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IAUC 4215: 1986 JK; 1986G

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                                                  Circular No. 4215
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 617-495-7244/7440/7444


1986 JK
     C. S. and E. M. Shoemaker report their discovery with the
0.46-m Schmidt telescope at Palomar of an asteroidal object, near
opposition but having direct motion:

     1986 UT            R.A.   (1950.0)    Decl.        B

     May   4.33281     15 15 27.38     -14 18 15.7
           5.37830     15 16 43.38     -14 25 17.0     17.5
           9.30764     15 22 38.63     -14 59 10.4
          10.27552     15 24 28.35     -15 09 51.0
          10.46563     15 24 47.74     -15 12 02.1

     1986 JK appears to be an Apollo object approaching the earth:

          T = 1986 July 1.461 ET
      Peri. = 232.229                    e =   0.70812
      Node  =  62.315   1950.0           a =   3.06993 AU
      Incl. =   2.200                    n =   0.183236
          q =   0.89604 AU               P =   5.38 years

     1986 ET     R.A. (1950.0) Decl.      p        r       V

     May  14    15 33.59    -16 03.4    0.137    1.147    15.3
          16    15 40.63    -16 44.8
          18    15 50.14    -17 39.5    0.102    1.113    14.6
          20    16 03.61    -18 53.8
          22    16 23.90    -20 37.2    0.069    1.080    13.8
          24    16 57.00    -23 02.9
          26    17 56.29    -26 09.2    0.040    1.049    13.1
          28    19 44.39    -27 41.8
          30    22 05.48    -21 44.8    0.030    1.020    13.9
     June  1    23 45.87    -12 07.7
           3     0 40.55    - 5 25.6    0.051    0.994    16.7


SUPERNOVA 1986G IN NGC 5128
     I. Bues, Remeis Observatory, Bamberg; H. W. Duerbeck, Astronomical
Institute, Muenster; and L. Kohoutek, Hamburg Observatory,
report: "Spectra (380-580 nm) taken with the 1.52-m telescope at
the European Southern Observatory on May 7.1 UT show the reddened
spectrum of a type I supernova around maximum.  Photomery with the
ESO 0.5-m telescope on May 8.2 gives V = 11.58, B-V = +0.99, U-B =
+0.51, indicating a small brightness increase since discovery."


1986 May 13                    (4215)              Brian G. Marsden

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