Circular No. 3028 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 Telex: 921428 Telephone: (617) 864-5758 1976 UA The following improved orbital elements, by B. G. Marsden, are based on 31 observations 1976 Oct. 22 to Nov. 27. Perturbations by all nine planets were taken into account. T = 1976 Aug. 10.8416 ET Epoch = 1976 Oct. 29.0 ET Peri. = 39.5777 e = 0.449832 Node = 211.2326 1950.0 a = 0.844007 AU Incl. = 5.8517 n = 1.271116 q = 0.464345 AU P = 0.775 year The object's closest approach to the earth (separation 0.00779 AU) occurred on 1976 Oct. 20.7 UT. Although the object is so faint, its orbit is quite well determined, and it can be expected that the object will be recovered on its approaches within 0.178 AU in Jan. 1981 and 0.116 AU in Oct. 1983 (not 1982 as was indicated in some publications); it will pass 0.029 AU from Mercury in June 1980. COMET MORI-SATO-FUJIKAWA (1975j) The following improved orbital elements were determined by the undersigned from 177 observations 1975 Oct. 6 to 1976 Sept. 20, perturbations by all nine planets being taken into account. Epoch = 1975 Dec. 14.0 ET T = 1975 Dec. 25.8774 ET Peri. = 246.2475 e = 0.997450 Node = 277.9800 1950.0 q = 1.603933 AU Incl. = 91.6061 1977 ET R. A. (1950) Decl. Delta r m2 Feb. 6 19 03.10 -25 22.7 5.738 4.936 19.2 16 19 08.41 -24 40.2 26 19 12.84 -23 58.7 5.690 5.114 19.4 Mar. 8 19 16.29 -23 18.2 18 19 18.65 -22 38.8 5.569 5.291 19.5 28 19 19.81 -22 00.6 Apr. 7 19 19.70 -21 23.8 5.406 5.467 19.5 17 19 18.25 -20 48.3 27 19 15.44 -20 14.2 5.239 5.640 19.6 May 7 19 11.28 -19 41.3 17 19 05.86 -19 09.7 5.111 5.812 19.7 27 18 59.34 -18 39.2 June 6 18 51.97 -18 09.7 5.068 5.983 19.8 16 18 44.04 -17 41.4 26 18 35.91 -17 14.4 5.143 6.152 19.9 July 6 18 27.93 -16 49.0 16 18 20.45 -16 25.4 5.351 6.319 20.1 26 18 13.76 -16 04.0 Aug. 5 18 08.07 -15 44.8 5.683 6.485 20.4 m2 = 8.5 + 5 log Delta + 10 log r PERIODIC COMET DU TOIT-NEUJMIN-DELPORTE The following predicted elements, by B. G. Marsden, were derived by extending the 1970 prediction forward, perturbations by all nine planets being taken into account. There is no possibility of observing the comet at this return T = 1977 Jan. 31.3759 ET Epoch = 1977 Jan. 17.0 ET Peri. = 115.9120 e = 0.508457 Node = 187.7691 1950.0 a = 3.414703 AU Incl. = 2.8639 n = 0.1561977 q = 1.678472 AU P = 6.310 years PERIODIC COMET KLEMOLA (1976j) The following precise positions have been reported: 1976 UT R. A. (1950) Decl. m1 Observer Sept.16.54965 23 03 51.91 - 0 57 13.6 13 Suzuki 17.55556 23 03 58.52 - 1 11 06.0 13 " 19.24444 23 04 10.97 - 1 34 04.3 Roemer 19.23542 23 04 10.93 - 1 33 57.0 " K. Suzuki (JCPM Oi Station). From Nihondaira Obs. Circ. No. 806. E. Roemer and L. M. Vaughn (Steward Observatory, KItt Peak). 229-cm reflector. Measurer: C. D. Vesely. COMET BRADFIELD (1975p) The following precise positions, obtained by L. V. Yurevich and D. I. Gorodetsklj at Alma-Ata, are from Kiev Komet. Tsirk. No. 199. Measurers: K. I. Churyumov, Yurevich and L. A. Drach. 1976 UT R. A. (1950) Decl. Jan. 31.63699 22 24 51.18 +36 47 39.0 31.64357 22 24 53.32 +36 47 57.9 Feb. 1.61941 22 31 17.26 +37 24 13.2 1.63309 22 31 22.14 +37 24 37.4 1977 January 17 (3028) Brian G. Marsden
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