Issue |
A&A
Volume 669, January 2023
|
|
---|---|---|
Article Number | A109 | |
Number of page(s) | 23 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202243879 | |
Published online | 24 January 2023 |
TOI-969: a late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter★,★★
1
Centro de Astrobiología (CAB, CSIC-INTA), Depto. de Astrofísica,
ESAC campus,
28692
Villanueva de la Cañada (Madrid), Spain
e-mail: Jorge.Lillo@cab.inta-csic.es
2
Dipartimento di Fisica, Universitá degli Studi di Torino,
via Pietro Giuria 1,
10125
Torino, Italy
3
Department of Physics, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL, UK
4
Centre for Exoplanets and Habitability, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL, UK
5
Center for Astrophysics, Harvard & Smithsonian,
60 Garden Street,
Cambridge, MA
02138, USA
6
European Southern Observatory,
Karl-Schwarzschildstr. 2,
85748
Garching bei München, Germany
7
Observatoire astronomique de l’Université de Genève,
Chemin Pegasi 51,
1290
Versoix, Switzerland
8
Instituto de Astrofísica de Andalucía (IAA-CSIC),
Glorieta de la Astronomía s/n,
18008
Granada, Spain
9
Chalmers University of Technology, Department of Space, Earth and Environment, Onsala Space Observatory,
439 92
Onsala, Sweden
10
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas,
4150-762
Porto, Portugal
11
Aix-Marseille Univ., CNRS, CNES, LAM,
Marseille, France
12
NASA Ames Research Center,
Moffett Field, CA
94035, USA
13
Instituto de Astrofísica de Canarias (IAC),
38205
La Laguna, Tenerife, Spain
14
Departamento de Astrofísica, Universidad de La Laguna (ULL),
38206,
La Laguna, Tenerife, Spain
15
Astrophysics Group, Keele University,
Staffordshire
ST5 5BG, UK
16
Department of Astronomy, University of California Berkeley,
Berkeley, CA
94720, USA
17
Department of Physics and Astronomy, Vanderbilt University,
Nashville, TN
37235, USA
18
Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto,
Rua do Campo Alegre,
4169-007
Porto, Portugal
19
Institute of Astronomy, University of Cambridge,
Madingley Road,
Cambridge,
CB3 0HA, UK
20
Komaba Institute for Science, The University of Tokyo,
3-8-1 Komaba, Meguro,
Tokyo
153-8902, Japan
21
Astrobiology Center,
2-21-1 Osawa, Mitaka,
Tokyo
181-8588, Japan
22
Department of Astronomy, University of Maryland,
College Park, MD
20742, USA
23
Center for Space and Habitability, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern, Switzerland
24
Carnegie Earth & Planets Laboratory,
5241 Broach Branch Road NW,
Washington, DC
20015, USA
25
Department of Astrophysical Sciences, Princeton University,
Princeton, NJ
08544, USA
26
SETI Institute/NASA Ames Research Center,
Moffett Field, CA
94035, USA
27
The Observatories of the Carnegie Institution for Science,
813 Santa Barbara St,
Pasadena, CA
91101, USA
28
International Center for Advanced Studies (ICAS) and ICIFI (CONICET), ECyT-UNSAM,
Campus Miguelete, 25 de Mayo y Francia,
(1650)
Buenos Aires, Argentina
29
Department of Astronomy of the University of Geneva,
51 Chemin de Pegasi,
1290
Versoix, Switzerland
30
Thüringer Landessternwarte Tautenburg,
Sternwarte 5,
07778
Tautenburg, Germany
31
Space Telescope Science Institute,
3700 San Martin Drive,
Baltimore, MD,
21218, USA
32
Max Planck Institute for Astronomy,
Königstuhl 17,
69117
Heidelberg, Germany
33
Department of Physics and Astronomy, University of New Mexico,
210 Yale Blvd NE,
Albuquerque, NM
87106, USA
34
Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology,
Cambridge, MA
02139, USA
35
Center for Data Intensive and Time Domain Astronomy, Department of Physics and Astronomy, Michigan State University,
East Lansing, MI
48824, USA
36
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology,
Cambridge, MA
02139, USA
37
Department of Aeronautics and Astronautics, MIT,
77 Massachusetts Avenue,
Cambridge, MA
02139, USA
38
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata,
Paseo del Bosque s/n,
(B1900)
Buenos Aires, Argentina
39
Department of Astronomy, Tsinghua University,
Beijing
100084, PR China
40
University of Southern Queensland, Centre for Astrophysics,
West Street,
Toowoomba, QLD
4350 Australia
Received:
27
April
2022
Accepted:
14
October
2022
Context. The current architecture of a given multi-planetary system is a key fingerprint of its past formation and dynamical evolution history. Long-term follow-up observations are key to complete their picture.
Aims. In this paper, we focus on the confirmation and characterization of the components of the TOI-969 planetary system, where TESS detected a Neptune-size planet candidate in a very close-in orbit around a late K-dwarf star.
Methods. We use a set of precise radial velocity observations from HARPS, PFS, and CORALIE instruments covering more than two years in combination with the TESS photometric light curve and other ground-based follow-up observations to confirm and characterize the components of this planetary system.
Results. We find that TOI-969 b is a transiting close-in (Pb ~ 1.82 days) mini-Neptune planet (mb = 9.1−1.0+1.1 M⊕, Rb = 2.765−0.097+0.088 R⊕), placing it on the lower boundary of the hot-Neptune desert (Teq,b = 941 ± 31 K). The analysis of its internal structure shows that TOI-969 b is a volatile-rich planet, suggesting it underwent an inward migration. The radial velocity model also favors the presence of a second massive body in the system, TOI-969 c, with a long period of Pc = 1700−280+290 days, a minimum mass of mc sin ic = 11.3−0.9+1.1 MJup, and a highly eccentric orbit of ec = 0.628−0.036+0.043.
Conclusions. The TOI-969 planetary system is one of the few around K-dwarfs known to have this extended configuration going from a very close-in planet to a wide-separation gaseous giant. TOI-969 b has a transmission spectroscopy metric of 93 and orbits a moderately bright (G = 11.3 mag) star, making it an excellent target for atmospheric studies. The architecture of this planetary system can also provide valuable information about migration and formation of planetary systems.
Key words: planets and satellites: detection / planets and satellites: fundamental parameters / planets and satellites: composition / techniques: radial velocities / techniques: photometric / stars: individual: TOI-969
Full Tables A.1–A.4 is only available at the CDS via anonymous ftp to cdsarc.cds.unistra.fr (130.79.128.5) or via https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/669/A109
© 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.
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