Electronic Telegram No. 4305 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 (441987) 2010 NY_65 [Editor's note: this text replaces that on CBET 4304.] J. D. Giorgini, M. Brozovic, S. P. Naidu, L. A. M. Benner, Jet Propulsion Laboratory (JPL); P. A. Taylor Arecibo Observatory; and A. Greenberg, University of California at Los Angeles, report that a non-gravitational acceleration has been detected influencing the motion of minor planet (441987). Recent Goldstone (8560-MHz, 3.5-cm) and Arecibo (2380-MHz, 12.6-cm) radar imaging at 15-m resolution produced round-trip delay measurement of the center-of-mass of (441987) to within 56-m over 2016 June 21, 22, and 26. Consistently biased delay offsets were observed, having a mean of -10.9 +/- 1.0 x 10^{-6} seconds relative to the prior gravity-only prediction of JPL orbit solution 63. This nominal ballistic trajectory estimate was based on 220 initial plane-of-sky optical angle measurements spanning 2010-2016 combined with four prior round-trip time-delay measurements and two Doppler frequency shift measurements reported by Arecibo in 2014 and 2015. The systematic 2.5-sigma offset observed is consistent with a mean heliocentric transverse non-gravitational acceleration over the data arc of -9.2 +/- 2.3 x 10^{-13} m/s^2, as subsequently estimated in JPL orbit solution 65 (dated 2016 July 29), with a 15-percent reduction in total dataset post-fit residual chi-square. The combined astrometric dataset consists of 228 optical angular measurements spanning 2010-2016 and the three radar apparitions spanned by nine radar delay and three Doppler-shift measurements. This object will continue to make yearly close approaches to the earth, and the authors anticipate future measurements in 2017, 2018, 2019, and 2020 that will be at least as precise, permitting ongoing refinement and characterization of the estimated force. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2016 CBAT 2016 August 22 (CBET 4305) Daniel W. E. Green