Issue |
A&A
Volume 688, August 2024
|
|
---|---|---|
Article Number | A223 | |
Number of page(s) | 30 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202450472 | |
Published online | 27 August 2024 |
Unveiling the internal structure and formation history of the three planets transiting HIP 29442 (TOI-469) with CHEOPS★
1
Weltraumforschung und Planetologie, Physikalisches Institut, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
e-mail: jo-ann.egger@unibe.ch
2
Center for Space and Habitability, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
3
Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology,
Cambridge,
MA
02139,
USA
4
Space Research Institute, Austrian Academy of Sciences,
Schmiedlstrasse 6,
8042
Graz,
Austria
5
European Space Agency (ESA), European Space Research and Technology Centre (ESTEC),
Keplerlaan 1,
2201
AZ
Noordwijk,
The Netherlands
6
Observatoire astronomique de l’Université de Genève,
Chemin Pegasi 51,
1290
Versoix,
Switzerland
7
Department of Astronomy, Stockholm University, AlbaNova University Center,
10691
Stockholm,
Sweden
8
INAF – Osservatorio Astrofisico di Torino,
Via Osservatorio 20,
10025
Pino Torinese,
Italy
9
Department of Physics, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL,
UK
10
Instituto de Astrofisica e Ciencias do Espaco, Universidade do Porto, CAUP, Rua das Estrelas,
4150-762
Porto,
Portugal
11
Astrobiology Research Unit, Université de Liège,
Allée du 6 Août 19C,
4000
Liège,
Belgium
12
Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège,
Allée du 6 Août 19C,
4000
Liège,
Belgium
13
Institute of Astronomy, KU Leuven,
Celestijnenlaan 200D,
3001
Leuven,
Belgium
14
Cavendish Laboratory,
JJ Thomson Avenue,
Cambridge
CB3 0HE,
UK
15
Dipartimento di Fisica e Astronomia “Galileo Galilei”, Università degli Studi di Padova,
Vicolo dell’Osservatorio 3,
35122
Padova,
Italy
16
INAF, Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio 5,
35122
Padova,
Italy
17
Department of Astronomy & Astrophysics, University of Chicago,
Chicago,
IL
60637,
USA
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
Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto, Rua do Campo Alegre,
4169-007
Porto,
Portugal
23
Institute of Optical Sensor Systems, German Aerospace Center (DLR),
Rutherfordstrasse 2,
12489
Berlin,
Germany
24
Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews,
North Haugh,
St Andrews
KY16 9SS,
UK
25
CFisUC, Department of Physics, University of Coimbra,
3004-516
Coimbra,
Portugal
26
AIRBUS DS Madrid,
Paseo John Lennon 2,
28906
Getafe (Madrid),
Spain
27
Institute of Planetary Research, German Aerospace Center (DLR),
Rutherfordstrasse 2,
12489
Berlin,
Germany
28
INAF, Osservatorio Astrofisico di Torino,
Via Osservatorio, 20,
10025
Pino Torinese To,
Italy
29
Centre for Mathematical Sciences, Lund University,
Box 118,
221 00
Lund,
Sweden
30
Aix Marseille Univ, CNRS, CNES, LAM,
38 rue Frédéric Joliot-Curie,
13388
Marseille,
France
31
ELTE Gothard Astrophysical Observatory,
Szent Imre h. u. 112,
9700
Szombathely,
Hungary
32
SRON Netherlands Institute for Space Research,
Niels Bohrweg 4,
2333
CA
Leiden,
The Netherlands
33
Centre Vie dans l’Univers, Faculté des sciences, Université de Genève,
Quai Ernest-Ansermet 30,
1211
Genève 4,
Switzerland
34
Leiden Observatory, University of Leiden,
PO Box 9513,
2300
RA
Leiden,
The Netherlands
35
Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory,
439 92
Onsala,
Sweden
36
Dipartimento di Fisica, Università degli Studi di Torino,
via Pietro Giuria 1,
10125,
Torino,
Italy
37
National and Kapodistrian University of Athens, Department of Physics, University Campus, Zografos
157 84,
Athens,
Greece
38
Department of Astrophysics, University of Vienna,
Türkenschanzstrasse 17,
1180
Vienna,
Austria
39
Institute for Theoretical Physics and Computational Physics, Graz University of Technology,
Petersgasse 16,
8010
Graz,
Austria
40
