Electronic Telegram No. 4262 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 (2535) H{\"A}MEENLINNA V. Benishek, Belgrade Astronomical Observatory; D. Pray, Sugarloaf Mountain Observatory, South Deerfield, MA, U.S.A.; P. Pravec, P. Kusnirak, K. Hornoch, H. Kucakova, and J. Vrastil, Ondrejov Observatory; J. Pollock, Appalachian State University; R. Groom and K. Stranger, Perth Observatory; A. Carbognani, Astronomical Observatory of the Aosta Valley Autonomous Region, Italy; R. Montaigut and A. Leroy, OPERA Observatory, France; and D. Reichart and J. Haislip, University of North Carolina, Chapel Hill, report that photometric observations taken with a 0.35-m telescope at the Sopot Observatory in Serbia, a 0.50-m telescope at the Sugarloaf Mountain Observatory, a 0.65-m telescope at the Ondrejov Observatory, a 0.36-m telescope at the Perth Observatory, a 0.81-m telescope at the Observatory of the Aosta Valley Autonomous Region, and a 0.20-m telescope at the OPERA Observatory during 2015 Dec. 18-2016 Feb. 19 reveal that minor planet (2535) is a binary system with an orbital period of 21.23 +/- 0.01 hr. The primary shows a period of 3.23106 +/- 0.00006 hr and has a lightcurve amplitude of 0.10 mag at solar phases 2-8 degrees, suggesting a nearly spheroidal shape. Mutual eclipse/occultation events that are 0.05- to 0.10-magnitude deep indicate a lower limit on the secondary-to-primary mean-diameter ratio of 0.22. The secondary is synchronous, and it has an amplitude of 0.03 mag in the observed lightcurve, suggesting a secondary elongation of about 1.5 after removing contribution of light from the primary. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2016 CBAT 2016 February 25 (CBET 4262) Daniel W. E. Green