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THE ASTRONOMER Electronic Circular No 905       1994 Dec 17 16.35UT
Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise,  Basingstoke,
Hants, RG22 4PP,England. Telephone/FAX(0256)471074 Int:+44256471074
INTERNET: GMH at AST.STAR.RL.AC.UK  or    GMH at GXVG.AST.CAM.AC.UK
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PERIODIC COMET KOPFF (1994s)
This comet has been recovered by C. W. Hergenrother, Lunar and
Planetary Laboratory, on CCD frames obtained by S. M. Larson with
the 1.5-m reflector at the Catalina Station.  The images are very
faint (near threshold on the second night).  The comet is stellar
in appearance, with no hint of a coma or tail.  The indicated
correction to the prediction on MPC 22032 is Delta(T) = +0.02 day.
     1994 UT             R.A. (2000) Decl.        m2
     Nov. 30.50175   10 26 18.01   +11 35 17.7   22.8
          30.50913   10 26 18.10   +11 35 17.7   22.0
          30.51556   10 26 18.21   +11 35 16.5   23.0
          30.52096   10 26 18.38   +11 35 16.5   21.8
     Dec.  1.51258   10 26 36.35   +11 34 25.1   22.8
           1.51769   10 26 36.56   +11 34 24.6   22.7
           1.52237   10 26 36.64   +11 34 24.6   23.0
IAUC 6111

PERIODIC COMET CLARK (1994t)
S. Nakano, Sumoto, Japan, reports the recovery of this comet
by A. Nakamura (Kuma Kogen, 0.60-m f/6.0 Ritchey-Chretien + CCD):
     1994 UT             R.A. (2000) Decl.        m1
     Dec.  5.85747   13 39 25.93   - 3 30 11.6   17.5
           5.86123   13 39 26.30   - 3 30 13.9
           5.86649   13 39 26.96   - 3 30 17.9
           6.84688   13 41 17.86   - 3 41 24.7   17.6
           6.85660   13 41 18.99   - 3 41 31.4
Nakamura notes the comet as being diffuse with central
condensation, with coma diameter 0'.35; on Dec. 5, there was a hint
of tail in p.a. 250 deg.
The following orbital elements by Nakano are from 35 observations,
1984-1994 (mean residual 0".92); nongravitational
parameters A1 = -0.31 +/- 0.73, A2 = -0.2796 +/- 0.0136.
T  1995 May  31.1063 TT      w 208.85468 )
e  0.50203950                O  59.72627 ) 2000.0
q  1.5524960 A.U.            i   9.50461 )
Source: IAUC 6112    Positions are geocentric
Ephemeris by G.Hurst using EPH.EXE by N.James:
m1 = 10.5 + 5.0 log R + 15.0 log r
  Date    R.A. (2000) Dec.     R       r     Elong  Mag.    Motion
          h  m       o  '     (AU)    (AU)     o          "/hr P.A.
1994 Dec
  14.00  13 54.94   -5  2.0   2.613   2.178   53.6  17.7    77  111
  19.00  14  4.64   -5 57.9   2.539   2.150   56.0  17.5    78  111
  24.00  14 14.48   -6 53.2   2.464   2.122   58.5  17.4    79  110
  29.00  14 24.46   -7 47.9   2.388   2.095   60.9  17.2    79  110
1995 Jan
   3.00  14 34.58   -8 41.8   2.313   2.067   63.3  17.1    80  110
   8.00  14 44.84   -9 34.9   2.237   2.040   65.7  16.9    81  109
  13.00  14 55.24  -10 27.1   2.162   2.013   68.0  16.7    81  109
  18.00  15  5.79  -11 18.4   2.087   1.986   70.4  16.6    82  108
  23.00  15 16.50  -12  8.6   2.013   1.960   72.7  16.4    83  107
  28.00  15 27.36  -12 57.8   1.939   1.934   75.0  16.2    84  107

KX AQUILAE
M.Iida, Nagano, Japan reports the detection of an outburst of this
obscure UG variable located at: RA 19h31m36s DEC +14 11.1[1950].
On 1994 Dec 6.379, mag 15.0 (0.16-m reflector + ST6 CCD unfiltered)
Confirmed by Osaka-Kyoiku Univ.team (K.Matsumoto) on Dec 6, R=16.

Guy M Hurst