Phase curve and variability analysis of WASP-12b using TESS photometry
arXiv:2102.00052 · doi:10.1093/mnrasl/slab014
Abstract
We analyse Sector 20 TESS photometry of the ultra-hot Jupiter WASP-12b, and extract its phase curve to study the planet's atmospheric properties. We successfully recover the phase curve with an amplitude of 549 62 ppm, and a secondary eclipse depth of 609 ppm. The peak of the phase curve is shifted by 0.049 0.015 in phase, implying that the brightest spot in the atmosphere is shifted from the substellar point towards the planet's evening terminator. Assuming zero albedo, the eclipse depth infers a day-side brightness temperature of 3128 K. No significant detection of flux from the night-side is found at 60 97 ppm, implying a night-side brightness temperature of 2529 K (1-). We do not detect any significant variability in the light from the planet over the 27 days of the TESS observations. Finally, we note that an ephemeris model taking orbital decay into account provides a significantly better fit than a constant-period model.
arXiv comment11 pages, 5 figures. Accepted for publication in MNRAS Letters
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