Issue |
A&A
Volume 689, September 2024
|
|
---|---|---|
Article Number | A52 | |
Number of page(s) | 21 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202450974 | |
Published online | 03 September 2024 |
Characterisation of the warm-Jupiter TOI-1130 system with CHEOPS and a photo-dynamical approach★
1
INAF, Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio 5,
35122
Padova,
Italy
e-mail: luca.borsato@inaf.it
2
ETH Zurich, Department of Physics,
Wolfgang-Pauli-Strasse 2,
8093
Zurich,
Switzerland
3
Observatoire astronomique de l’Université de Genève,
Chemin Pegasi 51,
1290
Versoix,
Switzerland
4
Weltraumforschung und Planetologie, Physikalisches Institut, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
5
Cavendish Laboratory,
JJ Thomson Avenue,
Cambridge
CB3 0HE,
UK
6
Department of Astronomy, Stockholm University, AlbaNova University Center,
10691
Stockholm,
Sweden
7
Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews, North Haugh,
St Andrews
KY16 9SS,
UK
8
European Space Agency (ESA), European Space Research and Technology Centre (ESTEC),
Keplerlaan 1,
2201
AZ
Noordwijk,
The Netherlands
9
Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory,
439 92
Onsala,
Sweden
10
Space Research Institute, Austrian Academy of Sciences,
Schmiedlstrasse 6,
8042
Graz,
Austria
11
Department of Physics, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL,
UK
12
CFisUC, Departamento de Física, Universidade de Coimbra,
3004-516
Coimbra,
Portugal
13
Dipartimento di Fisica, Università degli Studi di Torino,
via Pietro Giuria 1,
10125,
Torino,
Italy
14
Dipartimento di Fisica e Astronomia “Galileo Galilei”, Università degli Studi di Padova,
Vicolo dell’Osservatorio 3,
35122
Padova,
Italy
15
Laboratoire Lagrange, UMR7293, Observatoire de la Côte d’Azur, Université Côte d’Azur,
Boulevard de l’Observatoire CS 34229
06304
Nice Cedex,
France
16
School of Physics and Astronomy, University of Birmingham, Edgbaston,
Birmingham
B15 2TT,
UK
17
Center for Space and Habitability, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
18
Instituto de Astrofísica de Canarias,
Vía Láctea s/n,
38200
La Laguna, Tenerife,
Spain
19
Departamento de Astrofísica, Universidad de La Laguna,
Astrofísico Francisco Sanchez s/n,
38206
La Laguna, Tenerife,
Spain
20
Admatis,
5. Kandó Kálmán Street,
3534
Miskolc,
Hungary
21
Depto. de Astrofísica, Centro de Astrobiología (CSIC-INTA), ESAC campus,
28692
Villanueva de la Cañada (Madrid),
Spain
22
Instituto de Astrofisica e Ciencias do Espaco, Universidade do Porto, CAUP,
Rua das Estrelas,
4150-762
Porto,
Portugal
23
Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto,
Rua do Campo Alegre,
4169-007
Porto,
Portugal
24
University of Bern,
Sidlerstrasse 5,
3012
Bern,
Switzerland
25
Institute of Planetary Research, German Aerospace Center (DLR),
Rutherfordstrasse 2,
12489
Berlin,
Germany
26
INAF, Osservatorio Astrofisico di Torino,
Via Osservatorio, 20,
10025
Pino Torinese To,
Italy
27
Centre for Mathematical Sciences, Lund University,
Box 118,
221 00
Lund,
Sweden
28
Aix Marseille Univ, CNRS, CNES, LAM,
38 rue Frédéric Joliot-Curie,
13388
Marseille,
France
29
Astrobiology Research Unit, Université de Liège,
Allée du 6 Août 19C,
4000
Liège,
Belgium
30
Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège,
Allée du 6 Août 19C,
4000
Liège,
Belgium
31
Institute of Astronomy, KU Leuven,
Celestijnenlaan 200D,
3001
Leuven,
Belgium
32
ELTE Gothard Astrophysical Observatory,
Szent Imre h. u. 112,
9700
Szombathely,
Hungary
33
SRON Netherlands Institute for Space Research,
Niels Bohrweg 4,
2333
CA
Leiden,
The Netherlands
34
Centre Vie dans l’Univers, Faculté des sciences, Université de Genève,
Quai Ernest-Ansermet 30,
1211
Genève 4,
Switzerland
35
Leiden Observatory, University of Leiden,
PO Box 9513,
2300
RA
Leiden,
The Netherlands
36
National and Kapodistrian University of Athens, Department of Physics, University Campus, Zografos
GR-157 84,
Athens,
Greece
37
Department of Astrophysics, University of Vienna,
