Long-Cycle Dwarf Nova 1815+50 DV DRACONIS a possible WZ Sge-type cataclysmic variable is in outburst. This is only the second recorded outburst of DV Dra; the first one was a super-outburst in June 1984, when the star reached photographic magnitude 15.1. Just now, DV Draconis is faint and near the sun, so it is a difficult target for visual observers.