Electronic Telegram No. 4063 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION CBAT Director: Daniel W. E. Green; 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 (357439) 2004 BL_86 J. Pollock, Appalachian State University; P. Pravec, Ondrejov Observatory; J. Oey, Blue Mountains Observatory, Leura, NSW; and D. E. Reichart, J. B. Haislip and A. P. LaCluyze, University of North Carolina, Chapel Hill, report that photometric observations obtained during 2015 Jan. 20-24 reveal that minor planet (357439) is a binary system with an orbital period of 13.80 +/- 0.05 hr. The primary shows a period of 2.6205 +/- 0.0003 hr, and it has a lightcurve amplitude of 0.17 mag at solar phases 99-109 deg, suggesting a nearly spheroidal shape. Mutual eclipse/occultation events that are 0.05- to 0.07-magnitude deep indicate a secondary-to-primary mean-diameter ratio of 0.21 +/- 0.02. Minor planet 2004 BL_86 was discovered eleven years ago by the LINEAR program (cf. MPEC 2004-B80) and was later numbered (357439). Lance A. M. Benner, on behalf of the radar team reports that Goldstone delay-Doppler radar (8560-MHz, 3.5-cm, 3.75-m resolution) images obtained on 2015 Jan. 26 confirm that (357439) is a binary system. Preliminary estimates for diameters of the components are 300 m for the primary and 50-100 m for the secondary. Forty-four minor planets passing close to the earth have now been found to have companions via radar (eight of those discovered first via optical photometry), and at least two such minor planets have more than one companion. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2015 CBAT 2015 January 30 (CBET 4063) Daniel W. E. Green