Our time series analysis of V 368 Cep photometry ascertains the rotation pe
riod of 2.(d)74 uniquely. The manifestations of starspot induced luminosity
variations in this chromospherically active star include rapid light curve
changes and differential rotation of about 3%. We conclude that the single
rapidly rotating variable V 368 Cep is a high inclination Klv post T Tauri
star.