Issue |
A&A
Volume 677, September 2023
|
|
---|---|---|
Article Number | A38 | |
Number of page(s) | 20 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202346838 | |
Published online | 30 August 2023 |
TOI-2084 b and TOI-4184 b: Two new sub-Neptunes around M dwarf stars
1
Astrobiology Research Unit, Université de Liège,
Allée du 6 Août 19C,
4000
Liège, Belgium
e-mail: khalid.barkaoui@uliege.be
2
Department of Earth, Atmospheric and Planetary Science, Massachusetts Institute of Technology,
77 Massachusetts Avenue,
Cambridge, MA
02139, USA
3
Instituto de Astrofisica de Canarias (IAC),
Calle Vía Láctea s/n,
38200,
La Laguna, Tenerife, Spain
4
Oukaimeden Observatory, High Energy Physics and Astrophysics Laboratory, Faculty of sciences Semlalia, Cadi Ayyad University,
Marrakech, Morocco
5
Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto,
Rua do Campo Alegre,
4169-007
Porto, Portugal
6
Instituto de Astrofisica e Ciencias do Espaco, Universidade do porto, CAUP,
Rua das Estrelas,
150-762
Porto, Portugal
7
Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology,
Cambridge, MA
02139, USA
8
Center for Astrophysics and Space Sciences, UC San Diego,
UCSD Mail Code 0424, 9500 Gilman Drive,
La Jolla, CA
92093-0424, USA
9
Instituto de Astrofisica de Andalucia (IAA-CSIC),
Glorieta de la Astronomia s/n,
18008
Granada, Spain
10
Center for Astrophysics | Harvard & Smithsonian,
60 Garden St,
Cambridge, MA
02138, USA
11
NASA Ames Research Center,
Moffett Field, CA
94035, USA
12
Department of Physics & Astronomy, Vanderbilt University,
6301 Stevenson Center Ln.,
Nashville, TN
37235, USA
13
Instituto de Astronomia y Ciencias Planetarias de Atacama, Universidad de Atacama,
Copayapu 485,
Copiapo, Chile
14
Univ. Grenoble Alpes, CNRS, IPAG,
38000
Grenoble, France
15
Observatoire de Genève, Département d’Astronomie, Université de Genève,
Chemin Pegasi 51,
1290
Versoix, Switzerland
16
NASA Exoplanet Science Institute, Caltech/IPAC,
Mail Code 100-22, 1200 E. California Blvd.,
Pasadena, CA
91125, USA
17
Departamento de Astrofisica, Universidad de La Laguna (ULL),
38206
La Laguna, Tenerife, Spain
18
Institute for Astronomy, The University of Edinburgh, Royal Observatory,
Blackford Hill,
Edinburgh
EH9 3HJ, UK
19
Space Sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège,
Allée du 6 Août 19C,
4000
Liège, Belgium
20
University of St Andrews, Centre for Exoplanet Science, SUPA School of Physics & Astronomy,
North Haugh,
St Andrews,
KY16 9SS, UK
21
Center for Space and Habitability, University of Bern,
Gesellschaftsstrasse 6,
3012,
Bern, Switzerland
22
School of Physics & Astronomy, University of Birmingham,
Edgbaston,
Birmingham
B15 2TT, UK
23
AIM, CEA, CNRS, Université Paris-Saclay, Université de Paris,
91191
Gif-sur-Yvette, France
24
Komaba Institute for Science, The University of Tokyo,
3-8-1 Komaba, Meguro,
Tokyo
153-8902, Japan
25
University of Southern Denmark, University Library,
Campusvej 55,
5230
Odense M, Denmark
26
Cavendish Laboratory,
JJ Thomson Avenue,
Cambridge
CB3 0HE, UK
27
Centre for ExoLife Sciences, Niels Bohr Institute, University of Copenhagen,
Øster Voldgade 5,
1350
Copenhagen, Denmark
28
Universidad Nacional Autonoma de México, Instituto de Astronomia,
AP 70-264,
Ciudad de México
04510, Mexico
29
European Space Agency (ESA), European Space Research and Technology Centre (ESTEC),
Keplerlaan 1,
2201 AZ
Noordwijk, The Netherlands
30
Department of Physics and Astronomy, Georgia State University,
Atlanta, GA
30302-4106, USA
31
RECONS Institute,
Chambersburg, PA
17201, USA
32
Department of Physics, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL, UK
33
Department of Astrophysical and Planetary Sciences, University of Colorado Boulder,
Boulder, CO
80309, USA
34
Astrobiology Center,
2-21-1 Osawa, Mitaka,
Tokyo
181-8588, Japan
35
Universidad Nacional Autonoma de México, Instituto de Astronomia,
AP 106,
Ensenada
22800,
BC, Mexico
36
Department of Physics, Isfahan University of Technology,
Isfahan
84156-83111, Iran
37
Department of Astronomy, University of Maryland,
College Park, MD
20742, USA
38
South African Astronomical Observatory,
PO Box 9,
Observatory,
Cape Town
7935, South Africa
39
Astrophysics Group, Keele University,
Staffordshire
ST5 5BG, UK
40
Kotizarovci Observatory,
Sarsoni 90,
51216
Viskovo, Croatia
41
Department of Astrophysical Sciences, Princeton University,
Princeton, NJ
08544, USA
Received:
8
May
2023
Accepted:
26
June
2023
We present the discovery and validation of two TESS exoplanets orbiting nearby M dwarfs: TOI-2084 b, and TOI-4184b. We characterized the host stars by combining spectra from Shane/Kast and Magellan/FIRE, spectral energy distribution analysis, and stellar evolutionary models. In addition, we used Gemini-South/Zorro & -North/Alopeke high-resolution imaging, archival science images, and statistical validation packages to support the planetary interpretation. We performed a global analysis of multi-colour photometric data from TESS and ground-based facilities in order to derive the stellar and planetary physical parameters for each system. We find that TOI-2084 band TOI-4184 bare sub-Neptune-sized planets with radii of Rp = 2.47 ± 0.13R⊕ and Rp = 2.43 ± 0.21 R⊕, respectively. TOI-2084 b completes an orbit around its host star every 6.08 days, has an equilibrium temperature of Teq = 527 ± 8 K and an irradiation of Sp = 12.8 ± 0.8 S⊕. Its host star is a dwarf of spectral M2.0 ± 0.5 at a distance of 114 pc with an effective temperature of Teff = 3550 ± 50 K, and has a wide, co-moving M8 companion at a projected separation of 1400 au. TOI-4184 b orbits around an M5.0 ± 0.5 type dwarf star (Kmag = 11.87) each 4.9 days, and has an equilibrium temperature of Teq = 412 ± 8 K and an irradiation of Sp = 4.8 ± 0.4 S⊕. TOI-4184 is a metal poor star ([Fe/H] = −0.27 ± 0.09 dex) at a distance of 69 pc with an effective temperature of Teff = 3225 ± 75 K. Both planets are located at the edge of the sub-Jovian desert in the radius-period plane. The combination of the small size and the large infrared brightness of their host stars make these new planets promising targets for future atmospheric exploration with JWST.
Key words: techniques: photometric / stars: low-mass
© The Authors 2023
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.
This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.