The sub-Saturn Mass Transiting Planet HAT-P-12b
arXiv:1201.6419 · doi:10.1088/0004-6256/143/4/95
Abstract
We present new photometric data of the transiting planet HAT-P-12b observed in 2011. Our three transit curves are modelled using the JKTEBOP code and adopting the quadratic limb-darkening law. Including our measurements, 18 transit times spanning about 4.2 yr were used to determine the improved ephemeris with a transit epoch of 2,454,187.855600.00011 BJD and an orbital period of 3.213059610.00000035 d. The physical properties of the star-planet system are computed using empirical calibrations from eclipsing binary stars and stellar evolutionary models, combined with both our transit parameters and previously-known spectroscopic results. We found that the absolute dimensions of the host star are =0.730.02 M, =0.700.01 R, log =4.610.02, =2.100.09 , and =0.210.01 L. The planetary companion has =0.210.01 M, =0.940.01 R, log =2.770.02, =0.240.01 , and =96014 K. Our results agree well with standard models of irradiated gas giants with a core mass of 11.3 M.
17 pages, including 5 figures and 5 tables, accepted for publication in AJ
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