THE ASTRONOMER Electronic Circular No 737       1993 May  1 15.12UT
Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise,  Basingstoke,
Hants, RG22 4PP,England. Telephone/FAX(0256)471074 Int:+44256471074
TELEX: 9312111261 Answerback: TA G      TELECOM GOLD: 10074:MIK2885
GMH at UK.AC.RUTHERFORD.STARLINK.ASTROPHYSICS  STARLINK: RLSAC::GMH
GMH at UK.AC.CAM.ASTRONOMY.STARLINK            STARLINK: CAVAD::GMH
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COMET SHOEMAKER-LEVY (1993e)
Brian Marsden comments:
"Attempts at orbit determination from the Mar. 15-Apr. 1 arc
suggest that a parabolic solution is no longer viable, but the
likely location of the object near the surface of Jupiter's sphere
of influence--not to mention the near impossibility of measuring
the object's center of mass--continues to make the unequivocal
determination of an elliptical orbit extremely difficult.  A very
close encounter with Jupiter during 1992 continues to be a distinct
possibility, the most viable such solutions having still smaller
orbital eccentricities than in the example on IAUC 5726 and the
Jupiter encounter earlier in the year.  The orbit below puts the
object 0.007 AU from Jupiter on 1992 May 16 (tidal breakup
presumably requiring an approach to 0.001 AU) and indicates
that the object is at least temporarily in orbit about Jupiter and
currently near apojove at a distance of 0.31 AU.

		    Epoch = 1993 Apr. 3.0 TT
     T = 1997 Sept. 4.494 TT          Peri. = 348.427
     e = 0.07169                      Node  = 343.394   2000.0
     q = 4.71659 AU                   Incl. =   2.206
       a =  5.08085 AU     n = 0.086060     P =  11.45 years
IAUC 5744

Revised ephemeris by G.Hurst using EPH.EXE by N.James:

m =  3.0 + 5.0 log R + 10.0 log r

  Date    R.A. (2000) Dec.     R       r     Elong  Mag.    Motion
	  h  m       o  '     (AU)    (AU)     o          "/hr P.A.
1993 Apr
  13.00  12 17.27   -3  6.8   4.400   5.363  162.0  13.5    18  292
  18.00  12 15.12   -2 53.4   4.425   5.361  156.5  13.5    17  293
  23.00  12 13.13   -2 41.0   4.457   5.360  151.1  13.5    15  293
  28.00  12 11.34   -2 29.8   4.496   5.358  145.8  13.6    14  293
1993 May
   3.00  12  9.78   -2 19.9   4.540   5.356  140.5  13.6    12  293
   8.00  12  8.47   -2 11.6   4.590   5.355  135.3  13.6    10  293
  13.00  12  7.41   -2  4.8   4.645   5.353  130.2  13.6     8  293
  18.00  12  6.63   -1 59.7   4.705   5.351  125.1  13.6     5  294
  23.00  12  6.13   -1 56.3   4.768   5.349  120.2  13.7     3  294
  28.00  12  5.91   -1 54.8   4.835   5.348  115.3  13.7     1  300
1993 June
   2.00  12  5.98   -1 55.1   4.905   5.346  110.6  13.7     2  110
   7.00  12  6.33   -1 57.1   4.977   5.344  105.9  13.8     4  112
  12.00  12  6.96   -2  1.0   5.050   5.342  101.3  13.8     6  112
  17.00  12  7.85   -2  6.5   5.125   5.340   96.7  13.8     8  113
  22.00  12  9.00   -2 13.8   5.201   5.339   92.3  13.9    10  113
  27.00  12 10.41   -2 22.6   5.277   5.337   87.9  13.9    12  113
1993 July
   2.00  12 12.06   -2 33.1   5.352   5.335   83.6  13.9    14  113
   7.00  12 13.93   -2 45.0   5.427   5.333   79.3  13.9    16  113
  12.00  12 16.02   -2 58.3   5.501   5.331   75.1  14.0    18  113
  17.00  12 18.32   -3 13.0   5.574   5.329   71.0  14.0    19  113

DI UMA (Q1993/046)
Further to the outburst reported on E716 (charts on E716 and E717)
a further positive result has been obtained by G.Poyner on
Apr 23.968UT at 15.3. This was confirmed by T.Vanmunster on 26.8UT
at 15.7v.