TOI-1130: A photodynamical analysis of a hot Jupiter in resonance with an inner low-mass planet
Artikel i vetenskaplig tidskrift, 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.
Planetary systems
Techniques: radial velocities
Planets and satellites: individual: TOI-1130
Techniques: photometric
Författare
Judith Korth
Lunds universitet
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
D. Gandolfi
Universita degli Studi di Torino
J. Šubjak
Univerzita Karlova
European Southern Observatory (ESO)
Czech Academy of Sciences
Harvard-Smithsonian Center for Astrophysics
S. Howard
Observatoire de la Cote d'Azur
S. Ataiee
Ferdowsi University of Mashhad
Karen A. Collins
Harvard-Smithsonian Center for Astrophysics
Samuel N. Quinn
Harvard-Smithsonian Center for Astrophysics
A. J. Mustill
Lunds universitet
T. Guillot
Observatoire de la Cote d'Azur
N. Lodieu
Instituto de Astrofísica de Canarias
Universidad de la Laguna
A. M.S. Smith
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
M. Esposito
Thüringer Landessternwarte Tautenburg
F. Rodler
European Southern Observatory Santiago
Alexandra Muresan
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
L. Abe
Observatoire de la Cote d'Azur
Simon Albrecht
Aarhus Universitet
A. Alqasim
University College London (UCL)
Khalid Barkaoui
Universite de Liège
Massachusetts Institute of Technology (MIT)
Instituto de Astrofísica de Canarias
P. G. Beck
Instituto de Astrofísica de Canarias
Karl-Franzens-Universität Graz
Christopher J. Burke
Massachusetts Institute of Technology (MIT)
R.P. Butler
Carnegie Observatories
D. Conti
American Association of Variable Star Observers
Kevin I. Collins
George Mason University
J.D. Crane
Carnegie Observatories
F. Dai
California Institute of Technology (Caltech)
H. Deeg
Universidad de la Laguna
Instituto de Astrofísica de Canarias
P. Evans
El Sauce Observatory
S. Grziwa
Universität zu Köln
A. Hatzes
Thüringer Landessternwarte Tautenburg
T. Hirano
National Astronomical Observatory of Japan
National Institutes of Natural Sciences
Keith Horne
University of St Andrews
Chelsea X. Huang
University of Southern Queensland
Jon M. Jenkins
National Aeronautics and Space Administration (NASA)
Petr Kabath
Czech Academy of Sciences
J. F. Kielkopf
University of Louisville
E. Knudstrup
Aarhus Universitet
D. W. Latham
Harvard-Smithsonian Center for Astrophysics
J.H. Livingston
National Astronomical Observatory of Japan
The Graduate University for Advanced Studies (SOKENDAI)
National Institutes of Natural Sciences
R. Luque
University of Chicago
S. Mathur
Universidad de la Laguna
Instituto de Astrofísica de Canarias
F. Murgas
Instituto de Astrofísica de Canarias
Universidad de la Laguna
H. L.M. Osborne
University College London (UCL)
Enric Palle
Universidad de la Laguna
Instituto de Astrofísica de Canarias
Carina Persson
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Joseph E. Rodriguez
Michigan State University
Mark E. Rose
National Aeronautics and Space Administration (NASA)
Pamela Rowden
Royal Astronomical Society
R. Schwarz
Harvard-Smithsonian Center for Astrophysics
S. Seager
Massachusetts Institute of Technology (MIT)
L. M. Serrano
Universita degli Studi di Torino
Lizhou Sha
University of Wisconsin Madison
S.A. Shectman
Carnegie Observatories
Avi Shporer
Massachusetts Institute of Technology (MIT)
G. Srdoc
Kotizarovci Observatory
C. Stockdale
Hazelwood Observatory
Thiam Guan Tan
Perth Exoplanet Survey Telescope
J. K. Teske
Carnegie Observatories
Vincent Van Eylen
University College London (UCL)
A. Vanderburg
Massachusetts Institute of Technology (MIT)
Roland K. Vanderspek
Massachusetts Institute of Technology (MIT)
S. Wangm
Tsinghua University
J. N. Winn
Princeton University
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 675 A115Jämställdhet för excellens (Genie)
Stiftelsen Chalmers tekniska högskola, 2019-01-01 -- 2028-12-31.
Exoplaneter från rymden - CHEOPS och PLATO, ESA's nästa två rymdteleskop (fas 2)
Rymdstyrelsen (65/19), 2020-01-01 -- 2022-12-31.
Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/202244617