Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 2229: 1969i; SN IN IC 3476

The following International Astronomical Union Circular may be linked-to from your own Web pages, but must not otherwise be redistributed (see these notes on the conditions under which circulars are made available on our WWW site).


Read IAUC 2228  SEARCH Read IAUC 2230
IAUC number


                                                  Circular No. 2229
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Cable Address: SATELLITES, NEWYORK
Western Union: RAPID SATELLITE CAMBMASS


COMET BENNETT (1969i)
     The following precise positions have been reported:

     1970 UT             R. A. (1950) Decl.       Mag.   Observer
     Jan.  6.04075     0 31 07.06   -64 31 49.1          Potter
          11.05195     0 14 44.98   -63 29 47.1            "
          12.07907     0 11 46.85   -63 16 35.8            "
          13.04437     0 08 52.65   -63 03 03.3            "
          14.05062     0 06 02.31   -62 49 12.2            "
          15.04441     0 03 18.76   -62 35 17.7            "
          16.08039     0 00 32.91   -62 20 33.4            "
          18.04512    23 55 31.81   -61 52 05.4            "
          29.03548    23 31 30.74   -59 01 04.2            "
          31.04113    23 27 40.48   -58 27 44.8            "
     Feb.  1.03932    23 25 48.38   -58 10 51.3            "
           2.03308    23 23 58.04   -57 53 52.2            "
           3.03379    23 22 08.37   -57 36 29.7            "
           4.03451    23 20 19.71   -57 18 55.0            "
           6.02902    23 16 45.46   -56 43 04.1            "
           7.02975    23 14 58.72   -56 24 35.2            "
           8.02701    23 13 12.72   -56 05 52.7            "
           9.02910    23 11 26.48   -55 46 42.2            "
          10.02840    23 09 40.41   -55 27 10.2            "
          11.02772    23 07 54.30   -55 07 08.5            "
          12.02982    23 06 07.43   -54 46 34.6            "
          13.02846    23 04 20.50   -54 25 32.6            "
          14.02778    23 02 32.81   -54 03 53.2            "
          15.02641    23 00 44.45   -53 41 34.8            "
          16.02649    22 58 54.90   -53 18 27.2            "
          17.02575    22 57 04.55   -52 54 31.9            "
          18.02508    22 55 12.99   -52 29 41.2            "
     Mar. 18.40017    22 04 24.52   -20 44 57.8    0.5   Rodriguez
          18.40090    22 04 24.29   -20 44 50.3            "
          21.38762    22 03 56.71   -12 46 58.5    0.5   Pereyra
          21.38831    22 03 56.69   -12 46 50.5            "
          21.38900    22 03 56.82   -12 46 44.0            "
          22.83698    22 04 32.1    - 8 34 19     -0.5   Seki
          22.84398    22 04 32.6    - 8 33 06              "

H. Potter and A. Lokalov (National Observatory, Santiago).  Cerro
   El Roble station; Maksutov astrograph.  Measurer: C. Torres;
   Computer: H. Wroblewski.
J. J. Rodriguez and Z. M. Pereyra (Cordoba Observatory for the
   CNEGH).  33-cm astrograph.  Measurer: Miss B. Oviedo.  Objective
   prism spectra of both head and tail show strong continuum and
   emission.  The curved dust tail, 10o long, shows filaments
   extending along the prolongation of the radius vector.
T. Seki (Kochi Observatory).  22-cm f/5 camera.  Tail > 5o.

     Mr. J. C. Bennett, Pretoria, writes that on March 20.1 the
tail could be traced with the naked eye to at least 11o; on March
28.1 the tail was traced to more than 6o in spite of poor conditions.
On March 22.1 the magnitude of the central condensation was
estimated as 1.0, and in an 8-cm refractor (magnification up to
227 x) short faint jets were seen radiating from it on the sunward
side.  A guided 20-min exposure taken at the same time by K. J.
Sterling shows a straight gas tail that is almost as prominent as
the dust tail and which can be followed for some 20o.

     Mr. K. Simmons, Jacksonville, Florida, writes that on March
25.5 the magnitude (7 x 50 binoculars) was 1.6.  A central condensation,
of magnitude 6.0, and 0'.2 to 0'.4 in diameter, was observed
with a 21-cm reflector; the coma was 5' in diameter, the
brightest portion about 2'.5.  A fan-shaped tail, 2o.5 long as seen
with the naked eye, curved to p.a. 225o (near the coma in p.a.
215-220o); there was a 2' counter tail at p.a. 90o and jets at p.a. 75o
and 105o.

     Mr. D. Li, Honolulu, describes orange "pin-wheel" streamers
that on March 26.6 appeared to come out of the western arc of the
head envelope and sweep around to the east.  The comet's total
magnitude was 0.0, a magnitude fainter than the previous morning.

     Mr. J. E. Bortle, Mount Vernon, New York, reports that on
March 28.4 the comet was of magnitude 0.5, with a brilliant central
condensation of magnitude 1.7.  The curved tail extended about 5o
in the brightly moonlit sky.  Fountain-type jets extended from the
nucleus, and the appearance was very similar to that of comet 1861
II, as depicted by Secchi and by Schmidt.


SUPERNOVA IN IC 3476
     Mr. K. Locher, Wetzikon, Switzerland, sends the following
visual estimates (from comparison with nearby MVSO sequences):

       1970 UT            V
       Mar. 28.88   13.6 +/- 0.2
            30.85   13.8 +/- 0.2


1970 April 6                   (2229)              Brian G. Marsden

Read IAUC 2228  SEARCH Read IAUC 2230


Our Web policy. Index to the CBAT/MPC/ICQ pages.


Valid HTML 4.01!