| Issue |
A&A
Volume 701, September 2025
|
|
|---|---|---|
| Article Number | A240 | |
| Number of page(s) | 22 | |
| Section | Planets, planetary systems, and small bodies | |
| DOI | https://doi.org/10.1051/0004-6361/202554040 | |
| Published online | 22 September 2025 | |
The CHEOPS view of HD 95338b: Refined transit parameters, and a search for exomoons★
1
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences,
Konkoly Thege út 15–17.,
1121
Budapest,
Hungary
2
CSFK, MTA Centre of Excellence, Budapest,
Konkoly Thege út 15–17.,
1121
Budapest,
Hungary
3
HUN-REN-ELTE Exoplanet Research Group,
Szent Imre h. u. 112.,
Szombathely
9700,
Hungary
4
ELTE Eötvös Loránd University, Doctoral School of Physics,
Budapest,
H-1117 Budapest Pázmány Péter sétány 1/A,
Hungary
5
Center for Space and Habitability, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
6
Observatoire astronomique de l’Université de Genève,
Chemin Pegasi 51,
1290
Versoix,
Switzerland
7
Institute of Space Research, German Aerospace Center (DLR),
Rutherfordstrasse 2,
12489
Berlin,
Germany
8
ELTE Gothard Astrophysical Observatory,
9700
Szombathely,
Szent Imre h. u. 112,
Hungary
9
Centre Vie dans l’Univers, Faculté des sciences, Université de Genève,
Quai Ernest-Ansermet 30,
1211
Genève 4,
Switzerland
10
Department of Physics, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL,
UK
11
European Space Agency (ESA), European Space Research and Technology Centre (ESTEC),
Keplerlaan 1,
2201
AZ
Noordwijk,
The Netherlands
12
Instituto de Astrofisica e Ciencias do Espaco, Universidade do Porto, CAUP, Rua das Estrelas,
4150-762
Porto,
Portugal
13
Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège,
Allée du 6 Août 19C,
4000
Liège,
Belgium
14
Space Research Institute, Austrian Academy of Sciences,
Schmiedlstrasse 6,
8042
Graz,
Austria
15
INAF, Osservatorio Astrofisico di Catania,
Via S. Sofia 78,
95123
Catania,
Italy
16
Department of Astronomy, Stockholm University, AlbaNova University Center,
10691
Stockholm,
Sweden
17
Instituto de Astrofísica de Canarias, Vía Láctea s/n,
38200
La Laguna, Tenerife,
Spain
18
Departamento de Astrofísica, Universidad de La Laguna, Astrofísico Francisco Sanchez s/n,
38206
La Laguna, Tenerife,
Spain
19
Admatis,
5. Kandó Kálmán Street,
3534
Miskolc,
Hungary
20
Depto. de Astrofísica, Centro de Astrobiología (CSIC-INTA), ESAC campus,
28692
Villanueva de la Cañada (Madrid),
Spain
21
Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto, Rua do Campo Alegre,
4169-007
Porto,
Portugal
22
Max Planck Institute for Extraterrestrial Physics,
Gießenbachstraße 1,
Garching bei München
85748,
Germany
23
INAF, Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio 5,
35122
Padova,
Italy
24
Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews,
North Haugh,
St Andrews
KY16 9SS,
UK
25
CFisUC, Departamento de Física, Universidade de Coimbra,
3004-516
Coimbra,
Portugal
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
SRON Netherlands Institute for Space Research,
Niels Bohrweg 4,
2333
CA
Leiden,
The Netherlands
30
Leiden Observatory, University of Leiden,
PO Box 9513,
2300
RA
Leiden,
The Netherlands
31
Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory,
439 92
Onsala,
Sweden
32
Dipartimento di Fisica, Università degli Studi di Torino,
via Pietro Giuria 1,
10125
Torino,
Italy
33
National and Kapodistrian University of Athens, Department of Physics, University Campus, Zografos
157 84,
Athens,
Greece
34
Astrobiology Research Unit, Université de Liège,
Allée du 6 Août 19C,
4000
Liège,
Belgium
35
Department of Astrophysics, University of Vienna,
Türkenschanzstrasse 17,
1180
Vienna,
Austria
36
Division Technique INSU, CS20330,
83507
La Seyne sur Mer cedex,
France
37
Institute for Theoretical Physics and Computational Physics, Graz University of Technology,
Petersgasse 16,
