@article{article_1307803, title={Updated Orbital Decay Rate of WASP-12 with New Data from TESS and Ground-based Observations}, journal={Turkish Journal of Astronomy and Astrophysics}, volume={4}, pages={10–22}, year={2023}, DOI={10.55064/tjaa.1307803}, author={Kutluay, Ahmet Cem and Basturk, Ozgur and Yalçınkaya, Selçuk and Saguner Rambaldi, Tenay and Yerli, Sinan Kaan}, keywords={orbital decay, methods: data analysis, techniques: photometric, stars: individual: WASP-12, planetary systems}, abstract={We investigate the orbital decay behavior of the well-studied hot Jupiter WASP-12\,b orbiting its late-F host star on a 1.09-day orbit by analyzing its transit timings. Thanks to precise photometric data covering nearly 15 years of observations from the space and the ground since the discovery of the planet, including a transit light curve of our own, it became possible to study this behaviour in its details. This work updates the orbital period to a new value of $P = 1.0914202527 \pm 0.000000039\,\text{days}$ and agrees with the previous finding that the planetary orbit has been shrinking with an updated rate of $-31.03 \pm 0.94\,\text{ms yr}^{-1}$. This corresponds to an orbital decay timescale of $\tau =P/|\dot{P}| = 3.04 \pm 0.09\,\text{Myr}$ that we attribute to the strong tidal interactions between the host-star and the planet. We also update the reduced stellar tidal quality factor as $Q_{*}^{\prime} = (1.72 \pm 0.39) \times$ $10^{5}$, which corresponds to the lower bound of the previously reported values of the parameter.}, number={2}, publisher={Türk Astronomi Derneği}