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IAUC 2890: 1975o; 1975q; 1973 EA; NOTICE TO REGULAR SUBSCRIBERS

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                                                  Circular No. 2890
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


PERIODIC COMET GEHRELS 3 (1975o)
     Further positions have been reported as follows:

     1975 UT             R. A. (1950) Decl.        Observer
     Nov. 30.04437     1 34 06.99   +10 30 02.5    Schwartz
     Dec.  7.20903     1 32.32      +10 17.4       Roemer
           7.23264     1 32.31      +10 17.4         "
           8.15354     1 32 08.65   +10 16 03.1    Shao

G. Schwartz and C. Y. Shao (Harvard College Observatory, Agassiz
   Station).  155-cm reflector.  Measurer: Shao.
E. Roemer (Lunar and Planetary Laboratory).  154-cm reflector.

     The following improved elements, by B. G. Marsden, satisfy the
ten available positions within 2":

       T = 1977 Apr. 2.139 ET
   Peri. = 228.807                    e =   0.16925
   Node  = 243.080   1950.0           a =   4.09180 AU
   Incl. =   1.076                    n =   0.119078
       q =   3.39927 AU               P =   8.28 years

     1976 ET     R. A. (1950) Decl.     Delta     r      m2
     Jan.  3     1 33.50    +10 15.8    3.414   3.776   19.4
          13     1 37.03    +10 33.3
          23     1 42.08    +10 59.4    3.688   3.748   19.6
     Feb.  2     1 48.48    +11 32.8
          12     1 56.09    +12 12.4    3.955   3.721   19.7
          22     2 04.76    +12 56.8
     Mar.  3     2 14.37    +13 44.8    4.192   3.695   19.8
          13     2 24.80    +14 35.3
          23     2 35.93    +15 27.1    4.385   3.669   19.9

               m2 = 11.0 + 5 log Delta + 10 log r


COMET SATO (1975q)
     The following  precise positions have been reported:

     1975 UT             R. A. (1950) Decl.        m1    Observer
     Dec. 11.85515    12 19 24.5    + 2 47 39            Hiramatsu
          11.85723    12 19 24.9    + 2 47 16              "
          12.79583    12 20 19.20   - 0 57 21.5          Koishikawa
          12.80382    12 20 20.09   - 0 59 23.8    8.5   Seki
          12.80729    12 20 20.32   - 1 00 17.6            "
          12.82535    12 20 21.07   - 1 04 52.5          Koishikawa
          13.78646    12 21 24.66   - 5 21 21.0            "
          13.82512    12 21 27.04   - 5 32 11.9            "
          13.85191    12 21 29.2    - 5 39 50            Edamatsu
          13.86065    12 21 29.4    - 5 42 15              "
          15.79688    12 24 08.70   -15 46 39.1          Koishikawa
          15.85313    12 24 13.44   -16 05 51.1            "
          15.86597    12 24 14.94   -16 10 17.5    8.3   Seki
          15.87153    12 24 15.46   -16 12 13.8            "

V. Hiramatsu (Hamakita, Shizuoka).  7.5-cm f/4 camera.
M. Koishikawa (Sendai Observatory, Ayashi Station).
T. Seki (Kochi Observatory, Geisei Station).  The times of the Dec.
   15 observations were changed by +5 min.
K. Edamatsu (Sendai Observatory).  7.1-cm f/5.6 camera.

     Selected total visual magnitude estimates: Dec. 13.25 UT, 9.2
(G. M. Hurst, Northampton, England, 26-cm reflector); 14.55, 9.0
(D. Machholz, Concord, California, 25-cm reflector).

     I. Hasegawa, Nara, Japan, has suggested the possibility of
observing meteors associated with the comet on 1976 Jan. 2 from the
radiant R.A. = 195o, Decl. = +47o; V_inf = 54 km/s, r_c - r_e = -0.03 AU.

     Corrigendum.  The observation on Dec. 13.23295 UT (IAUC 2884)
was made by M. R. Dykes, assisted by R. L. Waterfield.


1973 EA
     Recovery observations of this Apollo object have been reported
as follows.  The position is close to that predicted on IAUC 2816.

     1975 UT          R. A. (1950) Decl.      Observer
     Dec.  1.97201   20 49.6     -13 58       McCrosky
           3.98266   20 57.5     -12 28       Schwartz
           4.08333   20 57.78    -12 23.2     Roemer
           4.11389   20 57.90    -12 21.8       "

R. E. McCrosky and G. Schwartz (Harvard College Observatory, Agassiz
   Station).  155-cm reflector.
E. Roemer and M. A. Daniel (University of Arizona).  Steward
   Observatory's 229-cm reflector, Kitt Peak.


NOTICE TO REGULAR SUBSCRIBERS
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Because of the extremely large number of Circulars issued recently,
a subscription can in fact expire only one or two months,
rather than the anticipated four months, after the bill is prepared.


1975 December 29               (2890)              Brian G. Marsden

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