Electronic Telegram No. 3780 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 A2 (HILL) [Editor's note: this text replaces that on CBET 3779 (correct dates).] R. E. Hill reports his discovery of a comet on CCD images taken with the Catalina Sky Survey's 0.68-m Schmidt telescope (discovery observations tabulated below); four co-added 40-s exposures taken in 4"-5" seeing on the discovery night show a condensed nuclear condensation around 7"-10" across and a fan-shaped tail 25"-30" long in p.a. about 270 deg, while follow-up images taken on Jan. 10.42-10.48 UT in 3"-5" seeing show a similar appearance, with the tail about 20"-25" long in p.a. about 270-275 deg. Follow-up images by J. A. Johnson with the Mount Lemmon 1.5-m reflector on Jan. 11.5 show a clearly visible coma about 6" in diameter and a tail in p.a. about 275 deg. After posting on the Minor Planet Center's PCCP webpage, other CCD astrometrists have also commented on the object's cometary appearance. J. V. Scotti writes that twenty-seven stacked exposures taken with the Spacewatch 1.8-m telescope at Kitt Peak on Jan. 10.55-10.56 show a 15" coma with a 0'.60 tail in p.a. 275 degrees, while twelve co-added 60-s exposures on Jan. 11.5 show a 13" coma with a 0'.65 tail in p.a. 274 degrees. H. Sato (Tokyo, Japan; remotely with an iTelescope 0.51-m f/6.8 astrograph + luminance filter near Mayhill, NM, U.S.A.; ten stacked 60-s exposures; Jan. 10.5) finds a moderately condensed coma of diameter 10" and a 30" tail toward p.a. 270 degrees, with magnitude 19.3 as measured within a circular aperture of radius 6".5. S. Foglia writes that seventy-five stacked 10-s images reveal a very diffuse round coma of diameter 12" in images taken by R. Holmes (Ashmore, IL, USA) on Jan. 14.4 with a 0.61-m f/4 astrograph of the Astronomical Research Observatory at Westfield. 2014 UT R.A. (2000) Decl. Mag. Observer Jan. 9.42551 10 23 39.27 +28 30 45.6 18.5 Hill 9.43066 10 23 39.37 +28 30 51.7 18.8 " 9.43581 10 23 39.43 +28 30 57.2 18.6 " 9.44095 10 23 39.48 +28 31 02.6 18.5 " 9.45355 10 23 39.72 +28 31 16.7 19.0 " 9.45937 10 23 39.81 +28 31 24.2 19.0 " 9.46515 10 23 39.84 +28 31 30.9 18.2 " 9.47091 10 23 39.86 +28 31 36.2 18.7 " The available astrometry, the following preliminary elliptical orbital elements by G. V. Williams, and an ephemeris appear on MPEC 2014-B01. T = 2013 Oct. 28.3871 TT Peri. = 356.2476 e = 0.649491 Node = 106.6719 2000.0 q = 2.074732 AU Incl. = 24.5132 a = 5.919191 AU n = 0.0684401 P = 14.40 years NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2014 CBAT 2014 January 16 (CBET 3780) Daniel W. E. Green