  We present the physical parameters of three short period close binaries using
the observed data from Kepler Space Telescope. All of these observations were
taken in a single bandpass (which approximates the Johnson V-band). Our three
systems are KIC 2715417, KIC 6050116 and KIC 6287172. The first system KIC
2715417 is considered a semi-detached system with the secondary component
filling the Roche lobe. The second system KIC 6050116 is an overcontact system,
while the third system KIC 6287172 belongs to ellipsoidal variables (ELV) as
deduced from the Roche lobe geometry. For photometric analysis, we used PHOEBE
software package which is based on the Wilson-Devinney code (Wilson-Devinney
1971). Due to lack of spectroscopic data, the photometric mass ratios are
determined from the analyses of the light curves using the Q-search method. The
absolute parameters are determined using three different methods, Harmanec
(1988), Maceroni-Van't Veer (1996) and Gazeas-Niarchos (2006).
