COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS NUMBER 659 Konkoly Observatory Budapest 1972 April 12 W UMa PHOTOELECTRIC MINIMA AND A NEW PERIOD VARIATION The period of W UMa was retained constant since 1951 and the light elements were: Min I=J.D. 2435918.4154+0.33363808 E. The figure shows the residuals referred to these elements, starting only from 1961. Between the end of 1963 and 1964, a delay of about 7 minutes occurred in the epochs of minimum without change of period: the observations till 1969 were well represented by only adding a constant term of +0.00525 to the zero epoch. A trend to a slightly shorter period was suspected after the observations of 1969 (Cester 1969, 1971) but the correction to the period amounted to only -7.10^-8. The observations of 1971 and 1972 confirm the suspicion and now the period is decidedly shorter. The new provisional elements deduced from the observations from 1970 to 1972 should be Min I=J.D.2440652.4107+0.3336369 E. i.e. the period variation begun after 1968-69 is of the order of 10^-6 days. The unpublished recent photoelectric minima obtained at Trieste are collected in the table: (O-C)_1 refers to the first light elements and (O-C)_2 to the latter ones. Hel. J.D. 2441000+ m.e. (O-C)_1 (O-C)_2 004.3979 +-0.0003 +0.0036 +0.0003 008.40114 0.00006 +0.0032 -0.0001 048.4376 0.0014 +0.0032 -0.0001 057.44612 0.00005 +0.0034 +0.0002 061.4492 0.0002 +0.0028 -0.0003 061.4491 0.0001 +0.0027 -0.0004 351.3799 0.0008 +0.0020 -0.0001 363.3910 0.0001 +0.0021 +0.0001 392.4175 0.0010 +0.0021 +0.0002 396.421313 0.00004 +0.0023 +0.0003 Ref.: B. Cester, 1969 Mem SAIt 40, 489 [BIBCODE 1969MmSAI..40..489C ] B. Cester, 1971 Mem SAIt 42, 61. [BIBCODE 1971MmSAI..42...61C ] [FIGURE 1] B. CESTER and M. PUCILLO Osservatorio Astronomico Trieste, Italy