Electronic Telegram No. 4902 Central Bureau for Astronomical Telegrams Mailing address: Hoffman Lab 209; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A. e-mail: cbatiau at eps.harvard.edu (alternate cbat at iau.org) URL http://www.cbat.eps.harvard.edu/index.html Prepared using the Tamkin Foundation Computer Network (4788) SIMPSON P. Sogorb, La Bastide des Jourdans, France; P. Pravec, Ondrejov Observatory; M. Husarik, G. Cervak, and M. Pikler, Skalnate Pleso Observatory; R. Durkee, Shed of Science South Observatory, Pontotoc, TX, U.S.A.; V. Benishek, Belgrade Astronomical Observatory; J. M. Bosch, Santa Maria de Montmagastrell, Tarrega, Spain; R. Behrend, Geneva Observatory; and V. Chiorny, Kharkiv Observatory, report that photometric observations taken with a 0.28-m telescope at the Bastidan Observatory in France, a 0.61-m telescope at the Skalnate Pleso Observatory, a 0.50-m telescope at the Shed of Science South Observatory, a 0.35-m telescope at the Sopot Observatory in Serbia, a 0.41-m telescope at the Santa Maria de Montmagastrell Observatory, and a 0.70-m telescope at the Chuguev station of the Kharkiv Observatory in Ukraine during 2020 Sept. 27-Nov. 15 reveal that minor planet (4788) is a binary system with an orbital period of 14.98 +/- 0.01 hr. The primary shows a period of 2.81752 +/- 0.00008 hr and has a light-curve amplitude of 0.18 mag at solar phases 4-12 degrees, suggesting a nearly spheroidal shape. Mutual eclipse/occultation events that are 0.03 to 0.07 magnitude deep indicate a lower limit on the secondary-to-primary mean-diameter ratio of 0.17. There is also a second rotational lightcurve component with a period of 3.1506 +/- 0.0002 hr and an amplitude of 0.03 mag in the combined primary-plus-secondary lightcurve, which may belong to the eclipsing/occulting secondary or to a third body of the system. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2021 CBAT 2021 January 7 (CBET 4902) Daniel W. E. Green