V485 Cen likely superoutburst The ultra-short period SU UMa-type dwarf nova V485 Cen is vyer likely undergoing a superoutburst. Time-resolved photometry (2 hour long or hopefully longer) is highly desired. If you succeed observing, please send your data also to Ishioka-san and Uemura-san (ishioka@kusastro.kyoto-u.ac.jp and uemura@kusastro.kyoto-u.ac.jp) for prompt analysis. YYYYMMDD(UT) mag observer 20020715.510 <140 (Rod Stubbings) 20020717.373 <140 (Rod Stubbings) 20020718.392 <139 (Rod Stubbings) 20020726.378 <144 (Rod Stubbings) 20020727.371 <144 (Rod Stubbings) 20020729.371 <148 (Rod Stubbings) 20020730.371 <144 (Rod Stubbings) 20020731.367 <140 (Rod Stubbings) 20020801.381 <144 (Rod Stubbings) 20020806.374 139 (Rod Stubbings) 20020806.382 139 (Rod Stubbings) 20020806.465 139 (Rod Stubbings) Regards, Taichi Kato VSNET Collaboration team