Doomed Worlds II: Reassessing Suggestions of Orbital Decay for TrES-5 b
Marvin Rothmeier, Elisabeth R. Adams, Karsten Schindler, Andre Beck, Brian Jackson, Jeffrey P. Morgenthaler, Amanda A. Sickafoose, Malia Barker, Luigi Mancini, John Southworth, Daniel Evans, and Alfred Krabbe

TL;DR
This study reanalyzed transit data for TrES-5b, finding no strong evidence of orbital decay and suggesting previous claims were likely due to data artifacts or outliers.
Contribution
It provides a comprehensive reexamination with new data, demonstrating that the orbital decay hypothesis for TrES-5b is not supported by current observations.
Findings
Revised period change rate is less than half of previous estimates.
The quadratic model preference has decreased over time.
Removing a single outlier negates the decay evidence.
Abstract
TrES-5b is one of only three ultra-hot Jupiters (UHJs) with suggestions of a possibly decreasing orbital period that have persisted through multiple independent analyses (G. Maciejewski et al. 2021; S. R. Hagey et al. 2022; E. S. Ivshina & J. N. Winn 2022; W. Wang et al. 2024; L. C. Yeh et al. 2024). While WASP-12 b's decreasing period is well-explained by tidally induced orbital decay (K. C. Patra et al. 2017), and stellar acceleration has been proposed for WASP-4 b (L. G. Bouma et al. 2020), the cause of the apparent trend for TrES-5 b has not been satisfactorily explained. This work extends the previous observations with 14 new ground-based transits from 2016-2024 and two newly-published midtimes for data from 2007 and 2009. Four TESS sectors (75, 77, 82, and 84) have also been included for the first time. With the new data, the case for a decreasing orbital period is much weaker…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astro and Planetary Science · Astronomy and Astrophysical Research
