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I report on the discovery of two cataclysmic variables in the same field inLyra originally identified from their magnitudes in USNO-B1.0 catalogue andPalomar images. The historical light curves were analyzed on 300+ photographicplates from Moscow collection covering 35 years of observations. One of twostars, USNO-B1.0 1320-0390658, is showing rather frequent outbursts from B~20to B=15.2 and is likely a dwarf nova of UGSS subtype. The other variable,USNO-B1.0 1321-0397655, has only one observed outburst in 1993 from R~19 toI=11.8 and is either a UGWZ dwarf nova or a recurrent nova. In both cases itsnext outburst can occur in the nearest future.

Two New Cataclysmic Variables in Lyra