Electronic Telegram No. 5081 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 (37424) 2001 YA_3 V. Benishek, Belgrade Astronomical Observatory; P. Pravec, Ondrejov Observatory; P. Sogorb, La Bastide des Jourdans, France; and R. Durkee, Shed of Science South Observatory (SSSO), Pontotoc, TX, U.S.A., report that photometric observations taken with a 0.35-m telescope at the Sopot Observatory in Serbia, a 0.28-m telescope at the Bastidan Observatory in France, and a 0.50-m telescope at the SSSO during Sept. 26-Nov. 7 reveal that minor planet (37424) is a binary system with an orbital period of 18.956 +/- 0.006 hr. The primary shows a period of 2.8251 +/- 0.0002 hr and has a lightcurve amplitude of 0.11 magnitude at solar phases 6-9 degrees, suggesting a nearly spheroidal shape. Mutual eclipse/occultation events that are 0.05 magnitude deep indicate a lower limit on the secondary-to-primary mean- diameter ratio of 0.22. SSSO observations taken on Nov. 7 showed a 0.07-mag- deep brightness attenuation centered at Nov. 7.3069 UT and lasting for 35 min that was not phased to the 0.05-mag-deep mutual events repeating with the 18.956-hr period above; the suspicion that it was a mutual event by a second satellite needs to be confirmed with future observations. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2021 CBAT 2021 December 9 (CBET 5081) Daniel W. E. Green