[IAUC] CBET 3418: 20130217 : COMET P/2013 CE_31 (MOSS)

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Dom Feb 17 16:19:11 ART 2013


                                                  Electronic Telegram No. 3418
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 en eps.harvard.edu (alternate cbat en iau.org)
URL http://www.cbat.eps.harvard.edu/index.html
Prepared using the Tamkin Foundation Computer Network


COMET P/2013 CE_31 (MOSS)
      An apparently asteroidal object discovery reported by Claudine Rinner
(discovery observations tabulated below) on CCD images taken with a 0.5-m f/3
reflector in the course of the Morocco Oukaimeden Sky Survey (MOSS; cf. CBET
3020) -- and assigned the minor-planet designation 2013 CE_31 on MPS 454006
(published Feb. 17) by the Minor Planet Center, with initial orbits appearing
on MPEC 2013-C43 and 2013-C46 (the "Daily Orbit Updates" for Feb. 10 and 11)
-- has been found to show cometary appearance by other CCD astrometrists.  An
independent discovery by Richard Wainscoat and Larry Denneau, University of
Hawaii, on images taken on Feb. 9 UT with the 1.8-m Pan-STARRS1 telescope (+
w filter) at Haleakala, was noted along with the presence of a tail > 1' long
in p.a. approximately 290 degrees; follow-up r-band images taken by Marco
Micheli and Wainscoat using the Canada-France-Hawaii Telescope at Mauna Kea
on Feb. 10 (queue observer Peter Forshay) show an extended nuclear
condensation, while three stacked images show the tail exending approximately
60" from the condensation in p.a. 290 deg.  J. Scotti (Lunar and Planetary
Laboratory, University of Arizona) writes that mosaic images taken by T. H.
Bressi with the Spacewatch 0.9-m f/3 reflector at Kitt Peak on Feb. 17.2
show a 9"-long tail in p.a. about 275 deg.  Scotti adds that subsequent
co-added images taken by R. S. McMillan, M. L. Terrenzoni, and himself on
Feb. 17.3 with the Steward Observatory 2.3-m Bok telescope show a coma
diameter of 7".0 and a narrow tail that extends 1'.67 in p.a. 285 degrees.

     2013 UT             R.A. (2000) Decl.       Mag.   Observer
     Feb.  5.11210   10 25 19.50   +15 40 21.8   20.3   Rinner
           5.12268   10 25 19.10   +15 40 23.7   20.2     "
           5.13316   10 25 18.81   +15 40 26.4   20.1     "
           5.14390   10 25 18.40   +15 40 29.0   19.5     "
           6.15171   10 24 46.84   +15 44 21.1   20.1     "
           6.16249   10 24 46.37   +15 44 23.2   20.4     "
           6.17299   10 24 46.05   +15 44 26.0   20.5     "
           6.18348   10 24 45.69   +15 44 28.3   20.0     "
           6.19400   10 24 45.34   +15 44 30.7   20.5     "

The available astrometry (including prediscovery Spacewatch observations
from Jan. 19), the following elliptical orbital elements by G. V. Williams,
and an ephemeris appear on MPEC 2013-D23.

     T = 2012 May  21.68047 TT        Peri. =  27.76370
     e = 0.1698669                    Node  =  87.15101 2000.0
     q = 4.0228047 AU                 Incl. =   4.72318
       a =  4.8459758 AU   n = 0.09239154   P =  10.67 years


NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
      superseded by text appearing later in the printed IAU Circulars.

                         (C) Copyright 2013 CBAT
2013 February 17                 (CBET 3418)              Daniel W. E. Green



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