THE ASTRONOMER Electronic Circular No 564      1991 Sept 21 14.30UT
Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise,  Basingstoke,
Hants, RG22 4PP, England. Telephone:  (0256)471074 Int:+44256471074
Telex: 9312111261 Answerback: TA G                     JANET BOXES:
GMH at UK.AC.CAM.ASTRONOMY.STARLINK or GUYH at UK.AC.SUSSEX.CLUSTER
TELECOM GOLD: 10074:MIK2885                       PRESTEL 256471074
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V635 CAS
Gary Poyner, Birmingham, reports that this optical component of an
x-ray source is again brightening (cf E514):
1991 Aug 4.00UT, 15.2; 9.06, 15.3; 12.04, 15.2; 18.01, 15.3; 18.99,
15.3; 20.05, 15.2; 30.97, 15.2; Sept 7.04, 14.9; 7.97, 15.1;
17.01, 14.8.

COMET SPACEWATCH (1991x)
J. V. Scotti, Lunar and Planetary Laboratory, has measured the
following positions of a comet discovered by T. Gehrels with the
0.91-m Spacewatch telescope on Kitt Peak.  On the final image the
condensation is essentially stellar, and there is a tail extending
more than 5' in p.a. 258 deg.
     1991 UT             R.A. (1950) Decl.         m2
     Sept. 8.26146   23 14 25.94   - 8 45 13.0
           8.28191   23 14 24.87   - 8 45 23.9     21.1
           8.30510   23 14 23.57   - 8 45 35.2
           8.32431   23 14 22.64   - 8 45 45.9
           8.34513   23 14 21.49   - 8 45 56.9
           8.36135   23 14 20.60   - 8 46 05.6     21.0
           9.27110   23 13 33.30   - 8 54 03.4
           9.27780   23 13 33.01   - 8 54 07.9     20.9
           9.28718   23 13 32.52   - 8 54 13.1
IAUC 5341

P/COMET CHERNYKH (1991o) SPLIT
J. Luu, Harvard-Smithsonian Center for Astrophysics; and D.Jewitt,
Institute for Astronomy, University of Hawaii, communicate:
"We have discovered that P/Chernykh has split.  Observations with
the 2.4-m telescope of the Michigan-Dartmouth-MIT Observatory on
Sept. 15 and 16 show that the secondary nucleus is separated from
the primary by 56".6 +/- 0".7 in p.a. 71 +/- 1 deg. Both primary
and secondary objects appear extended. The Mould R magnitudes of
the primary and secondary are 16.1 and 19.1, respectively, measured
within an 11".7-diameter diaphragm.  Neither the separation nor the
difference in magnitudes changed between nights."
IAUC 5347

SATELLITES OF SATURN AND NEPTUNE
The IAU Executive Committee has approved the following new
designations and names:
     Saturn XVIII  Pan       = 1981 S13
     Neptune III   Naiad     = 1989 N6
     Neptune IV    Thalassa  = 1989 N5
     Neptune V     Despina   = 1989 N3
     Neptune VI    Galatea   = 1989 N4
     Neptune VII   Larissa   = 1989 N2
     Neptune VIII  Proteus   = 1989 N1
The satellites of Neptune are numbered in order of increasing
distance from the primary.
IAUC 5347

Guy M Hurst