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We present an orbital solution study for the newly discovered system 1SWASPJ080150.03+471433.8 by means of new CCD observations in VRI bands. Ourobservations were carried out on 25 Feb. 2013 using the Kottamia opticaltelescope at NRIAG, Egypt. 12 new times of minima were estimated and theobserved light curves were analysed using the Wilson-Devinney code. Theaccepted orbital solution reveals that the primary component of is more massiveand hotter than the secondary one by about 280K. The system is an over-contactone with fillout ratio ~ 29% and is located at a distance of 195 Pc. Theevolutionary status of the system is investigated by means of stellar modelsand empirical data.

Orbital solution and evolutionary state for the eclipsing binary 1SWASP J080150.03+471433.8