Electronic Telegram No. 2141 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION M.S. 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) CBAT@CFA.HARVARD.EDU (science) URL http://www.cfa.harvard.edu/iau/cbat.html COMET C/2010 B1 (CARDINAL) An object discovered by R. D. Cardinal (Rothney Astrophysical Observatory, University of Calgary, 0.50-m f/1.0 reflector; discovery observation below) and placed on the NEO Confirmation Page has been reported as cometary by several observers. Y. Ikari (Moriyama, Shiga-Ken, Japan, 0.26-m f/7.0 reflector) notes that some of his exposures on Jan. 22.6 UT showed a coma of diameter 0'.2. D. Chestnov writes that three stacked exposures on Jan. 22.8 by T. Kryachko (Engelhardt Observatory, Zelenchukskaya Station, 0.3-m f/7 reflector) showed that the object appeared "softer" than the surrounding stars (FWHM 3".8 for the object, 3".1 for the stars), having a 0'.1-0'.2 coma with a strong condensation but no tail. J. M. Aymami (Tiana, Spain, 0.25-m f/4.3 Schmidt-Cassegrain) remarks that 39 co-added images totaling 3900 seconds around Jan. 22.9 showed a compact but nebulous object displaying what seemed to be a faint coma measuring 7".5. L. Buzzi (Varese, Italy, 0.38-m f/6.8 reflector) writes that a quite deep (limiting magnitude 20.5) stacked image totaling 25 minutes around Jan. 23.9 in very good seeing (but with thin, high clouds) showed the object to be stellar in appearance, although inspection of its profile revealed a FWHM some 20-25 percent larger than nearby stars of similar brightness. 2010 UT R.A. (2000) Decl. Mag. Observer Jan. 19.22247 08 12 28.90 +73 42 01.1 17.7 Cardinal Further astrometry, the following parabolic orbital elements and an ephemeris are given on MPEC 2010-B36. T = 2011 Feb. 6.708 TT Peri. = 211.920 Node = 277.336 2000.0 q = 2.92257 AU Incl. = 101.867 NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2010 CBAT 2010 January 23 (CBET 2141) Brian G. Marsden