Issue |
A&A
Volume 694, February 2025
|
|
---|---|---|
Article Number | A137 | |
Number of page(s) | 15 | |
Section | Planets, planetary systems, and small bodies | |
DOI | https://doi.org/10.1051/0004-6361/202452699 | |
Published online | 10 February 2025 |
Transit-timing variations in the AU Mic system observed with CHEOPS★
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 Gothard Astrophysical Observatory,
9700
Szombathely,
Szent Imre h. u. 112,
Hungary
5
INAF, Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio 5,
35122
Padova,
Italy
6
Dipartimento di Fisica, Università degli Studi di Torino,
via Pietro Giuria 1,
10125
Torino,
Italy
7
Observatoire astronomique de l’Université de Genève,
Chemin Pegasi 51,
1290
Versoix,
Switzerland
8
European Space Agency (ESA), European Space Research and Technology Centre (ESTEC),
Keplerlaan 1,
2201 AZ
Noordwijk,
The Netherlands
9
Department of Physics, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL,
UK
10
Department of Astronomy, Stockholm University, AlbaNova University Center,
10691
Stockholm,
Sweden
11
Astronomical Institute, Slovak Academy of Sciences,
05960
Tatranská Lomnica,
Slovakia
12
Center for Space and Habitability, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
13
Space Research and Planetary Sciences, Physics Institute, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
14
Instituto de Astrofísica de Canarias,
Vía Láctea s/n,
38200
La Laguna,
Tenerife,
Spain
15
Departamento de Astrofísica, Universidad de La Laguna,
Astrofísico Francisco Sanchez s/n,
38206
La Laguna,
Tenerife,
Spain
16
Admatis,
5. Kandó Kálmán Street,
3534
Miskolc,
Hungary
17
Depto. de Astrofísica, Centro de Astrobiología (CSIC-INTA), ESAC campus,
28692
Villanueva de la Cañada (Madrid),
Spain
18
Instituto de Astrofisica e Ciencias do Espaco, Universidade do Porto, CAUP, Rua das Estrelas,
4150-762
Porto,
Portugal
19
Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto, Rua do Campo Alegre,
4169-007
Porto,
Portugal
20
Space Research Institute, Austrian Academy of Sciences,
Schmiedlstrasse 6,
8042
Graz,
Austria
21
Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews,
North Haugh,
St Andrews
KY16 9SS,
UK
22
CFisUC, Departamento de Física, Universidade de Coimbra,
3004516
Coimbra,
Portugal
23
Institute of Planetary Research, German Aerospace Center (DLR),
Rutherfordstrasse 2,
12489
Berlin,
Germany
24
INAF, Osservatorio Astrofisico di Torino,
Via Osservatorio, 20,
10025
Pino Torinese,
To,
Italy
25
Centre for Mathematical Sciences, Lund University,
Box 118,
221 00
Lund,
Sweden
26
Aix Marseille Univ, CNRS, CNES, LAM,
38 rue Frédéric Joliot-Curie,
13388
Marseille,
France
27
SRON Netherlands Institute for Space Research,
Niels Bohrweg 4,
2333 CA
Leiden,
The Netherlands
28
Centre Vie dans l’Univers, Faculté des sciences, Université de Genève,
Quai Ernest-Ansermet 30,
1211
Genève 4,
Switzerland
29
Leiden Observatory, University of Leiden,
PO Box 9513,
2300 RA
Leiden,
The Netherlands
30
Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory,
439 92
Onsala,
Sweden
31
National and Kapodistrian University of Athens, Department of Physics, University Campus,
Zografos
157 84,
Athens,
Greece
32
Astrobiology Research Unit, Université de Liège,
Allée du 6 Août 19C,
4000
Liège,
Belgium
33
Department of Astrophysics, University of Vienna,
Türkenschanzstrasse 17,
1180
Vienna,
Austria
34
Division Technique INSU,
CS20330,
83507
La Seyne sur Mer cedex,
France
35
Institute for Theoretical Physics and Computational Physics, Graz University of Technology,
Petersgasse 16,
8010
Graz,
Austria
36
Konkoly Observatory, Research Centre for Astronomy and Earth Sciences,
1121
Budapest,
Konkoly Thege Miklós út 15–17,
Hungary
37
ELTE Eötvös Loránd University, Institute of Physics,
