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We present 14.3 years of previously unpublished photometric observations of UX Ari. The observations were ob- tained between 1987.9 and 2002.2 using the T3 0.4-metre Automatic Photoelectric Telescope at Fairborn Observatory and consist of 1228 B band and 1213 V band measurements. The comparison star was 62 Ari. We have analyzed the new data together with previously published photometric observations. The V magnitude shows variations with dominant periods of about 12 and 25 years, where the longest period seems to correspond to an activity cycle. The previously reported anticorrela- tion between the B V colour and V magnitude variations is confirmed.

BVphotometry of UX Ari in the period 1987–2002