Issue |
A&A
Volume 683, March 2024
|
|
---|---|---|
Article Number | A166 | |
Number of page(s) | 16 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202346999 | |
Published online | 19 March 2024 |
TOI-4860 b, a short-period giant planet transiting an M3.5 dwarf
1
Univ. Grenoble Alpes, CNRS, IPAG,
38000
Grenoble, France
e-mail: jose-manuel.almenara-villa@univ-grenoble-alpes.fr
2
Observatoire de Genève, Département d’Astronomie, Université de Genève,
Chemin Pegasi 51b,
1290
Versoix, Switzerland
3
Mullard Space Science Laboratory, University College London,
Holmbury St Mary, Dorking,
Surrey
RH5 6NT, UK
4
Department of Physics, University of Warwick,
Coventry, UK
5
Facultad de Ingeniería y Ciencias, Universidad Adolfo Ibáñez,
Av. Diagonal las Torres
2640,
Peñalolén, Santiago, Chile
6
Millennium Institute for Astrophysics (MAS),
Santiago, Chile
7
Data Observatory Foundation,
Santiago, Chile
8
Institut d’astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie,
98bis boulevard Arago,
75014
Paris, France
9
Observatoire de Haute-Provence, CNRS, Université d’Aix-Marseille,
04870
Saint-Michel-l’Observatoire, France
10
Laboratório Nacional de Astrofísica,
Rua Estados Unidos 154,
37504-364,
Itajubá, MG,
Brazil
11
CFisUC, Departamento de Física, Universidade de Coimbra,
3004-516
Coimbra, Portugal
12
IMCCE, UMR8028 CNRS, Observatoire de Paris, PSL Université, Sorbonne Univ.,
77 av. Denfert-Rochereau,
75014
Paris, France
13
Departamento de Matemática y Física Aplicadas, Universidad Católica de la Santísima Concepción,
Alonso de Rivera
2850,
Concepción, Chile
14
Université de Montréal, Département de Physique & Institut Trottier de Recherche sur les Exoplanètes,
Montréal, QC
H3C 3J7, Canada
15
Canada-France-Hawaii Telescope (CFHT) Corporation,
CNRS UAR2208, 65-1238 Mamalahoa Hwy,
Kamuela, HI
96743, USA
16
Department of Astrophysical Sciences, Princeton University,
NJ
08544, USA
17
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto,
CAUP, Rua das Estrelas,
4150-762
Porto, Portugal
18
Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto,
Rua Campo Alegre,
4169-007
Porto, Portugal
19
Center for Astrophysics | Harvard & Smithsonian,
60 Garden Street,
Cambridge, MA
02138, USA
20
NASA Exoplanet Science Institute – Caltech/IPAC,
1200 E. California Blvd,
Pasadena, CA
91125, USA
21
Department of Physics & Astronomy, McMaster University,
1280 Main St W,
Hamilton, ON
L8S 4L8, Canada
22
Department of Physics, McGill University,
3600 rue University,
Montréal, Québec
H3A 2T8, Canada
23
Department of Earth and Planetary Sciences, McGill University,
3450 rue University,
Montréal, Québec
H3A 0E8, Canada
24
Univ. Federal do Rio G. do Norte, UFRN, Dep. de Física,
CP 1641,
59072-970,
Natal, RN, Brazil
25
Université de Toulouse, CNRS, IRAP,
14 avenue Belin,
31400
Toulouse, France
26
Dept. of Earth Sciences, University of Hawai’i at Mänoa,
Honolulu, HI
96822, USA
27
Jet Propulsion Laboratory, California Institute of Technology,
4800 Oak Grove Drive,
Pasadena, CA
91109, USA
28
Wesleyan University,
Middletown, CT
06459, USA
29
Max Planck Institute for Astronomy,
Königstuhl 17,
69117
Heidelberg, Germany
30
NASA Ames Research Center,
Moffett Field, CA
94035, USA
31
LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Cité,
5 place Jules Janssen,
92195
Meudon, France
32
NASA Goddard Space Flight Center,
8800 Greenbelt Road,
Greenbelt, MD
20771, USA
33
SETI Institute,
189 Bernardo Ave, Suite 200,
Mountain View, CA
94043, USA
34
Physics & Astrophysics Group, Dept. of Physical & Environmental Sciences, University of Toronto Scarborough,
1265 Military Trail, Toronto,
Ontario,
M1C 1A4, Canada
35
David A. Dunlap Department of Astronomy & Astrophysics, University of Toronto.
50 St. George Street, Toronto,
Ontario
M5S 3H4, Canada
36
Department of Physics, University of Toronto,
60 St George Street, Toronto,
Ontario
M5S 1A7, Canada
37
Instituto de Astrofísica de Canarias (IAC),
38200
La Laguna, Tenerife, Spain
38
Dept. Astrofísica, Universidad de La Laguna (ULL),
38206
La Laguna, Tenerife, Spain
39
Department of Physics and Astronomy, University of Kansas,
1251 Wescoe Hall Drive,
Lawrence, KS
66045, USA
40
Research Institute for Advanced Computer Science, Universities Space Research Association,
Washington, DC
20024, USA
41
European Southern Observatory,
Alonso de Córdova 3107, Vitacura,
Región Metropolitana, Chile
42
Institute of Astronomy and Astrophysics, Academia Sinica,
Taipei
10617, Taiwan
Received:
25
May
2023
Accepted:
8
January
2024
We report the discovery and characterisation of a giant transiting planet orbiting a nearby M3.5V dwarf (d = 80.4pc, G = 15.1 mag, K=11.2mag, R* = 0.358 ± 0.015 R⊙, M* = 0.340 ± 0.009 M⊙). Using the photometric time series from TESS sectors 10, 36, 46, and 63 and near-infrared spectrophotometry from ExTrA, we measured a planetary radius of 0.77 ± 0.03 RJ and an orbital period of 1.52 days. With high-resolution spectroscopy taken by the CFHT/SPIRou and ESO/ESPRESSO spectrographs, we refined the host star parameters ([Fe/H] = 0.27 ± 0.12) and measured the mass of the planet (0.273 ± 0.006 MJ). Based on these measurements, TOI-4860 b joins the small set of massive planets (>80 ME) found around mid to late M dwarfs (<0.4 R⊙), providing both an interesting challenge to planet formation theory and a favourable target for further atmospheric studies with transmission spectroscopy. We identified an additional signal in the radial velocity data that we attribute to an eccentric planet candidate (e = 0.66 ± 0.09) with an orbital period of 427 ± 7 days and a minimum mass of 1.66 ± 0.26 MJ, but additional data would be needed to confirm this.
Key words: techniques: photometric / techniques: radial velocities / stars: individual: TOI-4860 / stars: low-mass / planetary systems
© The Authors 2024
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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