Electronic Telegram No. 5528 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 (9010) CANDELO V. Benishek, Belgrade Astronomical Observatory; P. Pravec, Ondrejov 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 and a 0.50-m telescope at the Shed of Science South Observatory during Jan. 26-Mar. 4 reveal that minor planet (9010) is a binary system with an orbital period of 12.958 +/- 0.003 hr. The primary shows a period of 3.1349 +/- 0.0005 hr and has a lightcurve amplitude of 0.10 magnitude at solar phases 2-6 degrees, suggesting a nearly spheroidal shape. Mutual eclipse/occultation events that are 0.06 magnitude deep indicate a secondary-to-primary mean-diameter ratio of 0.24 +/- 0.02. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2025 CBAT 2025 March 20 (CBET 5528) Daniel W. E. Green