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 plus or minus 0.000025 days. From the transit light curve we determine that the radius of the planet is R sub(P) = 1.257 plus or minus 0.053 R sub(J). HAT-P-5b has a mass of M su...

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Veröffentlicht in:The Astrophysical journal 2007-12, Vol.671 (2), p.L173-L176
Hauptverfasser: 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
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Sprache:eng
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Zusammenfassung:We report the discovery of a planet transiting a moderately bright (V = 12.00) G star, with an orbital period of 2.788491 plus or minus 0.000025 days. From the transit light curve we determine that the radius of the planet is R sub(P) = 1.257 plus or minus 0.053 R sub(J). HAT-P-5b has a mass of M sub(P) = 1.06 plus or minus 0.11 M sub(J), similar to the average mass of previously known transiting exoplanets, and a density of [unk] = 0.66 plus or minus 0.11 g cm super(-3). We find that the center of transit is [unk] = 2.454, 241.77663 plus or minus 0.00022 days (HJD), and the total transit duration is 0.1217 plus or minus 0.0012 days.
ISSN:1538-4357
0004-637X
1538-4357
DOI:10.1086/525022