TOI-6695: A Pair of Near-resonant Massive Planets Observed with TESS from the WINE Survey*

Abstract We present the discovery and characterization of a pair of warm Jovian-mass exoplanets orbiting the Sun-like star TOI-6695, based on Transiting Exoplanet Survey Satellite (TESS) transits and precise radial velocity (RV) measurements obtained with FEROS, HARPS, CHIRON, CORALIE, and PFS. The transiting exoplanet TOI-6695b has an orbital period of ∼80.4 days, a radius of 0.85 R jup , and a mass of 0.21 M jup . The outer planet has a minimum mass of 1.45 M jup and an orbital period of about 242.4 days, confidently constrained by the Doppler time-series data. The TOI-6695 exoplanet system exhibits transit-timing variations due to the dynamical interaction of the planets, which reside near a 3:1 mean-motion resonance. We modeled the TOI-6695 system’s orbital and dynamical configuration by performing self-consistent N -body fits of TESS photometry, ground-based photometry from Observatoire Moana, and precise RV data, all of which are consistent with the presence of a warm Jovian-mass duo of exoplanets.

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Publication Details

Journal
The Astronomical Journal
Published
2025-05-08
DOI
https://doi.org/10.3847/1538-3881/adc44e
Citations
1
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
1.15
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article

TOI-6695: A Pair of Near-resonant Massive Planets Observed with TESS from the WINE Survey*

F. Bouchy, J. McCormac, Jon M. Jenkins, Jan Eberhardt et al.
1 citations
The Astronomical Journal
Stellar, planetary, and galactic studies
1.15
article

TOI-6695: A Pair of Near-resonant Massive Planets Observed with TESS from the WINE Survey*

F. Bouchy, J. McCormac, Jon M. Jenkins, Jan Eberhardt, Marcelo Tala Pinto, Martin Schlecker, Soléne Ulmer-Moll, M. Lendl, D. Gandolfi, Rafael Brahm, Diana Dragomir, Arvind F. Gupta, Stephen A. Shectman, Sara Seager, N. Dunckel, Gavin Boyle, Jeffrey D. Crane, Johanna Teske, Néstor Espinoza, Rodrigo Leiva, G. Ricker, Andrés Jordán, D. J. Osip, Remo Burn, L. Acuña, Trifon Trifonov, Thomas Henning, Mélissa J. Hobson, Felipe Rojas, M. I. Jones, Joshua N. Winn
article en
1 citations

Abstract

Abstract We present the discovery and characterization of a pair of warm Jovian-mass exoplanets orbiting the Sun-like star TOI-6695, based on Transiting Exoplanet Survey Satellite (TESS) transits and precise radial velocity (RV) measurements obtained with FEROS, HARPS, CHIRON, CORALIE, and PFS. The transiting exoplanet TOI-6695b has an orbital period of ∼80.4 days, a radius of 0.85 R jup , and a mass of 0.21 M jup . The outer planet has a minimum mass of 1.45 M jup and an orbital period of about 242.4 days, confidently constrained by the Doppler time-series data. The TOI-6695 exoplanet system exhibits transit-timing variations due to the dynamical interaction of the planets, which reside near a 3:1 mean-motion resonance. We modeled the TOI-6695 system’s orbital and dynamical configuration by performing self-consistent N -body fits of TESS photometry, ground-based photometry from Observatoire Moana, and precise RV data, all of which are consistent with the presence of a warm Jovian-mass duo of exoplanets.

The Astronomical JournalVol. 169(6)
Openalex Percentile: Top 19%
Stellar, planetary, and galactic studies
1.15
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