Issue |
A&A
Volume 675, July 2023
|
|
---|---|---|
Article Number | A39 | |
Number of page(s) | 15 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202346406 | |
Published online | 30 June 2023 |
Three Saturn-mass planets transiting F-type stars revealed with TESS and HARPS
TOI-615b, TOI-622b, and TOI-2641b★
1
Observatoire de Genève, Université de Genève,
Chemin Pegasi 51,
1290
Versoix, Switzerland
e-mail: angeliki.psaridi@unige.ch
2
Vanderbilt University, Department of Physics & Astronomy,
6301 Stevenson Center Lane,
Nashville, TN
37235, USA
3
Astrophysics Group, Keele University,
Staffordshire
ST5 5BG, UK
4
Department of Physics, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL, UK
5
Centre for Exoplanets and Habitability, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL, UK
6
Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange,
Bd de l’Observatoire,
CS 34229,
06304
Nice cedex 4, France
7
Physikalisches Institut, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern, Switzerland
8
Astrobiology Research Unit, Université de Liège,
19C Allée du 6 Août,
4000
Liège, Belgium
9
Department of Earth, Atmospheric and Planetary Science, Massachusetts Institute of Technology,
77 Massachusetts Avenue,
Cambridge, MA
02139, USA
10
Instituto de Astrofísica de Canarias (IAC),
Calle Vía Láctea s/n,
38200
La Laguna, Tenerife, Spain
11
Center for Data Intensive and Time Domain Astronomy, Department of Physics and Astronomy, Michigan State University,
East Lansing, MI
48824, USA
12
Mullard Space Science Laboratory, University College London,
Holmbury St Mary, Dorking,
Surrey
RH5 6NT, UK
13
El Sauce Observatory,
Río Hurtado,
Coquimbo Province, Chile
14
University of Southern Queensland, Centre for Astrophysics,
West Street,
Toowoomba
QLD 4350, Australia
15
Department of Astrophysical Sciences, Princeton University,
Princeton, NJ
08544, USA
16
Center for Astrophysics | Harvard & Smithsonian,
60 Garden Street,
Cambridge, MA
02138, USA
17
University of Grenoble Alpes, CNRS, IPAG,
38000
Grenoble, France
18
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CauP,
Rua das Estrelas,
4150-762
Porto, Portugal
19
Department of Physics, Engineering and Astronomy, Stephen F. Austin State University,
1936 North St,
Nacogdoches, TX
75962, USA
20
Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology,
Cambridge, MA
02139, USA
21
Department of Aeronautics and Astronautics, Massachusetts Institute of Technology,
Cambridge, MA
02139, USA
22
SETI Institute,
189 Bernardo Ave, Suite 200,
Mountain View, CA
94043, USA
23
Facultad de Ingeniera y Ciencias, Universidad Adolfo Ibáñez,
Av. Diagonal las Torres
2640,
Peñalolén, Santiago, Chile
24
Millennium Institute for Astrophysics, Faculty of Physics,
Campus San Joaquin UC, Av. Vicuna Mackenna,
4860
Mascul, Santiago, Chile
25
Data Observatory Foundation, Eliodoro Yáñez,
2990
Providencia, Santiago, Chile
26
European Southern Observatory,
Alonso de Córdova 3107, Vitacura, Casilla,
19001
Santiago, Chile
27
NASA Ames Research Center,
Moffett Field, CA
94035, USA
28
Swinburne University of Technology, Centre for Astrophysics and Supercomputing,
John Street,
Hawthorn, VIC
3122, Australia
29
Cerro Tololo Inter-American Observatory/NSF’s NOIRLab,
Casilla 603,
La Serena, Chile
30
Astrophysics Group, Cavendish Laboratory,
J.J. Thomson Avenue,
Cambridge
CB3 0HE, UK
31
George Mason University,
4400 University Drive,
Fairfax, VA
22030, USA
32
Department of Extrasolar Planets and Atmospheres, Institute of Planetary Research, German Aerospace Center (DLR),
Rutherfordstraße 2,
12489
Berlin, Germany
33
Bryant Space Science Center, Department of Astronomy, University of Florida,
Gainesville, FL
32611, USA
34
University of Maryland, Baltimore County,
Baltimore, MD
21250, USA
35
NASA Goddard Space Flight Center,
8800 Greenbelt Rd,
Greenbelt, MD
20771, USA
36
Space Research Institute, Austrian Academy of Sciences,
Schmiedl-straße 6,
8042
Graz, Austria
37
Department of Physics and Astronomy, The University of North Carolina at Chapel Hill,
Chapel Hill, NC
27599-3255, USA
38
European Southern Observatory,
Karl-Schwarzschild-Strae 2,
85748
Garching bei München, Germany
39
South African Astronomical Observatory,
PO Box 9,
Observatory, Cape Town
7935, South Africa
40
School of Physics & Astronomy, University of Birmingham,
Edg-baston, Birmingham
B15 2TT, UK
41
Department of Electrical Engineering and Center of Astro Engineering, Pontificia Universidad Católica de Chile,
Av. Vicuña Mackenna
4860,
Santiago, Chile
42
Departamento de Astronomia, Universidad de Chile,
Casilla 36-D,
Santiago, Chile
43
Astrophysics Research Centre, Queen’s University Belfast,
Belfast
BT7 1NN, UK
Received:
14
March
2023
Accepted:
2
May
2023
While the sample of confirmed exoplanets continues to grow, the population of transiting exoplanets around early-type stars is still limited. These planets allow us to investigate the planet properties and formation pathways over a wide range of stellar masses and study the impact of high irradiation on hot Jupiters orbiting such stars. We report the discovery of TOI-615b, TOI-622b, and TOI-2641b, three Saturn-mass planets transiting main sequence, F-type stars. The planets were identified by the Transiting Exoplanet Survey Satellite (TESS) and confirmed with complementary ground-based and radial velocity observations. TOI-615b is a highly irradiated (~1277 F⊕) and bloated Saturn-mass planet (1.69−0.06+0.05 RJup and 0.43−0.08+0.09 MJup) in a 4.66 day orbit transiting a 6850 K star. TOI-622b has a radius of 0.82−0.03+0.03 RJup and a mass of 0.30−0.08+0.07 MJup in a 6.40 day orbit. Despite its high insolation flux (~600 F⊕), TOI-622b does not show any evidence of radius inflation. TOI-2641b is a 0.39−0.04+0.02 MJup planet in a 4.88 day orbit with a grazing transit (b = 1.04−0.06+0.05) that results in a poorly constrained radius of 1.61−0.64+0.46 RJup. Additionally, TOI-615b is considered attractive for atmospheric studies via transmission spectroscopy with ground-based spectrographs and JWST. Future atmospheric and spin-orbit alignment observations are essential since they can provide information on the atmospheric composition, formation, and migration of exoplanets across various stellar types.
Key words: planets and satellites: individual: TOI-615b / planets and satellites: individual: TOI-622b / stars: early-type / techniques: photometric / techniques: radial velocities / planets and satellites: individual: TOI-2641b
The photometric and radial velocity data in this work are 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/675/A39
© 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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