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IAUC 5189: 1991g; 1986 III

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                                                  Circular No. 5189
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Telephone 617-495-7244/7440/7444 (for emergency use only)
TWX 710-320-6842 ASTROGRAM CAM     EASYLINK 62794505
MARSDEN or GREEN@CFA.BITNET    MARSDEN or GREEN@CFAPS2.SPAN


COMET McNAUGHT-RUSSELL (1991g)
     The following precise positions have been reported:

     1991 UT             R.A. (1950) Decl.        m1    Observer
     Jan. 26.71715   11 23 43.87   -25 29 12.5          McKenzie
     Feb. 13.59457   11 08 43.13   -22 43 19.9   17.5   Gilmore
          13.66755   11 08 38.98   -22 42 31.7            "
          14.48740   11 07 53.12   -22 33 17.9          McNaught
          15.53275   11 06 54.00   -22 21 17.1            "

P. McKenzie and R. H. McNaught (Siding Spring).  Uppsala Southern
  Schmidt, except prediscovery Jan. 26 U.K. Schmidt Telescope plate.
A. C. Gilmore and P. M. Kilmartin (Mt. John University Observatory).

     Preliminary parabolic elements from 8 observations, Jan. 26-Feb. 15:

     T = 1990 Oct. 14.427 ET          Peri. = 320.384
                                      Node  = 161.034   1950.0
     q = 4.77030 AU                   Incl. = 113.386

     1991 ET      R.A. (1950) Decl.     Delta      r       m1
     Feb. 13    11 09.27    -22 50.0    4.090    4.865    16.4
          18    11 04.54    -21 52.1
          23    10 59.67    -20 49.0    4.018    4.881    16.4
          28    10 54.73    -19 41.4
     Mar.  5    10 49.79    -18 29.6    3.982    4.898    16.4


PERIODIC COMET HALLEY (1986 III)
     O. Hainaut, A. Smette, European Southern Observatory, La Silla;
and R. M. West, ESO, Garching, report:  "CCD V photometry with the
1.54-m Danish telescope at La Silla (seeing about 1".3) indicates a
major eruptive event at r = 14.3 AU.  Preliminary V magnitudes:
Feb. 12.3 UT, 21.4; 13.2, 21.8; 14.2, 21.9 (5" circular aperture,
centered on light peak); the variation is within the photometric
uncertainty.  This compares to predicted mean m2 about 25.3 of the
nucleus alone.  The light peak is near the northwest edge of a
diffuse, elliptically-shaped coma with major axis in the northeast-
southwest direction; it measures > 20" across (projected 200 000 km)
and m1 about 19.  Inspection of a V frame obtained with the 3.5-m
New Technology Telescope on Feb. 15.2 does not show any apparent
change."


1991 February 15               (5189)             Daniel W. E. Green

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