Planck-cmb-allsky

HAT-P-5b: A Jupiter-like Hot Jupiter Transiting a Bright Star

December 2007 • 2007ApJ...671L.173B

Authors • Bakos, G. Á. • Shporer, A. • Pál, A. • Torres, G. • Kovács, Géza • Latham, D. W. • Mazeh, T. • Ofir, A. • Noyes, R. W. • Sasselov, D. D. • Bouchy, F. • Pont, F. • Queloz, D. • Udry, S. • Esquerdo, G. • Sipőcz, B. • Kovács, Gábor • Stefanik, R. • Lázár, J. • Papp, I. • Sári, P.

Abstract • We report the discovery of a planet transiting a moderately bright (V=12.00) G star, with an orbital period of 2.788491+/-0.000025 days. From the transit light curve we determine that the radius of the planet is Rp=1.257+/-0.053 RJ. HAT-P-5b has a mass of Mp=1.06+/-0.11 MJ, similar to the average mass of previously known transiting exoplanets, and a density of ρp=0.66+/-0.11 g cm-3. We find that the center of transit is Tc=2,454,241.77663+/-0.00022 days (HJD), and the total transit duration is 0.1217+/-0.0012 days.

Based in part on observations obtained with the SOPHIE spectrograph mounted on the 1.93 m telescope at the Haute Provance Observatory.

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Brigitta Sipőcz

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