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IAUC 3826: 1983e

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                                                  Circular No. 3826
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
TWX 710-320-6842 ASTROGRAM CAM     Telephone 617-864-5758


COMET SUGANO-SAIGUSA-FUJIKAWA (1983e)
     Further precise positions have been reported as follows:

      1983 UT           R.A.   (1950.0)    Decl.      Observer

      June  6.46876    23 43 16.65    +38 22 23.7     Schweizer
            7.44514    23 28 23.86    +37 20 18.9     Giclas
            7.46043    23 28 08.78    +37 19 09.1     Schweizer
            9.29265    22 45 20.0     +33 28 15       Schwartz
           10.74576    21 46 39.16    +25 57 49.9     Gilmore
           10.76218    21 45 44.68    +25 49 50.9       "
           11.25391    21 18 14.0     +21 15 53       McCrosky
           11.29142    21 15 56.4     +20 50 59         "
           11.60836    20 55 33.10    +17 07 20.7     Gilmore
           11.61924    20 54 49.10    +16 58 56.6       "

F. Schweizer (Palomar Observatory).  1.2-m Schmidt telescope.
   Time changed by -5 min on June 6.  Measurer: J. Gibson.
H. L. Giclas (Lowell Observatory, Anderson Mesa Station).  Very
   diffuse and uncertain.  Measurer: E. Bowell.
G. Schwartz and R. E. McCrosky (Oak Ridge Observatory).  1.5-m
   reflector. Measurer: McCrosky.  Very uncertain on June 11.
A. C. Gilmore (Mount John University Observatory).  0.6-m reflector.
   Measurer: P. M. Kilmartin.  Inkdot measured on June 10.

     The following parabolic orbital elements have been determined
(with perturbations included) by the undersigned from 37
observations May 9-June 11:

                       Epoch 1983 June 12.0 ET
         T = 1983 May 1.3283 ET  Peri. =  82.1659
                                 Node  =  82.3426   1950.0
         q =   0.471083 AU       Incl. =  96.6219

     R. H. McNaught, Royal Greenwich Observatory, remarks that the
closest approach of the earth to the comet's orbit occurs on June
14.7 UT, when the earth will pass 0.048 AU inside the comet's
orbit, 2.9 days after the comet has passed this point.  Meteors are
possible from R.A. = +21deg, Decl. = +42deg (equinox 1950.0), with
V = 53 km/s.  A similar prediction is given by I. Hasegawa on YC 1995.

     Visual estimates of total magnitude and coma diameter: June
9.22 UT, 7.4,~ 18' (D. W. E. Green, Harvard, MA, 20 x 80 binoculars);
10.97, 7.0, 30' (J.-C. Merlin, Le Creusot, France, 7 x 50
binoculars); 12.08, 6.6, - (Merlin).


1983 June 13                   (3826)              Brian G. Marsden

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