Circular No. 5339 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Telephone 617-495-7244/7440/7444 (for emergency use only) TWX 710-320-6842 ASTROGRAM CAM EASYLINK 62794505 MARSDEN or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN COMET McNAUGHT-RUSSELL (1991w) The following precise positions have been reported: 1991 UT R.A. (1950) Decl. m1 Observer Sept. 5.55454 21 54 24.79 - 2 09 36.9 McNaught 6.55718 21 53 53.12 - 2 17 57.9 " 7.63473 21 53 19.22 - 2 26 55.1 18 Seki 7.64827 21 53 18.77 - 2 27 00.9 " 8.60880 21 52 48.86 - 2 35 01.9 McNaught R. H. McNaught (Siding Spring). Uppsala Southern Schmidt. Film dark on Sept. 6. T. Seki (Geisei). 0.6-m reflector. The following parabolic orbital elements, from the nine available observations Sept. 3-8, are rather uncertain, but they suggest that this comet may have a near-record large perihelion distance: T = 1991 Jan. 12.975 ET Peri. = 154.056 Node = 149.352 1950.0 q = 7.11258 AU Incl. = 104.876 1991 ET R.A. (1950) Decl. Delta r m1 Sept. 1 21 56.85 - 1 31.7 6.277 7.266 17.6 11 21 51.59 - 2 54.9 21 21 46.79 - 4 16.8 6.412 7.294 17.7 Oct. 1 21 42.64 - 5 35.5 11 21 39.28 - 6 49.2 6.667 7.323 17.8 21 21 36.84 - 7 56.8 31 21 35.34 - 8 57.6 7.009 7.355 17.9 Nov. 10 21 34.79 - 9 51.2 20 21 35.16 -10 37.6 7.390 7.388 18.0 NOVA SCUTI 1991 Further visual magnitude estimates: Sept. 3.85 UT, 12.1 (P. Schmeer, Bischmisheim, Germany); 4.88, 13.0 (A. Boattini, Florence, Italy); 5.47, 12.6 (P. Camilleri, Cobram, Victoria, Australia); 5.85, 13.1 (M. Tombelli, Montelupo, Italy); 6.41, 12.5 (A. F. A. L. Jones, Nelson, New Zealand). 1991 September 9 (5339) Brian G. Marsden
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