WZ Sge superhump period Dear Colleagues, The most recent estimate of the superhump period better agrees that of Bohusz and Udalski 1979 (IBVS 1979), P=0.057213, than that of Patterson et al. 1981 (ApJ 248, 1067), P=0.05714, obtained on the occassion of the 1978 superoutburst. We have more closely examined these original data. The cycle counts in Bohusz and Udalski 1979 have been found to be correct (to the present knowledge of the new superhump period), while there seem to be ambiguities in superhump identifications in Patterson et al. 1981. We have securely identified three superhump timings on Dec. 22-25, and probable one on Dec. 28. Three possible superhump timings on Dec. 19 and 26 do not match the currently determined period, and the ephemeris by Bohusz and Udalski 1979. It is very likely the period of 0.05714 d was strongly affected by these "noisy" identifications. Using new secure identifications of superhump times, from Bohusz and Udalski 1979 and Patterson et al. 1981, we obtained a refined superhump period of 0.05722 d for the 1978 superoutburst. This superhump period is 1.0% longer than the orbital period. Regards, Taichi Kato VSNET Collaboration team