RX Cha outburst The supposed SU UMa-type dwarf nova (reported superhump period 0.0839 d, Kato et al. (2001) IBVS 5117) is undergoing an outburst. The last outburst (superoutburst?) was in 2002 April. Although the present outburst may turn out to be a normal outburst, the excellent seasonal visibility would make RX Cha one of the most promising targets at this moment. Please observe as long as possible to check the presence of superhumps! YYYYMMDD(UT) mag observer 20021122.449 <144 (Rod Stubbings) 20021123.462 <144 (Rod Stubbings) 20021127.474 <146 (Rod Stubbings) 20021127.810 <144 (Andrew Pearce) 20021128.803 <150 (Andrew Pearce) 20021201.508 145 (Rod Stubbings) 20021201.567 145 (Rod Stubbings) Regards, Taichi Kato VSNET Collaboration team