Prospects from TESS and Gaia to constrain the flatness of planetary systems
Juan I. Espinoza-Retamal, Wei Zhu, Cristobal Petrovich

TL;DR
This study explores how Gaia astrometry can detect and characterize cold Jupiters in systems with TESS planets, helping to understand their formation by measuring mutual inclinations.
Contribution
It demonstrates the potential of Gaia to detect and measure the inclinations of cold Jupiters in TESS systems, providing new insights into planetary system dynamics.
Findings
Gaia can detect ~200 cold Jupiters in TESS systems during its 5-year mission.
Orbital inclinations can be measured with a precision of σ_{cos i}<0.2 in about 120 systems.
Gaia data can distinguish between dynamically cold and hot planetary systems based on mutual inclinations.
Abstract
The mutual inclination between planets orbiting the same star provides key information to understand the formation and evolution of multi-planet systems. In this work, we investigate the potential of Gaia astrometry in detecting and characterizing cold Jupiters in orbits exterior to the currently known TESS planet candidates. According to our simulations, out of the systems expected to have cold Jupiter companions, Gaia, by its nominal 5-year mission, should be able to detect cold Jupiters and measure the orbital inclinations with a precision of in of them. These numbers are estimated under the assumption that the orbital orientations of the CJs follow an isotropic distribution, but these only vary slightly for less broad distributions. We also discuss the prospects from radial velocity follow-ups to better constrain the derived…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Scientific Research and Discoveries
