TOI-1408: Discovery and Photodynamical Modeling of a Small Inner Companion to a Hot Jupiter Revealed by Transit Timing Variations
Artikel i vetenskaplig tidskrift, 2024
We report the discovery and characterization of a small planet, TOI-1408 c, on a 2.2 day orbit located interior to a previously known hot Jupiter, TOI-1408 b (P = 4.42 days, M = 1.86 ± 0.02 M Jup, R = 2.4 ± 0.5 R Jup) that exhibits grazing transits. The two planets are near 2:1 period commensurability, resulting in significant transit timing variations (TTVs) for both planets and transit duration variations for the inner planet. The TTV amplitude for TOI-1408 c is 15% of the planet’s orbital period, marking the largest TTV amplitude relative to the orbital period measured to date. Photodynamical modeling of ground-based radial velocity (RV) observations and transit light curves obtained with the Transiting Exoplanet Survey Satellite and ground-based facilities leads to an inner planet radius of 2.22 ± 0.06 R ⊕ and mass of 7.6 ± 0.2 M ⊕ that locates the planet into the sub-Neptune regime. The proximity to the 2:1 period commensurability leads to the libration of the resonant argument of the inner planet. The RV measurements support the existence of a third body with an orbital period of several thousand days. This discovery places the system among the rare systems featuring a hot Jupiter accompanied by an inner low-mass planet.
Författare
Judith Korth
Lunds universitet
Priyanka Chaturvedi
Tata Institute of Fundamental Research
Thüringer Landessternwarte Tautenburg
H. Parviainen
Instituto de Astrofísica de Canarias
Universidad de la Laguna
Ilaria Carleo
Instituto de Astrofísica de Canarias
Istituto nazionale di astrofisica (INAF)
Universidad de la Laguna
Michael Endl
The University of Texas at Austin
College of Natural Sciences
E. W. Guenther
Thüringer Landessternwarte Tautenburg
G. Nowak
Instituto de Astrofísica de Canarias
Universidad de la Laguna
Uniwersytet Mikolaja Kopernika
Carina Persson
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
P. MacQueen
College of Natural Sciences
A. J. Mustill
Lunds universitet
J. Cabrera
Deutsches Zentrums für Luft- und Raumfahrt (DLR)
William D. Cochran
The University of Texas at Austin
College of Natural Sciences
J. Lillo-Box
Centro de Astrobiologia (CAB)
D. Hobbs
Lunds universitet
F. Murgas
Universidad de la Laguna
Instituto de Astrofísica de Canarias
Michael Greklek-McKeon
California Institute of Technology (Caltech)
Hanna Kellermann
Ludwig-Maximilians-Universität München (LMU)
G. Hebrard
Centre national de la recherche scientifique (CNRS)
Institut d 'Astrophysique de Paris
A. Fukui
University of Tokyo
Instituto de Astrofísica de Canarias
Enric Palle
Universidad de la Laguna
Instituto de Astrofísica de Canarias
Jon M. Jenkins
National Aeronautics and Space Administration (NASA)
J. D. Twicken
SETI Institute
National Aeronautics and Space Administration (NASA)
Karen A. Collins
Harvard-Smithsonian Center for Astrophysics
Samuel N. Quinn
Harvard-Smithsonian Center for Astrophysics
J. Šubjak
Czech Academy of Sciences
Harvard-Smithsonian Center for Astrophysics
P. G. Beck
Universidad de la Laguna
Instituto de Astrofísica de Canarias
D. Gandolfi
Universita degli Studi di Torino
S. Mathur
Universidad de la Laguna
Instituto de Astrofísica de Canarias
H. Deeg
Universidad de la Laguna
Instituto de Astrofísica de Canarias
D. W. Latham
Harvard-Smithsonian Center for Astrophysics
Simon Albrecht
Aarhus Universitet
D. Barrado
Centro de Astrobiologia (CAB)
I. Boisse
Centre national de la recherche scientifique (CNRS)
Laboratoire d'Astrophysique de Marseille
Hervé Bouy
Laboratoire d'Astrophysique de Bordeaux
Institut Universitaire de France
X. Delfosse
Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
O. Demangeon
Universidade do Porto
R. A. García
Université Paris-Saclay
A. Hatzes
Thüringer Landessternwarte Tautenburg
N. Heidari
Institut d 'Astrophysique de Paris
Kai Ikuta
University of Tokyo
Petr Kabath
Czech Academy of Sciences
H. Knutson
California Institute of Technology (Caltech)
J.H. Livingston
National Institutes of Natural Sciences
The Graduate University for Advanced Studies (SOKENDAI)
National Astronomical Observatory of Japan
E. Martioli
Institut d 'Astrophysique de Paris
Laboratorio Nacional de Astrofisica, Itajuba
M. Morales-Calderon
Centro de Astrobiologia (CAB)
Giuseppe Morello
Instituto de Astrofísica de Canarias
Consejo Superior de Investigaciones Científicas (CSIC)
Norio Narita
University of Tokyo
National Institutes of Natural Sciences
Instituto de Astrofísica de Canarias
J. Orell-Miquel
Instituto de Astrofísica de Canarias
Universidad de la Laguna
H. L.M. Osborne
European Southern Observatory (ESO)
University College London (UCL)
Dinil B. Palakkatharappil
Université Paris-Saclay
Viktoria Pinter
Nordic Optical Telescope
University of Craiova
S. Redfield
Wesleyan University
Howard M. Relles
Harvard-Smithsonian Center for Astrophysics
R. Schwarz
Harvard-Smithsonian Center for Astrophysics
S. Seager
Massachusetts Institute of Technology (MIT)
Avi Shporer
Massachusetts Institute of Technology (MIT)
Marek Skarka
Masarykova Univerzita
Czech Academy of Sciences
G. Srdoc
Kotizarovci Observatory
M. Stangret
Istituto nazionale di astrofisica (INAF)
Luis Thomas
Ludwig-Maximilians-Universität München (LMU)
Max-Planck-Gesellschaft
Vincent Van Eylen
University College London (UCL)
Noriharu Watanabe
University of Tokyo
J. N. Winn
Princeton University
Astrophysical Journal Letters
2041-8205 (ISSN) 2041-8213 (eISSN)
Vol. 971 2 L28Exoplaneter från rymden - CHEOPS och PLATO, ESA's nästa två rymdteleskop (fas 2)
Rymdstyrelsen (65/19), 2020-01-01 -- 2022-12-31.
Rymdstyrelsen (177/19), 2020-01-01 -- 2022-12-31.
Jämställdhet för excellens (Genie)
Stiftelsen Chalmers tekniska högskola, 2019-01-01 -- 2028-12-31.
Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
DOI
10.3847/2041-8213/ad65fd