Circular No. 3283 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 617-864-5758 COMET SEARGENT (1978m) D. Herald, Kambah, near Canberra, provides the following precise positions, obtained with a 31-cm reflector: 1978 UT R. A. (1950) Decl. Oct. 2.75295 11 54 46.75 -38 44 56.6 2.76076 11 54 46.16 -38 45 41.2 2.78080 11 54 44.89 -38 47 37.8 4.73259 11 52 24.34 -41 56 54.9 4.76896 11 52 21.84 -42 00 30.6 The following parabolic orbital elements have been calculated. The ephemeris is from the first set. M. P. Candy B. G. Marsden (> 3 obs. Oct. 2-4) (5 obs. Oct. 2 & 4) T = 1978 Sept. 14.654 1978 Sept. 15.16 ET Peri. = 205.60 211.32 Node = 41.40 40.51 1950.0 Incl. = 68.63 66.51 q = 0.3683 0.3725 AU 1978 ET R. A. (1950) Decl. Delta r m1 Sept.29 11 58.88 -32 47.2 1.001 0.537 5.8 Oct. 4 11 53.25 -40 46.1 9 11 46.54 -49 04.4 0.871 0.734 6.9 14 11 37.39 -57 56.2 19 11 21.75 -67 24.2 0.787 0.932 7.7 24 10 42.8 -77 11.3 29 7 18 -85 04.4 0.772 1.124 8.4 m1 = 8.5 + 5 log Delta + 10 log r Visual magnitude estimate by B. Sumner, Perth, Australia (9 x 65 binoculars): Oct. 3.84 UT, 6.4, tail 2o long in p.a. ~ 180o. V533 HERCULIS J. Patterson, McDonald Observatory, writes that photoelectric observations from July 28 through Sept. 14 reveal the presence of strictly periodic oscillations in this old 1963 nova. The period is 63s.63303 +/- 0s.00003, the amplitude 2 percent in unfiltered light. 1978 October 6 (3283) Brian G. Marsden
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