Issue |
A&A
Volume 667, November 2022
|
|
---|---|---|
Article Number | A1 | |
Number of page(s) | 25 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202243093 | |
Published online | 28 October 2022 |
The HD 93963 A transiting system: A 1.04 d super-Earth and a 3.65 d sub-Neptune discovered by TESS and CHEOPS★
1
Dipartimento di Fisica, Università degli Studi di Torino,
via Pietro Giuria 1,
10125
Torino, Italy
e-mail: luisamaria.serrano@unito.it
2
Aix Marseille Univ., CNRS, CNES, LAM,
38 rue Frédéric JoliotCurie,
13388
Marseille, France
3
Department of Astronomy, Stockholm University, AlbaNova University Center,
10691
Stockholm, Sweden
4
Physikalisches Institut, University of Bern,
Gesellsschaftstrasse 6,
3012
Bern, Switzerland
5
Instituto de Astrofisica e Ciencias do Espaco, Universidade do Porto, CAUP,
Rua das Estrelas,
4150-762
Porto, Portugal
6
Instituto de Astrofisica de Canarias,
38200
La Laguna, Tenerife, Spain
7
Dept. Astrofísica, Universidad de La Laguna (ULL),
38206
La Laguna, Tenerife, Spain
8
NASA Exoplanet Science Institute – Caltech/IPAC,
1200 E. California Blvd,
Pasadena, CA
91125, USA
9
Space Science and Astrobiology Division NASA Ames Research Center,
M/S 245-6,
Moffett Field, CA
94035, USA
10
Center for Space and Habitability,
Gesellsschaftstrasse 6,
3012
Bern, Switzerland
11
Observatoire Astronomique de l’Université de Genève,
Chemin Pegasi 51,
Versoix, Switzerland
12
Department of Astronomy, Stockholm University,
106 91
Stockholm, Sweden
13
Space Research Institute, Austrian Academy of Sciences,
Schmiedlstrasse 6,
8042
Graz, Austria
14
Lund Observatory, Dept. of Astronomy and Theoretical Physics, Lund University,
Box 43,
22100
Lund, Sweden
15
Centre for Exoplanet Science, SUPA School of Physics and Astronomy, University of St Andrews,
North Haugh,
St Andrews
KY16 9SS, UK
16
Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology,
Cambridge, MA
02139, USA
17
Department of Physics, Shahid Beheshti University,
Tehran, Iran
18
Laboratoire J.-L. Lagrange, Observatoire de la Côte d’Azur (OCA), Université de Nice-Sophia Antipolis (UNS), CNRS,
Campus Valrose,
06108
Nice Cedex 2, France
19
Leiden Observatory, University of Leiden,
PO Box 9513,
2300 RA
Leiden, The Netherlands
20
Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory,
43992
Onsala, Sweden
21
Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University,
Ny Munkegade 120,
8000
Aarhus C, Denmark
22
Nordic Optical Telescope,
Rambla José Ana Fernández Pérez 7,
38711
Breña Baja, Spain
23
Center for Astrophysics | Harvard & Smithsonian,
60 Garden Street,
Cambridge, MA
02138, USA
24
Institute of Planetary Research, German Aerospace Center (DLR),
Rutherfordstrasse 2,
12489
Berlin, Germany
25
Rheinisches Institut für Umweltforschung an der Universität zu Köln,
Aachener Strasse 209,
50931
Köln, Germany
26
Institut de Ciencies de l’Espai (ICE, CSIC),
Campus UAB, Can Magrans s/n,
08193
Bellaterra, Spain
27
Institut d’Estudis Espacials de Catalunya (IEEC),
08034
Barcelona, Spain
28
Admatis,
5. Kandó Kálmán Street,
3534
Miskolc, Hungary
29
Depto. de Astrofisica, Centro de Astrobiología (CSIC-INTA),
ESAC campus,
28692
Villanueva de la Canada, Madrid, Spain
30
Departamento de Fisica e Astronomia, Faculdade de Ciencias, Universidade do Porto,
Rua do Campo Alegre,
4169-007
Porto, Portugal
31
Harvard-Smithsonian Center for Astrophysics,
60 Garden Street, P-333,
MS-16,
Cambridge, MA
02138, USA
32
Université Grenoble Alpes, CNRS, IPAG,
38000
Grenoble, France
33
NASA, Goddard Space Flight Center,
8800 Greenbelt Rd,
Greenbelt, MD
20771, USA
34
Université de Paris, Institut de physique du globe de Paris, CNRS,
75005
Paris, France
35
Centre for Mathematical Sciences Lund University,
Box 118,
SE 221 00
Lund, Sweden
36
Astrobiology Research Unit, Université de Liège,
Allée du 6 Août 19C,
4000
Liège, Belgium
37
Space sciences, Technologies and Astrophysics Research (STAR) Institute, Université de Liège,
Allée du 6 Août 19C,
4000
Liège, Belgium
38
University of California at Santa Cruz,
Santa Cruz, CA, USA
39
Komaba Institute for Science, The University of Tokyo,
3-8-1 Komaba, Meguro,
Tokyo
153-8902, Japan
40
Instituto de Astrofísica de Canarias (IAC),
38205
La Laguna, Tenerife, Spain
41
Astronomical Institute, Slovak Academy of Science, Stellar Department, Tatranská Lomnica,
05960
Vysoké Tatry, Slovakia
42
ELTE Eötvös Lorând University, Gothard Astrophysical Observatory,
9700
Szombathely,
Szent Imre h. u. 112,
Hungary
43
MTA-ELTE Exoplanet Research Group,
9700
Szombathely,
Szent Imre h. u. 112,
Hungary
44
MTA-ELTE Lendület Milky Way Research Group,
9700
Szombathely,
Szent Imre h. u. 112,
Hungary
45
University of Vienna, Department of Astrophysics,
Türkenschanzstrasse 17,
1180
Vienna, Austria
46
Institut d’astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie,
98bis boulevard Arago,
75014
Paris, France
47
