WZ Sge: strikingly different profile! (Sep. 10) Dear Colleagues, WZ Sge has shown another veru striking change in its orbital light curve! The analysis of the most recent data (L. Cook) has revealed that the profile has now become "sinusoidal", i.e. smooth maximum at phase 0.5 and minimum at phase slightly before 0. The overall appearance of the profile even resembles that of a reflection-type variable! Although it is not unlikely that we are observing the illuminated surface of the secondary star (reflection effect), the chance seems to be small because the disk light should have dominated at present. Anyway, such a profile has not been observed so far even during the entire rebrigtening period. Observers are strongly requested to follow the evolution of the light curve, and record the dramatic change! The representative light curves of the 11-th rebrightening have been posted on the VSNET WZ Sge page. Regards, Taichi Kato VSNET Collaboration team