Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 2768: P/PERRINE-MRKOS; 1975d

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 2767  SEARCH Read IAUC 2769
IAUC number


                                                  Circular No. 2768
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 PERRINE-MRKOS
     The prediction below, by B. G. Marsden, is from an orbit
fitted to observations at the 1962 and 1968 returns, with perturbations
by all nine planets taken into account.  Although the prediction
by R. Luss in Handb. Br. Astron. Assoc. for 1975 is very similar,
the comet's past behavior suggests that a large Delta-T correction
is not improbable.

       T = 1975 Aug. 2.8779 ET    Epoch = 1975 Aug. 16.0 ET
   Peri. = 166.4950                   e =   0.638226
   Node  = 239.9074   1950.0          a =   3.580887 AU
   Incl. =  17.8103                   n =   0.1454515
       q =   1.29547 AU               P =   6.776 years
                                                        For dT = +1d
     1975 ET     R. A. (1950) Decl.     Delta     r     dR.A.  dDecl.   m2
     May   8     0 08.87    +14 27.9    2.279   1.643   -1m65  - 5'9   20.5
          18     0 38.51    +17 17.3                    -1.82  - 5.4
          28     1 10.21    +19 59.9    2.089   1.517   -1.99  - 4.5   19.8
     June  7     1 44.13    +22 28.8                    -2.15  - 3.2
          17     2 20.26    +24 36.0    1.936   1.411   -2.31  - 1.3   19.2
          27     2 58.36    +26 13.1                    -2.42  + 1.0
     July  7     3 37.98    +27 12.7    1.827   1.335   -2.49  + 3.7   18.7
          17     4 18.35    +27 29.3                    -2.48  + 6.5
          27     4 58.54    +27 00.6    1.760   1.298   -2.41  + 9.1   18.4
     Aug.  6     5 37.64    +25 48.0                    -2.28  +11.3
          16     6 14.86    +23 56.4    1.727   1.305   -2.11  +12.9   18.4
          26     6 49.64    +21 32.5                    -1.92  +13.8
     Sept. 5     7 21.72    +18 44.0    1.714   1.355   -1.73  +14.1   18.6
          15     7 50.96    +15 38.4                    -1.56  +13.8
          25     8 17.39    +12 22.4    1.706   1.441   -1.42  +13.1   19.0
     Oct.  5     8 41.12    + 9 01.4                    -1.30  +12.1
          15     9 02.18    + 5 39.7    1.690   1.555   -1.21  +10.9   19.5
          25     9 20.65    + 2 20.9                    -1.14  + 9.6
     Nov.  4     9 36.51    - 0 52.5    1.657   1.686   -1.10  + 8.3   20.0
          14     9 49.68    - 3 58.0                    -1.08  + 7.0
          24    10 00.04    - 6 53.1    1.604   1.828   -1.09  + 5.8   20.5
     Dec.  4    10 07.40    - 9 35.2                    -1.12  + 4.7
          14    10 11.50    -12 00.8    1.540   1.976   -1.18  + 3.9   20.9

            m2 = 15.5 + 5 log Delta + 15 log r

     The total magnitude m1 could reach 15 in July or August.


COMET BRADFIELD (1975d)
     Mr. D. Herald, Woden, near Canberra, provides the following
precise positions.  He remarks that the comet has a fanshaped tail
and that a condensation of m2 ~ 12 was apparent after April 3.

     1975 UT             R. A. (1950) Decl.        m1
     Mar. 30.39757     2 19 09.83   -19 19 36.5
          30.39931     2 19 10.28   -19 19 35.6
     Apr.  3.39097     2 36 35.41   -18 26 37.1
           3.39792     2 36 36.90   -18 26 33.4
           4.38924     2 40 59.23   -18 12 28.0
           4.39167     2 41 00.46   -18 12 28.8
           6.40556     2 49 55.82   -17 42 47.2    9.0
           6.40903     2 49 56.81   -17 42 48.7

     The following parabolic elements, by the undersigned, are from
12 observations Mar. 13 to Apr. 6:

       T = 1975 Apr. 4.632 ET    Peri. = 264.182
                                 Node  = 157.236   1950.0
       q = 1.21632 AU            Incl. =  55.262

     1975 ET     R. A. (1950) Decl.     Delta     r      m1
     Apr. 18     3 42.17    -14 26.6    1.838   1.234    8.7
          23     4 04.74    -12 51.2
          28     4 27.10    -11 11.9    1.850   1.269    8.9
     May   3     4 49.07    - 9 30.7
           8     5 10.53    - 7 49.9    1.898   1.322    9.1
          13     5 31.37    - 6 11.3
          18     5 51.50    - 4 36.8    1.979   1.388    9.4
          23     6 10.85    - 3 07.7
          28     6 29.39    - 1 45.0    2.088   1.466    9.8
     June  2     6 47.13    - 0 29.3
           7     7 04.07    + 0 39.1    2.220   1.553   10.1
          12     7 20.23    + 1 40.2
          17     7 35.64    + 2 34.2    2.368   1.647   10.5
          22     7 50.34    + 3 21.4
          27     8 04.36    + 4 02.2    2.524   1.746   10.9

                m1 = 6.5 + 5 log Delta + 10 log r

     Mr. T. B. Tregaskis, Mount Eliza, Victoria, writes that on
Mar. 22.424 UT he observed the comet at total magnitude about 9.5
(using a 32-cm reflector at 150 x).  The comet was very faint,
diffuse, 2' in diameter, round, with very slight condensation (less
than on Mar. 13) and no tail.


1975 April 15                  (2768)              Brian G. Marsden

Read IAUC 2767  SEARCH Read IAUC 2769


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


Valid HTML 4.01!