Exoplanets & Exomoons

Metrics For Optimizing Searches For Tidally Decaying Exoplanets

By Keith Cowing
Status Report
astro-ph.EP
August 9, 2023
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Metrics For Optimizing Searches For Tidally Decaying Exoplanets
(top) The blue dots show the evolution of σt pred tra for WASP-12 b during the last several years, as calculated using the data from Yee et al. (2020) and Equation 14. The orange curve (which uses the right y-axis) illustrates the corresponding evolution of the difference in Bayesian Information Criterion (BIC) comparing a linear ephemeris BIC(lin) to a quadratic ephemeris BIC(quad). (bottom) The blue dots show the difference between the observed transit time t(E) at epoch E and a linear ephemeris fit T0 + P E. The orange line shows the quadratic ephemeris term using the dP/dE (86.7 µs orbit−1 ) from Yee et al. (2020). — astro-ph.EP

Tidal interactions between short-period exoplanets and their host stars drive orbital decay and have likely led to engulfment of planets by their stars.

Precise transit timing surveys, with baselines now spanning decades for some planets, are directly detecting orbital decay for a handful of planets, with corroboration for planetary engulfment coming from independent lines of evidence. More than that, recent observations have perhaps even caught the moment of engulfment for one unfortunate planet.

These portentous signs bolster prospects for ongoing surveys, but optimizing such a survey requires considering the astrophysical parameters that give rise to robust timing constraints and large tidal decay rates, as well as how best to schedule observations conducted over many years. The large number of possible targets means it is not feasible to continually observe all planets that might exhibit detectable tidal decay. In this study, we explore astrophysical and observational properties for a short-period exoplanet system that can maximize the likelihood for observing tidally driven transit-timing variations.

We consider several fiducial observational strategies and real exoplanet systems reported to exhibit decay. We show that moderately frequent (a few transits per year) observations may suffice to detect tidal decay within just a few years. Tidally driven timing variations take time to grow to detectable levels, and so we estimate how long that growth takes as a function of timing uncertainties and tidal decay rate and provide thresholds for deciding that tidal decay has been detected.

Brian Jackson, Elisabeth R. Adams, Jeffrey P. Morgenthaler

Comments: Accepted to AJ; 17 pages, 8 figures
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2308.04587 [astro-ph.EP] (or arXiv:2308.04587v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2308.04587
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Submission history
From: Brian Jackson
[v1] Tue, 8 Aug 2023 21:15:22 UTC (2,767 KB)
https://arxiv.org/abs/2308.04587
Astrobiology

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