Dear colleagues, I just concluded a 6.0 hours observing session (unfiltered CCD, 0.35-m f/6.3 SCT) of GZ Cnc at CBA Belgium Observatory. Atmospheric conditions tonight (January 31/February 01, 2003) were relatively good, with long and stable clear periods. The resulting light curve is amongst the most interesting, but also most complex ones I have seen in months (see www.cbabelgium.com). At the beginning of the session, GZ Cnc was fading by about 0.5 mag, as part of what seemed to be the slope of a superhump. The subsequent rise showed a first remarkable and symmetric dip of about 0.35 mag around JD ++2671.46. Apparently, this was the start of a gradual brightening of the object, which continued till the end of the session. However, this rising trend was superimposed with lots of irregular and short period oscillations about 0.1 - 0.2 mag in amplitude. Large amplitude modulations started to appear again in the light curve around JD ++2671.57, when GZ Cnc showed an amazing, eclipse-like 0.8 magnitude drop. After that, high amplitude variations continued to exist until the end of my observing session. What a nice show this variable puts on ! I'd be interested to see the further evolution, and hopefully some stations in the US will be able to take over from here. Best regards, Tonny Vanmunster CBA Belgium Observatory email : Tonny.Vanmunster@cbabelgium.com website : www.cbabelgium.com