Konkoly Observatory, Research Centre for Astronomy and Earth Sciences,
Konkoly Thege Miklós út 15-17,
1121
Budapest,
Hungary
41
ELTE Eötvös Loránd University, Institute of Physics,
Pázmány Péter sétány 1/A,
1117
Budapest,
Hungary
42
Lund Observatory, Division of Astrophysics, Department of Physics, Lund University,
Box 118,
22100
Lund,
Sweden
43
IMCCE, UMR8028 CNRS, Observatoire de Paris, PSL Univ., Sorbonne Univ.,
77 av. Denfert-Rochereau,
75014
Paris,
France
44
Institut d’astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie,
98bis blvd. Arago,
75014
Paris,
France
45
Astrophysics Group, Lennard Jones Building, Keele University,
Staffordshire,
ST5 5BG,
UK
46
European Space Agency, ESA - European Space Astronomy Centre,
Camino Bajo del Castillo s/n,
28692
Villanueva de la Cañada, Madrid,
Spain
47
INAF, Osservatorio Astrofisico di Catania,
Via S. Sofia 78,
95123
Catania,
Italy
48
ETH Zurich, Department of Physics,
Wolfgang-Pauli-Strasse 2,
8093
Zurich,
Switzerland
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
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas,
4150-762
Porto,
Portugal
53
Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Rua do Campo Alegre,
4169-007
Porto,
Portugal
54
HUN-REN-ELTE Exoplanet Research Group,
Szent Imre h. u. 112.,
Szombathely
9700,
Hungary
55
Institute of Astronomy, University of Cambridge,
Madingley Road,
Cambridge,
CB3 0HA,
UK
Received:
22
April
2024
Accepted:
25
June
2024
Multiplanetary systems spanning the radius valley are ideal testing grounds for exploring the different proposed explanations for the observed bimodality in the radius distribution of close-in exoplanets. One such system is HIP 29442 (TOI-469), an evolved K0V star hosting two super-Earths and one sub-Neptune. We observed HIP 29442 with CHEOPS for a total of 9.6 days, which we modelled jointly with two sectors of TESS data to derive planetary radii of 3.410 ± 0.046, 1.551 ± 0.045, and 1.538 ± 0.049 R⊕ for planets b, c, and d, which orbit HIP 29442 with periods of 13.6, 3.5, and 6.4 days, respectively. For planet d this value deviates by more than 3σ from the median value reported in the discovery paper, leading us to conclude that caution is required when using TESS photometry to determine the radii of small planets with low per-transit signal-to-noise ratios and large gaps between observations. Given the high precision of these new radii, combining them with published RVs from ESPRESSO and HIRES provides us with ideal conditions to investigate the internal structure and formation pathways of the planets in the system. We introduced the publicly available code plaNETic, a fast and robust neural network-based Bayesian internal structure modelling framework. We then applied hydrodynamic models to explore the upper atmospheric properties of these inferred structures. Finally, we identified planetary system analogues in a synthetic population generated with the Bern model for planet formation and evolution. Based on this analysis, we find that the planets likely formed on opposing sides of the water iceline from a protoplanetary disk with an intermediate solid mass. We finally report that the observed parameters of the HIP 29442 system are compatible with a scenario where the second peak in the bimodal radius distribution corresponds to sub-Neptunes with a pure H/He envelope and with a scenario with water-rich sub-Neptunes.
Key words: techniques: photometric / planets and satellites: formation / planets and satellites: interiors / planets and satellites: individual: HIP 29442 / planetary systems
This article uses data from the CHEOPS Guaranteed Time Observation programme CH_PR100031. The raw and detrended photometric time-series data are 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/688/A223
© 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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