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

Autor:	Tsevi Mazeh, Gáspár Á. Bakos, Robert W. Noyes, François Bouchy, Stéphane Udry, Guillermo Torres, Dimitar Sasselov, I. Papp, D. Queloz, D. W. Latham, Gábor L. Kovács, Pál Sári, András Pál, Aviv Ofir, Frederic Pont, J. Lazar, Géza Kovács, Brigitta Sipocz, Avi Shporer, Gil Esquerdo
Rok vydání:	2007
Předmět:	Physics Astrophysics (astro-ph) FOS: Physical sciences Astronomy and Astrophysics Radius Astrophysics Orbital period Light curve Exoplanet Jupiter Space and Planetary Science Planet Hot Jupiter Transit (astronomy)
Zdroj:	The Astrophysical Journal. 671:L173-L176
ISSN:	1538-4357 0004-637X
Popis:	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 RJup. HAT-P-5b has a mass of Mp = 1.06 +/- 0.11 MJup, similar to the average mass of previously-known transiting exoplanets, and a density of rho = 0.66 +/- 0.11 g cm^-3 . We find that the center of transit is Tc = 2,454,241.77663 +/- 0.00022 (HJD), and the total transit duration is 0.1217 +/- 0.0012 days. 5 pages, submitted to APJL
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0dd98eb457d775270926a1bde2c4afb https://doi.org/10.1086/525022 Zobrazit plný text záznamu