Possible recovery of V893 Sco, or a new variable star? Katsumi Haseda (haseda@mxs.meshnet.or.jp) reports the photographic discovery of a new variable star using 10cm F4.0 twin astrograph. Kodak T-Max 400 film was used. 16h 15m 15s.1 (J2000.0) -28o 37' 40" This object may be identical with the following ROSAT source. 161516.2 -283711 (2000.0) 1RXS161516.2-283712 0.346 0.94 0.53 Considering the rapid change in brightness, and the possible identity with the ROSAT source, this variable may be identical with V893 Sco, a "lost" suspected dwarf nova despite many investigators efforts. The object also lies ~6' from the obscure suspected variable NSV07570. Follow-up observations, quiescent photometry and spectroscopy, secure optical identification of the ROSAT source, future search for possible outbursts, and search for archival images are strongly encouraged. object YYMMDD(UT) mag code SCOV893? 980128.852 130p (HAS) SCOV893? 980201.843 125p (HAS) SCOV893? 980226.835 152p (HAS) SCOV893? 980301.817 152p (HAS) SCOV893? 980308.806 152p (HAS) Observer's code: (HAS): (tentative designation), Katsumi Haseda Regards, Taichi Kato