Decaying orbit of the hot Jupiter WASP-12b confirmation with TESS observations. (2021)
Keywords :
Exoplanets ; Exoplanet dynamics ; Exoplanet astronomy ; Exoplanet tides
Abstract:Theory suggests that the orbits of some close-in giant planets should decay due to tidal interactions with their host stars. To date, WASP-12b is the only hot Jupiter reported to have a decaying orbit, at a rate of 29{+/-}2ms/yr. We analyzed data from NASA's Transiting Exoplanet Survey Satellite (TESS) to verify that WASP-12b's orbit is indeed changing. We find that the TESS transit and occultation data are consistent with a decaying orbit with an updated period of 1.091420090{+/-}0.000000041days and a decay rate of 32.53{+/-}1.62ms/yr. We find an orbital decay timescale of {tau}=P/|P|=2.90{+/-}0.14Myr. If the observed decay results from tidal dissipation, the modified tidal quality factor is
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Transiting Exoplanet Survey Satellite (TESS) observed WASP-12b in
Sector 20 (2019 December 24 through 2020 January 20). These
observations were processed by the Science Processing Operations
Center (SPOC) pipeline. All of the SPOC data products are publicly
accessible from the Mikulski Archive for Space Telescopes (MAST;
http://archive.stsci.edu/).
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