Electronic Telegram No. 3801 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 C2 (STEREO) K. Battams, Naval Research Laboratory, reports that a comet has been found by Alan Watson in images obtained with the STEREO-A satellite (visible in both COR-2 and HI-1 instrumental data), and astrometry and photometry was submitted to Battams from Man-To Hui (Canton, China), and the computed geocentric position for the first astrometric observation is tabulated below. Battams notes a nuclear condensation that is slightly diffuse, and the comet clearly has a thin, diffuse tail, adding that the peak brightness was probably around mag 6 (close to when it passed behind the COR-2 occulting disk) and that the comet may have transited the solar disk as observed from the spacecraft; by the time that the comet left the HI-1 field-of-view, the brightness was around mag 12, and it then appeared very diffuse and elongated with no nuclear condensation apparent. 2014 UT R.A. (2000) Decl. Mag. Feb. 1.46 20 09.77 -19 34.0 7.0 The reduced astrometry, along with the following parabolic orbital elements G. V. Williams and a search ephemeris for ground-based observers to try looking for the comet, appear on MPEC 2014-C25. The object may be near mag 13-14 at elongations 20-30 deg for ground-based observers in the next week or two, if the comet has survived intact. T = 2014 Feb. 18.6577 TT Peri. = 57.5181 Node = 283.3470 2000.0 q = 0.508074 AU Incl. = 135.3097 NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2014 CBAT 2014 February 8 (CBET 3801) Daniel W. E. Green