Electronic Telegram No. 3937 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/2014 Q4 = P/2005 Q4 (LINEAR) K. Sarneczky, Szeged, Hungary, reports his recovery of comet P/2005 Q4 (cf. IAUC 8595) on CCD images obtained with a 0.60-m Schmidt telescope. He remarks that the object was stellar in appearance. G. V. Williams was able to identify additional observations of P/2005 Q4 taken with the 1.8-m Ritchey-Chretien Pan-STARRS telescope earlier the same night. 2014 UT R.A. (2000) Decl. Mag. Observer Aug. 22.52203 0 18 19.48 -10 53 26.1 20.0 Pan-STARRS 22.53320 0 18 19.16 -10 53 25.5 20.2 " 22.54438 0 18 18.84 -10 53 24.8 20.1 " 22.55558 0 18 18.51 -10 53 24.1 20.2 " 22.99990 0 18 06.64 -10 52 59.1 19.9 Sarneczky 23.00831 0 18 06.39 -10 52 58.6 19.8 " 23.01422 0 18 06.22 -10 52 58.2 19.7 " The indicated correction to the prediction by G. V. Williams on MPC 75706 is Delta(T) = -0.26 day. The following linked orbital elements by Williams are from 186 observations spanning 2005 Aug. 31-2014 Aug. 23 (mean residual 0".5); additional orbital elements and an ephemeris appear on MPEC 2014-Q39. Epoch = 2005 Sept.27.0 TT T = 2005 Sept.28.24204 TT Peri. = 50.89975 e = 0.6065865 Node = 11.41425 2000.0 q = 1.7543503 AU Incl. = 17.64990 a = 4.4593035 AU n = 0.10466549 P = 9.417 years Epoch = 2015 Feb. 27.0 TT T = 2015 Feb. 16.51519 TT Peri. = 50.97474 e = 0.6079989 Node = 11.37084 2000.0 q = 1.7404116 AU Incl. = 17.66651 a = 4.4398131 AU n = 0.10535546 P = 9.355 years NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2014 CBAT 2014 August 24 (CBET 3937) Michael Rudenko