Article (Scientific journals)
Evidence for transit-timing variations of the 11 Myr exoplanet TOI-1227 b
Almenara, J. M.; Bonfils, X.; Guillot, T. et al.
2024In Astronomy and Astrophysics, 683, p. 96
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Keywords :
techniques: photometric; stars: individual: TOI-1227; planetary systems
Abstract :
[en] TOI-1227 b is an 11 Myr old validated transiting planet in the middle of its contraction phase, with a current radius of 0.85 Rj. It orbits a low-mass pre-main sequence star (0.170 M⊙, 0.56 R⊙) every 27.4 days. The magnetic activity of its young host star induces radial velocity jitter and prevents good measurements of the planetary mass. We gathered additional transit observations of TOI-1227 b with space- and ground-based telescopes, and we detected highly significant transit-timing variations (TTVs). Their amplitude is about 40 min and their dominant timescale is longer than 3.7 yr. Their most probable origin is dynamical interactions with additional planets in the system. We modeled the TTVs with inner and outer perturbers near first and second order resonances; several orbital configurations provide an acceptable fit. More data are needed to determine the actual orbital configuration and eventually measure the planetary masses. These TTVs and an updated transit chromaticity analysis reinforce the evidence that TOI-1227 b is a planet.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Almenara, J. M.;  University of Geneva, Astronomical Observatory, Institute de Planetologie et d'Astrophysique de Grenoble
Bonfils, X.;  Institute de Planetologie et d'Astrophysique de Grenoble
Guillot, T.;  Observatoire de la Cote d'Azur, France
Timmermans, Mathilde  ;  Université de Liège - ULiège > Astrobiology
Díaz, R. F.;  National University of San Martin, Argentina
Venturini, J.;  University of Geneva, Astronomical Observatory
Petit, A. C.;  Observatoire de la Cote d'Azur, France
Forveille, T.;  Institute de Planetologie et d'Astrophysique de Grenoble
Suárez, O.;  Observatoire de la Cote d'Azur, France
Mékarnia, D.;  Observatoire de la Cote d'Azur, France
Triaud, A. H. M. J.;  University of Birmingham, School of Physics and Astronomy
Abe, L.;  Observatoire de la Cote d'Azur, France
Bendjoya, P.;  Observatoire de la Cote d'Azur, France
Bouchy, F.;  University of Geneva, Astronomical Observatory
Bouvier, J.;  Institute de Planetologie et d'Astrophysique de Grenoble
Delrez, Laetitia ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Exoplanets in Transit: Identification and Characterization
Dransfield, G.;  University of Birmingham, School of Physics and Astronomy
Ducrot, E.;  CEA Saclay, Service d'Astrophysique
Gillon, Michaël  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO)
Hooton, M. J.;  University of Cambridge, Institute of Astronomy
Jehin, Emmanuel  ;  Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
Mann, A. W.;  University of North Carolina, Department of Physics and Astronomy
Mardling, R.;  Monash University, School of Physics, University of Geneva, Astronomical Observatory
Murgas, F.;  Astrophysical Institute of the Canaries, University of La Laguna, Department of Astrophysics
Leleu, A.;  University of Geneva, Astronomical Observatory
Lendl, M.;  University of Geneva, Astronomical Observatory
Queloz, D.;  University of Cambridge, Institute of Astronomy
Seager, S.;  MIT, Center for Space Research/Kavli Institute, MIT, Department of Earth and Planetary Science, Massachusetts Institute of Technology
Winn, J.;  Princeton University, Department of Astrophysical Sciences
Fernández, S. Zuñiga;  University of Liege, Belgium
More authors (20 more) Less
Language :
English
Title :
Evidence for transit-timing variations of the 11 Myr exoplanet TOI-1227 b
Publication date :
01 March 2024
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences, Les Ulis, Fr
Volume :
683
Pages :
A96
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 19 March 2024

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