PHOTOMETRICALLY DERIVED MASSES AND RADII OF THE PLANET AND STAR IN THE TrES-2 SYSTEM

PHOTOMETRICALLY DERIVED MASSES AND RADII OF THE PLANET AND STAR IN THE TrES-2 SYSTEM

We measure the mass and radius of the star and planet in the TrES-2 system using 2.7 years of observations by the Kepler spacecraft. The light curve shows evidence for ellipsoidal variations and Doppler beaming on a period consistent with the orbital period of the planet with amplitudes of 2.79 [sup...

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Bibliographic Details
Main Authors: Barclay, Thomas, Huber, Daniel, Rowe, Jason F., Fortney, Jonathan J., Morley, Caroline V., Quintana, Elisa V., Fabrycky, Daniel C., Barentsen, Geert, Bloemen, S., Christiansen, Jessie L., Demory, Brice-Olivier, Fulton, Benjamin J., Jenkins, Jon M., Mullally, Fergal, Ragozzine, Darin, Seader, Shaun E., Shporer, Avi, Tenenbaum, Peter, Thompson, Susan E.
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:en_US
Published: IOP Publishing 2015
Online Access:http://hdl.handle.net/1721.1/95638

Internet

http://hdl.handle.net/1721.1/95638

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