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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