Passer à la navigation principale Passer à la recherche Passer au contenu principal

Photodynamical analysis of the nearly resonant planetary system WASP-148: Accurate transit-timing variations and mutual orbital inclination

  • J. M. Almenara
  • , G. Hébrard
  • , R. F. Díaz
  • , J. Laskar
  • , A. C.M. Correia
  • , D. R. Anderson
  • , I. Boisse
  • , X. Bonfils
  • , D. J.A. Brown
  • , V. Casanova
  • , A. Collier Cameron
  • , M. Fernández
  • , J. M. Jenkins
  • , F. Kiefer
  • , A. Lecavelier Des Etangs
  • , J. J. Lissauer
  • , G. MacIejewski
  • , J. McCormac
  • , H. Osborn
  • , D. Pollacco
  • G. Ricker, J. Sánchez, S. Seager, S. Udry, D. Verilhac, J. Winn
  • Université de Genève
  • LTHE (UMR 5564 CNRS/IRD/Université de Grenoble)
  • Institut d’Astrophysique de Paris
  • Observatoire de Haute-Provence
  • Instituto de Tecnologías en Detección y Astropartículas (CNEACONICET-UNSAM)
  • Sorbonne Univ.
  • University of Coimbra
  • University of Warwick
  • University of Warwick
  • Keele University
  • LAM
  • Instituto de Astrofísica de Andalucía-CSIC
  • University of St Andrews
  • NASA Ames Research Center
  • Nicolaus Copernicus University
  • University of Bern
  • Massachusetts Institute of Technology
  • Massachusetts Institute of Technology
  • Massachusetts Institute of Technology
  • Observatoire Hubert-Reeves
  • Princeton University

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

12 Citations (Scopus)

Résumé

WASP-148 is a recently announced extra-solar system harbouring at least two giant planets. The inner planet transits its host star. The planets travel on eccentric orbits and are near the 4:1 mean-motion resonance, which implies significant mutual gravitational interactions. In particular, this causes transit-timing variations of a few minutes, which were detected based on ground-based photometry. This made WASP-148 one of the few cases where such a phenomenon was detected without space-based photometry. Here, we present a self-consistent model of WASP-148 that takes into account the gravitational interactions between all known bodies in the system. Our analysis simultaneously fits the available radial velocities and transit light curves. In particular, we used the photometry secured by the Transiting Exoplanet Survey Satellite (TESS) and made public after the WASP-148 discovery announcement. The TESS data confirm the transit-timing variations, but only in combination with previously measured transit times. The system parameters we derived agree with those previously reported and have a significantly improved precision, including the mass of the non-transiting planet. We found a significant mutual inclination between the orbital planes of the two planets: I = 41.0+6.2 -7.6 based on the modelling of the observations, although we found I = 20.8 ± 4.6 when we imposed a constraint on the model enforcing long-term dynamical stability. When a third planet was added to the model - based on a candidate signal in the radial velocity - the mutual inclination between planets b and c changed significantly allowing solutions closer to coplanar. We conclude that more data are needed to establish the true architecture of the system. If the significant mutual inclination is confirmed, WASP-148 would become one of the only few candidate non-coplanar planetary systems. We discuss possible origins for this misalignment.

langue originaleAnglais
Numéro d'articleA134
journalAstronomy and Astrophysics
Volume663
Les DOIs
étatPublié - 1 juil. 2022
Modification externeOui

Empreinte digitale

Examiner les sujets de recherche de « Photodynamical analysis of the nearly resonant planetary system WASP-148: Accurate transit-timing variations and mutual orbital inclination ». Ensemble, ils forment une empreinte digitale unique.

Contient cette citation