Var73 Dra: first ER UMa-like dwarf nova in the period gap? Donn Starkey's most recent observation almost certainly confirms that the present outburst is a superoutburst(!). This finding suggests that the minimum supercycle length of Var73 Dra is around ~60 d (or possibly slightly shorter). This shortness of the supercycle is comparable to those of ER UMa-type dwarf novae. In conjunction with Antipin and Pavlenko (2002) A&A 391, 565, the supercycle of this object may not be as stable as in ER UMa stars. Such a variation of the supercycles was also recorded in the in-the-gap SU UMa-type dwarf nova, NY Ser (Nogami et al. 1998, PASJ 50, L1). Further observations of Var73 Dra during the present outburst is planned. We also strongly encourage multi-longitude observations to compensate the short visibility in this season. Regards, Taichi Kato VSNET Collaboration team