8010
Graz,
Austria
38
ELTE Eötvös Loránd University, Institute of Physics,
Pázmány Péter sétány 1/A,
1117
Budapest,
Hungary
39
IMCCE, UMR8028 CNRS, Observatoire de Paris, PSL Univ., Sorbonne Univ.,
77 av. Denfert-Rochereau,
75014
Paris,
France
40
Institut d’astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie,
98bis blvd. Arago,
75014
Paris,
France
41
Astrophysics Group, Lennard Jones Building, Keele University,
Staffordshire
ST5 5BG,
UK
42
European Space Agency, ESA – European Space Astronomy Centre, Camino Bajo del Castillo s/n,
28692
Villanueva de la Cañada, Madrid,
Spain
43
Weltraumforschung und Planetologie, Physikalisches Institut, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
44
Dipartimento di Fisica e Astronomia “Galileo Galilei”, Università degli Studi di Padova,
Vicolo dell’Osservatorio 3,
35122
Padova,
Italy
45
ETH Zurich, Department of Physics,
Wolfgang-Pauli-Strasse 2,
8093
Zurich,
Switzerland
46
Cavendish Laboratory,
JJ Thomson Avenue,
Cambridge
CB3 0HE,
UK
47
Fachbereich Geowissenschaften, Freie Universität Berlin, Institut für Geologische Wissenschaften, Fachrichtung Planetologie und Fernerkundung,
Malteserstr. 74–100,
12249
Berlin,
Germany
48
Institut de Ciencies de l’Espai (ICE, CSIC), Campus UAB, Can Magrans s/n,
08193
Bellaterra,
Spain
49
Institut d’Estudis Espacials de Catalunya (IEEC),
08860
Castelldefels (Barcelona),
Spain
50
Institute of Astronomy, University of Cambridge,
Madingley Road,
Cambridge
CB3 0HA,
UK
51
Deutsches Zentrum für Luft- und Raumfahrt (DLR),
Markgrafenstrasse 37,
10117
Berlin,
Germany
52
Université de Paris, Institut de physique du globe de Paris, CNRS,
75005
Paris,
France
53
Laboratory for Climate and Ocean-Atmosphere Studies, Department of Atmospheric and Oceanic Sciences, School of Physics, Peking University,
Beijing
100871,
China
★★ Corresponding author.
Received:
5
February
2025
Accepted:
15
July
2025
Context. Despite the ever-increasing number of known exoplanets, no uncontested detections have been made of their satellites, known as exomoons.
Aims. The quest to find exomoons is at the forefront of exoplanetary sciences. Certain space-born instruments are thought to be suitable for this purpose. We show the progress made with the CHaracterising ExOPlanets Satellite (CHEOPS) in this field using the HD 95338 planetary system. We present a novel methodology as an important step in the quest to find exomoons.
Methods. We utilised ground-based spectroscopic data in combination with Gaia observations to obtain precise stellar parameters. These were then used as input in the analysis of the planetary transits observed by CHEOPS and the Transiting Exoplanet Survey Satellite (TESS). In addition, we searched for the signs of satellites primarily in the form of additional transits in the Hill sphere of the eccentric Neptune-sized planet HD 95338b in a sequential approach based on four CHEOPS visits. We also briefly explored the transit timing variations of the planet.
Results. We present refined stellar and planetary parameters, narrowing down the uncertainty on the planet-to-star radius ratio by a factor of ten. We also pin down the ephemeris of HD 95338b. Using injection-and-retrieval tests, we show that a 5σ detection of an exomoon would be possible at RMoon = 0.8 R⊕ with the methodology presented here.
Conclusions. We exclude the transit of an exomoon in the HD 95338 system with RMoon ≈0.6 R⊕ at the 1σ level. The algorithm used for finding the transit-like event can be used as a baseline for other similar targets, observed by CHEOPS or other missions.
Key words: methods: data analysis / techniques: photometric / planets and satellites: individual: HD 95338b
© The Authors 2025
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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