COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 683 Konkoly Observatory Budapest 1972 May 29 NEW VARIABLE STAR IN THE OPEN CLUSTER NGC 7128 The star No. 5 of the Hoag etal. (1961, Publ. Naval Obs. Vol. XVII, Part VII.) catalogue located exactly in the centre of the open cluster NGC 7128 has been found as variable during photographic observations of the Nova Cephei 1971 between July 18, 1971 and April 20, 1972 with the Schmidt camera (80/120, f=240 cm) of Hamburg Observatory. This star, denoted in our list as HBV 478, RA=21h42m13.88s, D=+53deg29'32.2" (1950, Cygnus) was measured on 18 plates in the V (Kodak 103a-D+GG11) and B (Kodak IIa-O+GG13) international system, giving the following results: JD_hel V B JD_hel V B 2441151.489 12.57m - 2441207.46 12.14 12.99 1172.380 12.34 - 1240.36 12.13 13.07 1181.508 - 12.98m 1266.27 12.35 13.17 1183.427 12.43 - 1331.26 12.36 13.06 1183.513 - 13.00 1394.62 12.60 13.43 1187.487 12.53 - 1428.58 12.26 12.86 Mean V=12.37, B=13.07 The mean deviation of one measurement, +-0.17m both in V and B, is about three times larger than the corresponding measuring errors, which strongly supports the variability of that star. The amplitude of about 0.5 mag. in both colours could be suspected. Our mean V and B values are in close agreement with those given by Hoag et al., V=12.35, B-V=+0.78, U-B=0.00. The determination of the type of variability and further studies of this star could be very useful because of the fact that HBV 478=7128-5 is an early-type star (B2V - Hoag, Applequist 1965, ApJ Suppl. No. 107, 215) and a physical member of the cluster. Hamburg-Bergedorf Observatory 18 May, 1972 L. KOHOUTEK