Tentative Evidence for Transit Timing Variations of WASP-161b
Fan Yang, Ranga-Ram Chary

TL;DR
This paper presents evidence of transit timing variations in WASP-161b using TESS, archival, and CHEOPS data, suggesting a possible changing orbital period or precession, with implications for understanding the planet's dynamics.
Contribution
It provides the first detection of TTVs in WASP-161b and models potential causes, including a quadratic period change and precession, using combined observational data.
Findings
Detected significant TTVs in WASP-161b with up to 203-minute offsets.
Modeled TTVs with a quadratic function indicating a period change.
Predicted a 5-minute timing variation in upcoming CHEOPS observations.
Abstract
We report on the detection of transit timing variations (TTV) of WASP-161b by using the combination of TESS data and archival data. The midpoint of the transits in TESS data are offset by 67 minutes in Jan. 2019, and 203 minutes in Jan. 2021, based on the ephemeris published in previous work. We are able to reproduce the transit timings from the archival light curve (SSO-Europa; Jan. 2018) and find SSO-Europa timing is consistent with the published ephemeris under a constant period assumption. Conversely, we find that the SSO-Europa transit midpoint indicates a 6.62-minute variation at 4.40 compared to the prediction obtained from TESS timings, and a constant orbit period assumption. The TTVs could be modeled with a quadratic function, yielding a constant period change. The period derivative is -1.16102.2510 days per day…
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Stellar, planetary, and galactic studies · Geophysics and Gravity Measurements
