Electronic Telegram No. 3387 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 COMET P/2013 B1 = P/2006 K2 (McNAUGHT) J. V. Scotti, Lunar and Planetary Laboratory, University of Arizona, reports his recovery of comet P/2006 K2 (cf. IAUC 8714) on images obtained with the Spacewatch 1.8-m f/2.7 reflector at Kitt Peak (astrometry tabulated below); the object appeared very slightly diffuse on both nights (with a possible tail, but aligned with a faint star trail and may not be real on the Jan. 19 image; the comet was too close to a field star on Jan. 20 to determine anything about a tail). 2013 UT R.A. (2000) Decl. Mag. Observer Jan. 19.53190 13 54 18.15 -10 39 53.1 21.8 Scotti 19.53935 13 54 18.62 -10 39 56.0 22.0 " 19.54616 13 54 19.08 -10 39 59.5 21.9 " 20.50575 13 55 23.23 -10 47 31.2 19.7 " 20.51318 13 55 23.66 -10 47 34.2 21.0 " 20.52061 13 55 24.18 -10 47 38.0 21.9 " The indicated correction to the prediction by B. G. Marsden on MPC 69911 is Delta(T) = -0.17 day. The following linked orbital elements by G. V. Williams (from 98 observations spanning 2006 May 22-2013 Jan. 20; mean residual 0".5) and an ephemeris appear on MPEC 2013-B58. Epoch = 2013 Aug. 16.0 TT T = 2013 Aug. 2.49291 TT Peri. = 237.99202 e = 0.4332735 Node = 15.50186 2000.0 q = 2.0977230 AU Incl. = 6.68168 a = 3.7014734 AU n = 0.13840192 P = 7.12 years NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2013 CBAT 2013 January 21 (CBET 3387) Daniel W. E. Green