MM Hya bright outburst! As already reported by Rod Stubbings and Andrew Pearce, the SU UMa-type dwarf nova MM Hya = PG0911-066 is undergoing a rare, bright (reaching 13.0 mag) outburst. The outburst is most likely a superoutburst. The last superoutburst of MM Hya (most of outbursts of MM Hya are superoutburst, as in SW UMa and WZ Sge-type dwarf novae) was observed in 2000 April. Observations of superhumps are strongly encouraged, as well as time-resolved spectroscopy to possibly detect spiral waves (the system is possibly a rather high-inclination system, and the lines may be detected in emission even during outburst). Regards, VSNET Collaboration team