Pázmány Péter sétány 1/A,
1117
Budapest,
Hungary
38
Lund Observatory, Division of Astrophysics, Department of Physics, Lund University,
Box 118,
22100
Lund,
Sweden
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
INAF, Osservatorio Astrofisico di Catania,
Via S. Sofia 78,
95123
Catania,
Italy
44
Institute of Optical Sensor Systems, German Aerospace Center (DLR),
Rutherfordstrasse 2,
12489
Berlin,
Germany
45
Weltraumforschung und Planetologie, Physikalisches Institut, University of Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
46
Dipartimento di Fisica e Astronomia “Galileo Galilei”, Università degli Studi di Padova,
Vicolo dell’Osservatorio 3,
35122
Padova,
Italy
47
ETH Zurich, Department of Physics,
Wolfgang-Pauli-Strasse 2,
8093
Zurich,
Switzerland
48
Cavendish Laboratory,
JJ Thomson Avenue,
Cambridge
CB3 0HE,
UK
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
Weltraumforschung und Planetologie, Physikalisches Institut, University of Bern,
Sidlerstrasse 5,
3012
Bern,
Switzerland
53
ESOC, European Space Agency,
Robert Bosch Str. 5,
64293
Darmstadt,
Germany
54
Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège,
Allée du 6 Août 19C,
4000
Liège,
Belgium
55
Institute of Astronomy, University of Cambridge,
Madingley Road,
Cambridge
CB3 0HA,
UK
56
Leibniz Institute for Astrophysics,
An der Sternwarte 16,
14482
Potsdam,
Germany
★★ Corresponding author; boldog.adam@csfk.org
Received:
22
October
2024
Accepted:
8
January
2025
Context. AU Mic is a very active M dwarf star with an edge-on debris disk and two known transiting sub-Neptunes with a possible third planetary companion. The two transiting planets exhibit significant transit-timing variations (TTVs) that are caused by the gravi tational interaction between the bodies in the system.
Aims. Using photometrical observations taken with the CHaracterizing ExOPlanet Satellite (CHEOPS), we aim to constrain the plan etary radii, the orbital distances, and the periods of AU Mic b and c. Furthermore, our goal is to determine the superperiod of the TTVs for AU Mic b and to update the transit ephemeris for both planets. Additionally, based on the perceived TTVs, we study the possible presence of a third planet in the system.
Methods. We conducted ultra-high precision photometric observations with CHEOPS in 2022 and 2023. We used Allesfitter to fit the planetary transits and to constrain the planetary and orbital parameters. We combined our new measurements with results from previous years to determine the periods and amplitudes of the TTVs. We applied dynamical modelling based on TTV measurements from the 2018–2023 period to reconstruct the perceived variations.
Results. We found that the orbital distances and periods for AU Mic b and c agree with the results from previous works. However, the values for the planetary radii deviate slightly from previous values, which we attribute to the effect of spots on the stellar surface. AU Mic c showed very strong TTVs, with transits that occurred ∼80 minutes later in 2023 than in 2021. Through a dynamical analysis of the system, we found that the observed TTVs can be explained by a third planet with an orbital period of ∼12.6 days and a mass of 0.203−0.024+0.022 M⊕. We explored the orbital geometry of the system and found that AU Mic c has a misaligned retrograde orbit. The limited number of AU Mic observations prevented us from determining the exact dynamical configuration and planetary parameters. Further monitoring of the system with CHEOPS might help to improve these results.
Key words: planets and satellites: fundamental parameters
© 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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