Electronic Telegram No. 5097 Central Bureau for Astronomical Telegrams Mailing address: Hoffman Lab 209; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A. e-mail: cbatiau@eps.harvard.edu (alternate cbat@iau.org) URL http://www.cbat.eps.harvard.edu/index.html Prepared using the Tamkin Foundation Computer Network (5121) NUMAZAWA V. Benishek, Belgrade Astronomical Observatory; P. Pravec, Ondrejov Observatory; V. Chiorny, Kharkiv Observatory; and R. Durkee, Shed of Science South Observatory, Pontotoc, TX, U.S.A., report that photometric observations taken with a 0.35-m telescope at the Sopot Observatory in Serbia, a 0.70-m telescope at the Chuguev station of the Kharkiv Observatory in Ukraine, and a 0.50-m telescope at the Shed of Science South Observatory during 2021 Oct. 20-Dec. 8 reveal that minor planet (5121) is a binary system with an orbital period of 17.18 +/- 0.01 hr. The primary shows a period of 2.6646 +/- 0.0002 hr and has a lightcurve amplitude of 0.13 magnitude at solar phases 6-9 degrees, suggesting a nearly spheroidal shape. Mutual eclipse/occultation events that are 0.07 to 0.14 magnitude deep indicate a lower limit on the secondary-to-primary mean-diameter ratio of 0.26. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2022 CBAT 2022 February 14 (CBET 5097) Daniel W. E. Green