USNO 1395-0370731 is a 14.9 magnitude star in the constellation Cygnus. I discovered it to be variable on images taken on 22 October, 2010. Although only a portion of the lightcurve was observed, sufficient data was obtained to determine that the star was a W UMa eclipsing binary. Further observations were made during 2014 and 2015. These confirmed that the star is a W UMa variable. The period derived was 8.42990 hours and the amplitude was 0.31 magnitudes.