Possible superoutburst of GX Cas As notified by several observers, the SU UMa-type dwarf nova GX Cas is undergoing a very bright, likely super, outburst. YYMMDD(UT) mag observer 971018.480 <145 (G. Hanson) 971018.810 <152 (G. Poyner) 971019.128 <152 (G. Hanson) 971020.166 <152 (G. Hanson) 971021.783 136 (G. Poyner) 971021.790 133 (J. Pietz) 971021.850 130 (T. Kinnunen) The latest superoutburst of GX Cas occurred in 1996 Sept. - Oct., reaching mv=13.3 (J. Pietz). Time-resolved observations are highly encouraged for this SU UMa star, having one of the longest superhump periods. For more information of GX Cas, see http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/gxcas.html For a most recent compilation of parameters of SU UMa stars, see Nogami et al. (1997, PASP in press); preprint available from: http://ftp.kusastro.kyoto-u.ac.jp/pub/vsnet/preprints/SX_LMi Regards, Taichi Kato