Electronic Telegram No. 5692
Central Bureau for Astronomical Telegrams
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(5482) KORANKEI
     V. Benishek, Belgrade Astronomical Observatory; and P. Pravec, Ondrejov
Observatory, report that photometric observations taken with a 0.35-m
telescope at the Sopot Observatory in Serbia during Mar. 7-Apr. 11 reveal
that minor planet (5482) is a binary system with an orbital period of 22.11 
+/- 0.01 hr.  The primary shows a period of 3.38507 +/- 0.00009 hr and has a 
lightcurve amplitude of 0.19 magnitude at solar phases 3-18 degrees, 
suggesting a nearly spheroidal shape.  Mutual eclipse/occultation events that
are 0.13 magnitude deep indicate a lower limit on the secondary-to-primary
mean-diameter ratio of 0.36.

NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
      superseded by text appearing later in the printed IAU Circulars.

                         (C) Copyright 2026 CBAT
2026 May 26                      (CBET 5692)              Daniel W. E. Green