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Kepler-14b: A Massive Hot Jupiter Transiting an F Star in a Close Visual Binary

November 2011 • 2011ApJS..197....3B

Authors • Buchhave, Lars A. • Latham, David W. • Carter, Joshua A. • Désert, Jean-Michel • Torres, Guillermo • Adams, Elisabeth R. • Bryson, Stephen T. • Charbonneau, David B. • Ciardi, David R. • Kulesa, Craig • Dupree, Andrea K. • Fischer, Debra A. • Fressin, François • Gautier, Thomas N., III • Gilliland, Ronald L. • Howell, Steve B. • Isaacson, Howard • Jenkins, Jon M. • Marcy, Geoffrey W. • McCarthy, Donald W. • Rowe, Jason F. • Batalha, Natalie M. • Borucki, William J. • Brown, Timothy M. • Caldwell, Douglas A. • Christiansen, Jessie L. • Cochran, William D. • Deming, Drake • Dunham, Edward W. • Everett, Mark • Ford, Eric B. • Fortney, Jonathan J. • Geary, John C. • Girouard, Forrest R. • Haas, Michael R. • Holman, Matthew J. • Horch, Elliott • Klaus, Todd C. • Knutson, Heather A. • Koch, David G. • Kolodziejczak, Jeffrey • Lissauer, Jack J. • Machalek, Pavel • Mullally, Fergal • Still, Martin D. • Quinn, Samuel N. • Seager, Sara • Thompson, Susan E. • Van Cleve, Jeffrey

Abstract • We present the discovery of a hot Jupiter transiting an F star in a close visual (0farcs3 sky projected angular separation) binary system. The dilution of the host star's light by the nearly equal magnitude stellar companion (~0.5 mag 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+0.35 - 0.34 M J and a radius of Rp = 1.136+0.073 - 0.054 R J, yielding a mean density of ρ p = 7.1 ± 1.1 g cm-3.

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Jessie Christiansen

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David Ciardi

Senior Scientist