Electronic Telegram No. 3928 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 C/2014 OE_4 An apparently asteroidal object (discovery images tabulated below) reported by the Pan-STARRS program, that was posted on the Minor Planet Center's NEO Confirmation Page and given the minor-planet designation 2014 OE_4 (orbits on MPEC 2014-O57 and 2014-O70), has been found to be cometary. R. J. Wainscoat and M. Micheli report that images obtained with the Pan-STARRS 1.8-m reflector on July 26 and 28 show that the object is extended with respect to stellar images: FWHM 1".27 for 2014 OE_4 vs 1".13 for stars on July 26; 1".4 vs. 1"2 on July 28). D. J. Tholen reports that his images, obtained in evening twilight with the 2.24-m University of Hawaii reflector on July 30 and 31, show that 2014 OE_4 is an extended source. 2013 UT R.A. (2000) Decl. Mag. Observer July 26.28251 15 32 28.52 -15 22 47.16 20.7 Pan-STARRS 26.29446 15 32 28.44 -15 22 45.09 20.8 " 26.30641 15 32 28.34 -15 22 42.66 20.7 " G. V. Williams was able to link additional observations of 2014 OE_4 going back to May 8. The available astrometry, the following orbital elements by Williams (from 42 observations spanning 2014 May 8-July 31; mean residual 0".2), and an ephemeris appear on MPEC 2014-P08. Epoch = 2016 Nov. 28.0 TT T = 2016 Dec. 10.73533 TT Peri. = 65.75699 e = 0.9995837 Node = 240.40002 2000.0 q = 6.2429433 AU Incl. = 81.34323 NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2014 CBAT 2014 August 2 (CBET 3928) Michael Rudenko