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Circular No. 6894 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) BMARSDEN@CFA.HARVARD.EDU or DGREEN@CFA.HARVARD.EDU (science) URL http://cfa-www.harvard.edu/iau/cbat.html Phone 617-495-7244/7440/7444 (for emergency use only) COMET C/1998 J1 (SOHO) C. St. Cyr, Naval Research Laboratory, on behalf of the SOHO-LASCO Consortium (cf. IAUC 6685), reports the discovery by S. Stezelberger of a bright comet in the northwestern corner of the field of view of the C3 coronagraph, some 8 deg from the sun: 1998 UT R.A. (2000) Decl. May 3.779 2 10.2 +19 35 Preliminary measurements by Stezelberger and St. Cyr, reduced by G. V. Williams and given on MPEC 1998-J13, show the comet, estimated by St. Cyr at mag 0 and possibly brighter, continuing to move across the top of the C3 field. There is a fanshaped tail extending antisunward at least to the edge of the field, and there may be a separate narrow tail extending roughly along the direction of motion. Computations by the undersigned show that the observations are represented rather unequivocally by the following parabolic orbital elements and suggest that the comet might become observable from the ground, particularly later in the month at solar elongations favoring the southern hemisphere. T = 1998 May 8.901 TT Peri. = 107.577 Node = 348.442 2000.0 q = 0.17454 AU Incl. = 55.085 1998 TT R. A. (2000) Decl. Delta r Elong. Phase m1 May 5 2 23.55 +21 24.8 1.190 0.234 7.7 35.4 0.1 6 2 35.00 +22 50.6 1.165 0.211 7.5 38.6 -0.4 7 2 47.69 +24 06.1 1.137 0.191 7.6 44.3 -0.9 8 3 01.57 +25 04.1 1.107 0.178 8.1 52.9 -1.3 9 3 16.29 +25 37.0 1.075 0.175 8.9 63.6 -1.4 10 3 31.27 +25 40.0 1.042 0.180 9.9 74.8 -1.4 11 3 45.90 +25 13.5 1.010 0.194 11.0 84.5 -1.1 12 3 59.81 +24 22.3 0.980 0.215 12.3 91.9 -0.7 13 4 12.86 +23 12.2 0.953 0.239 13.6 96.9 -0.3 14 4 25.07 +21 48.3 0.930 0.266 15.0 100.0 0.1 15 4 36.54 +20 14.3 0.910 0.294 16.6 101.6 0.5 16 4 47.35 +18 33.2 0.892 0.323 18.2 102.2 0.8 17 4 57.60 +16 47.0 0.878 0.352 19.9 101.9 1.2 (C) Copyright 1998 CBAT 1998 May 5 (6894) Brian G. Marsden
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