Issue |
A&A
Volume 675, July 2023
|
|
---|---|---|
Article Number | A115 | |
Number of page(s) | 19 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202244617 | |
Published online | 07 July 2023 |
TOI-1130: A photodynamical analysis of a hot Jupiter in resonance with an inner low-mass planet★
1
Department of Space, Earth and Environment, Astronomy and Plasma Physics, Chalmers University of Technology,
Chalmersplatsen 4,
412 96
Gothenburg, Sweden
e-mail: judith.korth@fysik.lu.se
2
Lund Observatory, Division of Astrophysics, Department of Physics, Lund University,
Box 43,
22100
Lund, Sweden
3
Dipartimento di Fisica, Università degli Studi di Torino,
via Pietro Giuria 1,
10125
Torino, Italy
4
Astronomical Institute of the Czech Academy of Sciences,
Fričova 298,
25165
Ondřejov, Czech Republic
5
Astronomical Institute of Charles University,
V Holešovičkách 2,
180 00
Prague, Czech Republic
6
ESO,
Karl-Schwarzschild-Straße 2,
85748
Garching bei München, Germany
7
Center for Astrophysics, Harvard & Smithsonian,
60 Garden Street,
Cambridge, MA
02138, USA
8
Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange,
Bd de l’Observatoire,
CS 34229,
06304
Nice Cedex 4, France
9
Department of Physics, Faculty of Sciences, Ferdowsi University of Mashhad,
Mashhad
91775-1436, Iran
10
Instituto de Astrofísica de Canarias (IAC),
38200
La Laguna, Tenerife, Spain
11
Universidad de La Laguna (ULL), Departamento de Astrofísica,
38206
La Laguna, Tenerife, Spain
12
Institute for Planetary Research, German Aerospace Center (DLR),
Rutherfordstr. 2,
12489
Berlin, Germany
13
Thüringer Landessternwarte Tautenburg,
Sternwarte 5,
07778
Tautenburg, Germany
14
European Southern Observatory,
Alonso de Cordova
3107,
Vitacura, Santiago de Chile, Chile
15
Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University,
Ny Munkegade 120,
8000
Aarhus C, Denmark
16
Mullard Space Science Laboratory, University College London,
Holmbury St Mary, Dorking,
Surrey
RH5 6NT, UK
17
Astrobiology Research Unit, Université de Liège,
Allée du 6 Août 19C,
4000
Liège, Belgium
18
Department of Earth, Atmospheric and Planetary Science, Massachusetts Institute of Technology,
77 Massachusetts Avenue,
Cambridge, MA
02139, USA
19
Institut für Physik, Karl-Franzens Universität Graz,
Universitätsplatz 5/II, NAWI Graz,
8010
Graz, Austria
20
Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology,
Cambridge, MA
02139, USA
21
Carnegie Earth and Planets Laboratory,
5241 Broad Branch Road NW,
Washington, DC
20015, USA
22
American Association of Variable Star Observers,
49 Bay State Road,
Cambridge, MA
02138, USA
23
George Mason University,
4400 University Drive,
Fairfax, VA,
22030 USA
24
The Observatories of the Carnegie Institution for Science,
813 Santa Barbara St.,
Pasadena, CA
91101, USA
25
Division of Geological and Planetary Sciences,
1200 E California Blvd,
Pasadena, CA
91125, USA
26
El Sauce Observatory,
Coquimbo Province, Chile
27
Rheinisches Institut für Umweltforschung, Abt. Planetenforschung, an der Universität zu Köln,
Aachener Straße 209,
50931
Cologne, Germany
28
Astrobiology Center,
2-21-1 Osawa, Mitaka,
Tokyo
181-8588, Japan
29
National Astronomical Observatory of Japan,
2-21-1 Osawa, Mitaka,
Tokyo
181-8588, Japan
30
SUPA School of Physics & Astronomy, North Haugh, University of St Andrews,
St Andrews
KY16 9SS,
Scotland, UK
31
University of Southern Queensland, Centre for Astrophysics,
West Street,
Toowoomba, QLD
4350 Australia
32
NASA Ames Research Center,
Moffett Field, CA
94035, USA
33
Department of Physics and Astronomy, University of Louisville,
Louisville, KY
40292, USA
34
Department of Astronomy, The Graduate University for Advanced Studies (SOKENDAI),
2-21-1 Osawa, Mitaka,
Tokyo, Japan
35
Department of Astronomy & Astrophysics, University of Chicago,
Chicago, IL
60637, USA
36
Department of Space, Earth and Environment, Chalmers University of Technology,
Onsala Space Observatory,
439 92
Onsala, Sweden
37
Center for Data Intensive and Time Domain Astronomy, Department of Physics and Astronomy, Michigan State University,
East Lansing, MI
48824, USA
38
Royal Astronomical Society,
Burlington House, Piccadilly,
London
W1J 0BQ, UK
39
Department of Aeronautics and Astronautics, MIT,
77 Massachusetts Avenue,
Cambridge, MA
02139, USA
40
Department of Astronomy, University of Wisconsin-Madison,
475 N Charter St,
Madison, WI
53706, USA
41
Kotizarovci Observatory,
Sarsoni 90,
51216
Viskovo, Croatia
42
Hazelwood Observatory,
Australia
43
Perth Exoplanet Survey Telescope,
Perth, Western Australia
44
Department of Astronomy, Tsinghua University,
Beijing
100084, PR China
45
Department of Astrophysical Sciences, Princeton University,
Princeton, NJ
08544, USA
Received:
28
July
2022
Accepted:
2
May
2023
The TOI-1130 is a known planetary system around a K-dwarf consisting of a gas giant planet, TOI-1130 c on an 8.4-day orbit that is accompanied by an inner Neptune-sized planet, TOI-1130 b, with an orbital period of 4.1 days. We collected precise radial velocity (RV) measurements of TOI-1130 with the HARPS and PFS spectrographs as part of our ongoing RV follow-up program. We performed a photodynamical modeling of the HARPS and PFS RVs, along with transit photometry from the Transiting Exoplanet Survey Satellite (TESS) and the TESS Follow-up Observing Program (TFOP). We determined the planet masses and radii of TOI-1130 b and TOI-1130 c to be Mb = 19.28 ± 0.97M⊕ and Rb = 3.56 ± 0.13 R⊕, and Mc = 325.59 ± 5.59M⊕ and Rc = 13.32−1.41+1.55 R⊕, respectively. We have spectroscopically confirmed the existence of TOI-1130 b, which had previously only been validated. We find that the two planets have orbits with small eccentricities in a 2:1 resonant configuration. This is the first known system with a hot Jupiter and an inner lower mass planet locked in a mean-motion resonance. TOI-1130 belongs to the small, yet growing population of hot Jupiters with an inner low-mass planet that poses a challenge to the pathway scenario for hot Jupiter formation. We also detected a linear RV trend that is possibly due to the presence of an outer massive companion.
Key words: planetary systems / planets and satellites: individual: TOI-1130 / techniques: photometric / techniques: radial velocities
© The Authors 2023
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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