Circular No. 3516 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 CERNIS-PETRAUSKAS (1980k) An exposure of this comet on Aug. 29.14 UT by E. Everhart, University of Denver, shows a very conspicuous, straight, narrow antitail, 14' in length. The earth crossed the comet's orbit plane on Sept. 2.7 UT. Z. Sekanina, Harvard-Smithsonian Center for Astrophysics, remarks: "At the time of observation the earth was less than 2o from the comet's orbit plane. The antitail is measured to be in p.a. 257o +/- 1o (or 4o.5 from the direction to the sun), suggesting a broad range of emission times from 120 to 10 days before perihelion (i.e., at heliocentric distances from 2.3 to 0.6 AU). The observed length of the antitail indicates the maximum radiation-pressure effect on the dust particles to be between 0.25 and 0.55 percent of the solar attraction and the corresponding minimum particle size to be on the order of several tenths of 1 mm." Further precise positions have been reported as follows: 1980 UT R. A. (1950) Decl. m1 Observer Sept. 1.46562 14 19 08.51 +26 44 44.0 14.5 Seki 6.84549 14 37 54.52 +25 20 31.7 Grossmann 7.82535 14 41 11.84 +25 05 10.9 " T. Seki (Geisei). From Japan Astron. Circ. No. 249. M. Grossmann and S. Wagner. Hoher List Observatory). Improved parabolic orbital elements by the undersigned: T = 1980 June 22.4420 ET Peri. = 337.8131 Node = 159.9275 1950.0 q = 0.523208 AU Incl. = 49.0733 1980 ET R. A. (1950) Decl. Delta r m1 Sept.28 15 39.71 +20 12.3 Oct. 8 16 04.06 +18 09.5 2.537 2.089 15.2 18 16 26.26 +16 24.3 28 16 46.73 +14 56.8 2.919 2.374 16.1 Nov. 7 17 05.79 +13 46.5 17 17 23.67 +12 52.8 3.288 2.648 16.8 27 17 40.48 +12 14.8 Dec. 7 17 56.35 +11 51.5 3.627 2.910 17.4 17 18 11.31 +11 42.1 27 18 25.39 +11 45.5 3.918 3.164 18.0 1980 September 22 (3516) Brian G. Marsden
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