论文信息 - HAT-P-5b: A Jupiter-like Hot Jupiter Transiting a Bright Star - 字舞流文

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

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.

D. Queloz | Geza Kovacs | S. Udry | A. Ofir | F. Pont | Harvard-Smithsonian Center for Astrophysics | D. W. Latham | A. Pal | F. Bouchy | R. W. Noyes | B. Sipocz | E. University | B. Sipocz | Avi Shporer | F. Bouchy | S. Udry | T. Mazeh | D. Latham | D. Sasselov | G. Torres | A. Ofir | G. Esquerdo | D. Queloz | A. Pál | F. Pont | R. Noyes | G. Kovacs | G. Bakos | J. Lázár | Gabor Kovacs | G. A. Bakos | G. Torres | D. D. Sasselov | J. Lazar | I. Papp | P. Sári | A. Shporer | I. Papp | T. Mazeh | Eotvos Lor'and University | P. Sari | G. Esquerdo | Hubble Fellow. Wise Observatory | Tel Aviv University Department of Astronomy | Budapest Konkoly Observatory | Budapest Observatoire Astronomique de l'Universite de Geneve | Institut d'Astrophysique de Paris Hungarian Astronomical Association | H. C. F. Astrophysics | G. Kovacs | Tel A Astronomy

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