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25 April 2024
 
  » arxiv » 1106.5510

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Kepler-14b: A massive hot Jupiter transiting an F star in a close visual binary
Lars A. Buchhave ; David W. Latham ; Joshua A. Carter ; Jean-Michel Désert ; Guillermo Torres ; Elisabeth R. Adams ; Stephen T. Bryson ; David B. Charbonneau ; David R. Ciardi ; Craig Kulesa ; Andrea K. Dupree ; Debra A. Fischer ; François Fressin ; Thomas N. Gautier III ; Ronald L. Gilliland ; Steve B. Howel ; Howard Isaacson ; Jon M. Jenkins ; Geoffrey W. Marcy ; Donald W. McCarthy ; Jason F. Rowe ; Natalie M. Batalha ; William J. Borucki ; Timothy M. Brown ; Douglas A. Caldwell ; Jessie L. Christiansen ; William D. Cochran ; Drake Deming ; Edward W. Dunham ; Mark Everett ; Eric B. Ford ; Jonathan J. Fortney ; John C. Geary ; Forrest R. Girouard ; Michael R. Haas ; Matthew J. Holman ; Elliott Horch ; Todd C. Klaus ; Heather A. Knutson ; David G. Koch ; Jeffrey Kolodziejczak ; Jack J. Lissauer ; Pavel Machalek ; Fergal Mullally ; Martin D. Still ; Samuel N. Quinn ; Sara Seager ; Susan E. Thompson ; Jeffrey Van Cleve ;
Date 27 Jun 2011
AbstractWe present the discovery of a hot Jupiter transiting an F star in a close visual (0.3" sky projected angular separation) binary system. The dilution of the host star’s light by the nearly equal magnitude stellar companion (~ 0.5 magnitudes fainter) significantly affects the derived planetary parameters, and if left uncorrected, leads to an underestimate of the radius and mass of the planet by 10% and 60%, respectively. Other published exoplanets, which have not been observed with high-resolution imaging, could similarly have unresolved stellar companions and thus have incorrectly derived planetary parameters. Kepler-14b (KOI-98) has a period of P = 6.790 days and correcting for the dilution, has a mass of Mp = 8.40 +0.19-0.18 MJ and a radius of Rp = 1.136 +0.073-0.054 RJ, yielding a mean density of rho = 7.1 +- 1.1 g cm-3.
Source arXiv, 1106.5510
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