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IAUC 3941: 1983v; Poss. Occn BY SATURNIAN MAGNETOSPHERIC RING; Z And

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                                                  Circular No. 3941
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 617-495-7244/7440/7444


PERIODIC COMET HARTLEY-IRAS (1983v)
     Ephemeris from the elements on MPC 8672:

     1984 ET     R.A. (1950.0) Decl.      p        r       m1

     Apr. 10    19 34.9     +71 00.8    1.635    1.777    10.1
          20    17 44.5     +77 42.5
          30    14 34.6     +77 49.4    1.718    1.954    10.6
     May  10    12 46.2     +71 40.5
          20    12 05.41    +64 10.0    1.957    2.138    11.3
          30    11 49.24    +57 00.3
     June  9    11 43.40    +50 35.1    2.314    2.325    12.0
          19    11 42.67    +44 57.1
          29    11 44.82    +40 01.9    2.731    2.512    12.7
     July  9    11 48.73    +35 43.3
          19    11 53.76    +31 55.8    3.157    2.698    13.3
          29    11 59.54    +28 34.0
     Aug.  8    12 05.83    +25 33.8    3.557    2.881    13.9
          18    12 12.42    +22 51.9
          28    12 19.21    +20 25.5    3.902    3.062    14.3

     Total visual magnitude estimate by C. E. Spratt, Victoria, BC
(0.20-m reflector): Apr. 22.21 UT, 10.2.


POSSIBLE OCCULTATION BY SATURNIAN MAGNETOSPHERIC RING
     J. C. Bhattacharyya, Indian Institute of Astrophysics, Bangalore,
reports that observations by Santhanam and Rozario with the
1-m telescope at Kavalur indicate systematic extinction of SAO
158913 on March 24 and 25, apparently in accordance with the
prediction by Mink (1983, A.J. 88, 559) of occultations of the star
by the supposed magnetospheric ring at 14 radii from the center of
Saturn.  Observations on Mar. 24 in integrated light showed two
prominent and several smaller and narrow absorbing features beween
20h14m and 20h20m UT, the maximum extinction being 0.58 mag.
Observations on Mar. 25 using a B filter showed similar structures
between 20h18m and 20h24m with a maximum extinction of 0.28 mag.


Z ANDROMEDAE
     Visual magnitudes: Mar. 30.5 UT, 9.8 (J. Morgan, Prescott,
AZ); Apr. 2.4, 9.7 (J. Bortle, Stormville, NY); 9.4, 9.7 (Bortle).


1984 April 25                  (3941)              Brian G. Marsden

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