Türkenschanzstrasse 17,
1180
Vienna,
Austria
38
Institute for Theoretical Physics and Computational Physics, Graz University of Technology,
Petersgasse 16,
8010
Graz,
Austria
39
Konkoly Observatory, Research Centre for Astronomy and Earth Sciences,
Konkoly Thege Miklós út 15-17,
1121
Budapest,
Hungary
40
ELTE Eötvös Loránd University, Institute of Physics,
Pázmány Péter sétány 1/A,
1117
Budapest,
Hungary
41
Lund Observatory, Division of Astrophysics, Department of Physics, Lund University,
Box 118,
22100
Lund,
Sweden
42
IMCCE, UMR8028 CNRS, Observatoire de Paris, PSL Univ., Sorbonne Univ.,
77 av. Denfert-Rochereau,
75014
Paris,
France
43
Institut d’astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie,
98bis blvd. Arago,
75014
Paris,
France
44
Astrophysics Group, Lennard Jones Building, Keele University,
Staffordshire
ST5 5BG,
UK
45
Istituto di Scienze Polari del Consiglio Nazionale delle Ricerche (CNR-ISP),
via Torino 155,
30172
Venezia-Mestre,
Italy
46
Programma Nazionale di Ricerche in Antartide (PNRA),
Lungotevere Grande Ammiraglio Thaon di Revel 76,
00196
Rome,
Italy
47
INAF, Osservatorio Astrofisico di Catania,
Via S. Sofia 78,
95123
Catania,
Italy
48
Institute of Optical Sensor Systems, German Aerospace Center (DLR),
Rutherfordstrasse 2,
12489
Berlin,
Germany
49
Institut fuer Geologische Wissenschaften, Freie Universitaet Berlin,
Maltheserstrasse 74-100,
12249
Berlin,
Germany
50
Institut de Ciencies de l’Espai (ICE, CSIC), Campus UAB,
Can Magrans s/n,
08193
Bellaterra,
Spain
51
Institut d’Estudis Espacials de Catalunya (IEEC),
08860
Castelldefels (Barcelona),
Spain
52
HUN-REN-ELTE Exoplanet Research Group,
Szent Imre h. u. 112.,
Szombathely
9700,
Hungary
53
Institute of Astronomy, University of Cambridge,
Madingley Road,
Cambridge
CB3 0HA,
UK
Received:
3
June
2024
Accepted:
6
July
2024
Context. Among the thousands of exoplanets discovered to date, approximately a few hundred gas giants on short-period orbits are classified as ‘lonely’ and only a few are in a multi-planet system with a smaller companion on a close orbit. The processes that formed multi-planet systems hosting gas giants on close orbits are poorly understood, and only a few examples of this kind of system have been observed and well characterised.
Aims. Within the contest of a multi-planet system hosting a gas giant on short orbits, we characterise the TOI-1130 system by measuring masses and orbital parameters. This is a two-transiting planet system with a Jupiter-like planet (c) on a 8.35 days orbit and a Neptune-like planet (b) on an inner (4.07 days) orbit. Both planets show strong anti-correlated transit timing variations (TTVs). Furthermore, radial velocity (RV) analysis showed an additional linear trend, a possible hint of a non-transiting candidate planet on a far outer orbit.
Methods. Since 2019, extensive transit and radial velocity observations of the TOI-1130 have been acquired using TESS and various ground-based facilities. We present a new photo-dynamical analysis of all available transit and RV data, with the addition of new CHEOPS and ASTEP+ data, which achieve the best precision to date on the planetary radii and masses and on the timings of each transit.
Results. We were able to model interior structure of planet b constraining the presence of a gaseous envelope of H/He, while it was not possible to assess the possible water content. Furthermore, we analysed the resonant state of the two transiting planets, and we found that they lie just outside the resonant region. This could be the result of the tidal evolution that the system underwent. We obtained both masses of the planets with a precision of less than 1.5%, and radii with a precision of about 1% and 3% for planet b and c, respectively.
Key words: methods: data analysis / methods: observational / techniques: photometric / telescopes / 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.
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.