CT Hya superoutburst? As reported by Rod Stubbings, the large-amplitude SU UMa-type dwarf nova CT Hya is undergoing a bright outburst. The outburst may be a superoutburst. The last reported superoutburst occurred in 2000 December. Although several past superoutbursts have been observed by the VSNET Collaboration, early coverage of a likely superoutburst is still very wanted. The star was claimed to be something intermediate between usual SU UMa stars and WZ Sge-type stars (or TOADs), see Nogami et al. 1996 (PASJ 48, 607). Early coverage is thus extremeely important to see whether there is any similarity of the superhump growth with WZ Sge-type stars. YYYYMMDD(UT) mag observer 20021015.368 <145 (Mike Simonsen) 20021101.435 <145 (Mike Simonsen) 20021101.728 <144 (Rod Stubbings) 20021107.680 <144 (Rod Stubbings) 20021110.746 <146 (Rod Stubbings) 20021111.742 140 (Rod Stubbings) 20021111.754 139 (Rod Stubbings) Regards, Taichi Kato VSNET Collaboration team