Read IAUC 3427
Circular No. 3426
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 617-864-5758
SATURN
A. Dollfus, Observatoire de Paris, reports that a search for
an outer ring of Saturn has been made using a focal coronagraph
with the Pic du Midi reflector. A faint lineament was suspected on
two plates taken around Nov. 1d04h50m UT. It extends eastward in
the ring plane from the outer edge of ring A up to 3.40 Saturn
radii, where the image of Saturn II (Enceladus) is located. Its
yellow magnitude could be estimated as ~ 18 per linear arcsecond.
The line is not seen on the western side of Saturn.
1979 VA
Further precise positions have been reported as follows:
1979 UT R. A. (1950) Decl. Mag. Observer
Nov. 17.21181 1 45 31.02 +24 55 30.5 Giclas
22.15590 2 14 42.85 +24 06 42.6 Bowell
23.42936 2 20 44.74 +23 54 39.6 14 Gilmore
23.44603 2 20 49.14 +23 54 33.6 "
24.23750 2 24 20.70 +23 45 58.9 Kowal
24.25833 2 24 25.83 +23 45 47.0 "
H. L. Giclas and E. Bowell (Lowell Observatory, Anderson Mesa Station).
0.3-m photographic telescope. Measurer: M. L. Kantz.
A. C. Gilmore and P. M. Kilmartin (Happy Valley, Wellington). 0.2-m
astrograph. Long. = -174o45', Lat. = -41o20'.
C. Kowal (Hale Observatories). l.2-m Schmidt telescope. Beginning
and end of trail. Measurer: S. J. Bus.
A. W. Harris, Jet Propulsion Laboratory, reports that photoelectric
observations at Table Mountain Observatory on Nov. 16.1 UT
gave V = 13.25 +/- 0.05, B-V = +0.72, U-B = +0.30. The rotation
period deduced from the small-amplitude (~ 0.05 mag) lightcurve is ~
4 hours.
SUPERNOVA IN ESO 153-G27
J. Maza, Department of Astronomy, University of Chile, writes
that the offset of the supernova reported on IAUC 3424 is 6" east
(rather than west) and 15" north of the galaxy's nucleus.
1979 November 29 (3426) Brian G. Marsden
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