BC, México
Barkaoui, Khalid ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Exotic
Bixel, A.; Steward Observatory, The University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USA
Burdanov, A.; Department of Earth, Atmospheric and Planetary Science, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA, 02139, USA
Chen, W. P.; Graduate Institute of Astronomy, National Central University, 300 Jhongda Road, Zhongli, Taoyuan, 32001, Taiwan
Chinchilla, P.; Astrobiology Research Unit, Université de Liège, Allée du 6 Août 19C, 4000, Liège, Belgium ; Instituto de Astrofísica de Canarias (IAC), Calle Vía Láctea s/n, 38200, La Laguna, Tenerife, Spain
Collins, K. A.; Center for Astrophysics, Harvard & Smithsonian, 60 Garden Street, Cambridge, MA, 02138, USA
Daylan, T.; Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA ; Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
de Wit, J.; Department of Earth, Atmospheric and Planetary Science, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA, 02139, USA
Delrez, Laetitia ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Exotic
Dévora-Pajares, M.; Dpto. Física Teórica y del Cosmos, Universidad de Granada, 18071, Granada, Spain
Dietrich, Jérémy
Dransfield, G.; School of Physics & Astronomy, University of Birmingham, Edgbaston, Birmimgham, B15 2TT, UK
Ducrot, Elsa ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Exotic
Fausnaugh, M.; Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA ; Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
Furlan, E.; NASA Exoplanet Science Institute, Caltech/IPAC, Mail Code 100-22, 1200 E. California Blvd., Pasadena, CA 91125, USA
Gabor, P.; Vatican Observatory Research Group, University of Arizona, 933 N Cherry Ave., Tucson AZ, 85721-0065, USA
Gan, T.; Department of Astronomy, Tsinghua University, Beijing, 100084, PR China
Garcia, Lionel ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Exotic
Ghachoui, M.; Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, Cadi Ayyad University, Marrakech, Morocco
Giacalone, S.; Department of Astronomy, 501 Campbell Hall, University of California at Berkeley, Berkeley, CA, 94720, USA
Gibbs, A. B.; Department of Physics & Astronomy, University of California, Los Angeles, Los Angeles, CA 90095, USA
Gillon, Michaël ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Exotic
Gnilka, C.; NASA Ames Research Center, Moffett Field, CA 94035, USA
Gore, R.; Department of Astronomy, 501 Campbell Hall, University of California at Berkeley, Berkeley, CA, 94720, USA
Guerrero, N.; Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA ; Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
Henning, T.; Max Planck Institute for Astronomy (MPIA), Koenigstuhl 17, 69117, Heidelberg, Germany
Hesse, K.; Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA ; Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
Jehin, Emmanuel ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Origines Cosmologiques et Astrophysiques (OrCa)
Jenkins, J. M.; NASA Ames Research Center, Moffett Field, CA 94035, USA
Latham, D. W.; Center for Astrophysics, Harvard & Smithsonian, 60 Garden Street, Cambridge, MA, 02138, USA
Lester, K.; NASA Ames Research Center, Moffett Field, CA 94035, USA
McCormac, J.; Department of Physics, University of Warwick, Coventry, CV4 7AL, UK
Murray, C. A.; Cavendish Laboratory, JJ Thomson Avenue, Cambridge, CB3 0HE, UK
Niraula, P.; Department of Earth, Atmospheric and Planetary Science, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA, 02139, USA
Pedersen, P. P.; Cavendish Laboratory, JJ Thomson Avenue, Cambridge, CB3 0HE, UK
Ricker, G.; Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA ; Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
Rodriguez, D. R.; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD, 21218, USA
Schroeder, A.; Department of Astronomy, 501 Campbell Hall, University of California at Berkeley, Berkeley, CA, 94720, USA
Schwarz, R. P.; Patashnick Voorheesville Observatory, Voorheesville, NY 12186, USA
Scott, N.; NASA Ames Research Center, Moffett Field, CA 94035, USA
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