Observatoire de Haute-Provence, CNRS, Université d’Aix-Marseille,
04870
Saint-Michel-l’Observatoire, France
48
Department of Physics, University of Warwick,
Gibbet Hill Road,
Coventry
CV4 7AL, UK
49
Science and Operations Department – Science Division (SCI-SC), Directorate of Science, European Space Agency (ESA), European Space Research and Technology Centre (ESTEC),
Keplerlaan 1,
2201-AZ
Noordwijk, The Netherlands
50
NASA Ames Research Center,
Mail Stop 269-3,
Bldg. T35A, Rm. 102,
PO Box 1,
Moffett Field, CA
94035-0001, USA
51
Konkoly Observatory, Research Centre for Astronomy and Earth Sciences,
1121
Budapest,
Konkoly Thege Miklós út 15-17,
Hungary
52
IMCCE, UMR8028 CNRS, Observatoire de Paris, PSL Univ.,
Sorbonne Univ., 77 av. Denfert-Rochereau,
75014
Paris, France
53
INAF, Osservatorio Astronomico di Padova,
Vicolo dell’Osservatorio 5,
35122
Padova, Italy
54
Astrophysics Group, Keele University,
Staffordshire
ST5 5BG, UK
55
Astrobiology Center,
2-21-1 Osawa,
Mitaka, Tokyo
181-8588, Japan
56
Department of Astrophysics, University of Vienna,
Tuerkenschanzstrasse 17,
1180
Vienna, Austria
57
INAF, Osservatorio Astrofisico di Catania,
Via S. Sofia 78,
95123
Catania, Italy
58
Citizen Scientist, Marica,
Rio de Janeiro, Brazil
59
Institute of Optical Sensor Systems, German Aerospace Center (DLR),
Rutherfordstrasse 2,
12489
Berlin, Germany
60
Dipartimento di Fisica e Astronomia “Galileo Galilei”, Universita degli Studi di Padova,
Vicolo dell’Osservatorio 3,
35122
Padova, Italy
61
ETH Zurich, Department of Physics,
Wolfgang-Pauli-Strasse 27,
8093
Zurich, Switzerland
62
Cavendish Laboratory,
JJ Thomson Avenue,
Cambridge
CB3 0HE, UK
63
ESTEC, European Space Agency,
2201 AZ
Noordwijk, The Netherlands
64
Center for Astronomy and Astrophysics, Technical University Berlin,
Hardenberstrasse 36,
10623
Berlin, Germany
65
Institut für Geologische Wissenschaften, Freie Universität Berlin,
12249
Berlin, Germany
66
Royal Astronomical Society,
Burlington House, Piccadilly,
London
W1J 0BQ, UK
67
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology,
Cambridge, MA
02139, USA
68
Department of Aeronautics and Astronautics, MIT,
77 Massachusetts Avenue,
Cambridge, MA
02139, USA
69
SETI Institute/NASA Ames Research Center,
339 Bernardo Ave, Suite 200,
Mountain View, CA
94043, US
70
Institute of Astronomy, University of Cambridge,
Madingley Road,
Cambridge
CB3 0HA, UK
Received:
12
January
2022
Accepted:
19
June
2022
We present the discovery of two small planets transiting HD 93963A (TOI-1797), a GOV star (M* = 1.109 ± 0.043M⊙, R* = 1.043 ± 0.009 R⊙) in a visual binary system. We combined TESS and CHEOPS space-borne photometry with MuSCAT 2 ground-based photometry, ‘Alopeke and PHARO high-resolution imaging, TRES and FIES reconnaissance spectroscopy, and SOPHIE radial velocity measurements. We validated and spectroscopically confirmed the outer transiting planet HD 93963 A c, a sub-Neptune with an orbital period of Pc ≈ 3.65 d that was reported to be a TESS object of interest (TOI) shortly after the release of Sector 22 data. HD 93963 A c has amass of Mc = 19.2 ± 4.1 M⊕ and a radius of Rc = 3.228 ± 0.059 R⊕, implying a mean density of ρc = 3.1 ± 0.7 g cm-3. The inner object, HD 93963 A b, is a validated 1.04 d ultra-short period (USP) transiting super-Earth that we discovered in the TESS light curve and that was not listed as a TOI, owing to the low significance of its signal (TESS signal-to-noise ratio ≈6.7, TESS + CHEOPS combined transit depth Db = 141.5−8.3+8.5 ppm). We intensively monitored the star with CHEOPS by performing nine transit observations to confirm the presence of the inner planet and validate the system. HD 93963 A b is the first small (Rb = 1.35 ± 0.042 R⊕) USP planet discovered and validated by TESS and CHEOPS. Unlike planet c, HD 93963 Ab is not significantly detected in our radial velocities (Mb = 7.8 ± 3.2 M⊕). The two planets are on either side of the radius valley, implying that they could have undergone completely different evolution processes. We also discovered a linear trend in our Doppler measurements, suggesting the possible presence of a long-period outer planet. With a V-band magnitude of 9.2, HD 93963 A is among the brightest stars known to host a USP planet, making it one of the most favourable targets for precise mass measurement via Doppler spectroscopy and an important laboratory to test formation, evolution, and migration models of planetary systems hosting ultra-short period planets.
Key words: planets and satellites: detection / planets and satellites: fundamental parameters / instrumentation: photometers / instrumentation: spectrographs / methods: data analysis
Tables of DRS and PIPE extracted lightcurves and detrended data are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/667/A1
© L. M. Serrano et al. 2022
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.