WZ SAGITTAE (UGSU) Visual magnitude estimates by P. Schmeer, Bischmisheim, Germany: July 22.98 UT, [13.5 ; 23.886, 8.4 ; 23.896, 8.4 Sequence: Henden and Honeycutt, H/T Instrument: 203-mm SCT Outburst confirmed! WZ Sge is the dwarf nova with the brightest outbursts. Previous brightenings occurred on 1913 Nov. 27, 1946 June 28, and 1978 Dec. 1. These three outbursts were all supermaxima; normal outbursts of WZ Sge have not yet been observed. The intervals between the four known outbursts were 32.58, 32.43, and 22.64 years, respectively. So the current outburst occurs 10 years earlier than expected. What does this imply? Outbursts of WZ Sge do not occur very regularly? A few superoutbursts were missed during the last century (pretty unlikely)? Or could the current outburst be the first ever recorded normal outburst (mean cycle length about 11 years???)? There is still a gap of 13 hours between the last negative and the first outburst observation of WZ Sge. Did anyone in the Americas observe the WZ Sge field last night - or take a photo of the region? Regards, Patrick P.S.: SGEWZ 20010722.98 <135 Scp SGEWZ 20010723.886 84 Scp SGEWZ 20010723.896 84 Scp