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IAUC 2210: 1969b; (1620); 1970a

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                                                  Circular No. 2210
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 KOHOUTEK (1969b)
     The following precise positions have been reported:

     1969/70 UT          R.A. (1950) Decl.       Mag.   Observer
     Dec.  3.38194   18 22 51.48   +28 21 34.3          Seki
           9.38819   18 28 28.94   +29 07 48.0            "
     Jan.  7.87535   19 06 00.09   +35 50 35.4            "
           8.86788   19 07 36.60   +36 10 06.6   12       "
          10.88229   19 10 56.30   +36 51 08.6            "
          11.87972   19 12 38.77   +37 12 09.4            "
          15.87301   19 19 45.31   +38 40 57.2   10       "
          15.88056   19 19 46.18   +38 41 04.1            "
          18.88264   19 25 28.81   +39 52 57.5            "
          19.87865   19 27 26.56   +40 17 44.2            "
          31.74630   19 54 28.81   +45 51 34.3          Milet
     Feb.  3.74711   20 02 38.02   +47 27 12.5            "

T. Seki (Kochi Observatory).
B. Milet (Nice Observatory).


(1620) GEOGRAPHOS
     Mr. M. Antal, Skalnate Pleso Observatory, communicates the
following positions, obtained with the 30-cm f/5 astrograph:

     1969 UT             R.A. (1950) Decl.
     Sept. 8.87500   20 20 37.00   - 7 53 20.2
           8.89097   20 20 41.49   - 7 51 46.7
           9.84653   20 25 17.55   - 6 22 57.2
           9.85347   20 25 19.47   - 6 22 20.8*
           9.86181   20 25 21.38   - 6 21 33.3*
           9.86875   20 25 23.21   - 6 20 58.8
           9.88264   20 25 26.82   - 6 19 44.4
           9.88958   20 25 28.53   - 6 19 11.2*
           9.89653   20 25 30.45   - 6 18 33.0
           9.90347   20 25 32.19   - 6 17 56.2
           9.91042   20 25 33.86   - 6 17 20.7*

* Measurement difficult.


COMET DAIDO-FUJIKAWA (1970a)
     Further precise positions have been reported as follows:

     1970 UT             R.A. (1950) Decl.       Mag.   Observer
     Feb.  2.85417*  19 29 11.67   + 0 52 43.6    7.0   Urata
           4.84635   19 41 44.65   - 1 13 43.1          Yumoto
           6.54965   19 53 53.05   - 3 16 14.1          Giclas
           6.85197** 19 56 11.99   - 3 39 28.9    6     Urata

T. Urata (Nihondaira Observatory).  * Tail 0.5o.  ** Tail 1.5o.
T. Yumoto (Tachibana Observatory).  Long. = -138o25', Lat. = +35o01'.
H. L. Giclas (Lowell Observatory).  33-cm photographic telescope.

     Dr. Elizabeth Roemer, Lunar and Planetary Laboratory, reports
that on Feb. 7.5 at least 4o of tail could be seen in binoculars,
even though the sky was getting bright in the dawn.

     New elements from 26 observations Jan. 28 to Feb. 7:

     T = 1970 Feb. 15.8055 ET         Peri. = 266.6514
                                      Node  =  29.9154  1950.0
     q = 0.065740 AU                  Incl. = 100.1658

1970 TT     R. A. (1950) Decl.     Delta      r    Elong.  Mag.
Feb. 20    22 38.34    - 3 34.4
     21    22 41.65    - 1 16.2    1.162    0.279   11.7    2.5
     22    22 44.49    + 0 48.9
     23    22 47.02    + 2 43.4    1.218    0.356   14.3    4.2

Feb. 28    22 57.16    +10 25.9
Mar.  5    23 05.33    +16 14.0    1.470    0.673   22.7    8.8
     10    23 12.57    +20 55.1
     15    23 19.25    +24 52.5    1.692    0.934   27.7   11.2
     20    23 25.52    +28 19.6
     25    23 31.47    +31 24.9    1.890    1.164   31.6   12.9
     30    23 37.13    +34 14.1
Apr.  4    23 42.53    +36 51.1    2.067    1.374   35.1   14.1
      9    23 47.68    +39 18.7
     14    23 52.56    +41 38.9    2.224    1.570   38.6   15.2
     19    23 57.16    +43 53.3
     24     0 01.46    +46 02.9    2.364    1.755   42.3   16.0
     29     0 05.45    +48 08.9
May   4     0 09.08    +50 11.8    2.487    1.931   46.2   16.8

          Mag. = 10.5 + 5 log Delta + 15 log r


1970 February 13               (2210)              Brian G. Marsden

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