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We present the results of differential, time series photometry for GSC02038-00293, a suspected RS CVn binary, using data collected with the OpenUniversity's PIRATE robotic telescope located at the Observatori Astronomic deMallorca between 10 May and 13 June 2010. A full orbital period cycle in the Vband and partial cycle of B and R bands were obtained for GSC 02038-00293showing an orbital period of 0.4955 +/- 0.0001 days. This period is in closeagreement with that of previously published values but significantly differentto that found by the All Sky Automated Survey of 0.330973 days. We suggest GSC02038-00293 is a short period eclipsing RS CVn star and from our data alone wecalculate an ephemeris of JD 2455327.614 + 0.4955(1) x E. We also find that thepreviously observed six to eight year cycle of star spot activity whichaccounts for the behaviour of the secondary minimum is closer to six years andthat there is detectable reddening at both minima.

An investigation of GSC 02038-00293, a suspected RS CVn star, using CCD photometry