Year: 2025
Type: preprint
Abstract: The Roman Space Telescope Galactic Bulge Time Domain Survey (GBTDS) is expected to detect ~$10^5$ transiting planets. Many of these planets will have short orbital periods and are thus susceptible to tidal decay. We use a catalog of simulated transiting planet detections to predict the yield of orbital decay detections in the Roman GBTDS. Assuming a constant stellar tidal dissipation factor, $Q^{'}_{*}$, of $10^6$, we predict ~ 5 - 10 detections. We additionally consider an empirical period-dependent parameterization of $Q^{'}_{*} \propto P^{-3}$ and find a substantially suppressed yield. We conclude that Roman will provide constraints on the rate of planet engulfment in the Galaxy and probe the physics of tidal dissipation in stars.
Source: arXiv (Cornell University)
Authors: Carden, Kylee, Gaudi, B. Scott, Wilson, Robert F.
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Awards: G3782671888, G4266415239, G6561015458
OpenAlex ID: W6979262005
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