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Circular No. 7733 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) CBAT@CFA.HARVARD.EDU (science) URL http://cfa-www.harvard.edu/iau/cbat.html ISSN 0081-0304 Phone 617-495-7440/7244/7444 (for emergency use only) COMET P/2001 T3 (NEAT) K. Lawrence, S. Pravdo, and E. F. Helin, Jet Propulsion Laboratory, report the discovery by the NEAT program of a comet with a faint coma on CCD images taken with the Palomar 1.2-m Schmidt telescope. The object also appears cometary on CCD images taken by P. Pravec and P. Kusnirak at Ondrejov (moderately condensed coma of diameter 0'.2 on Oct. 14.9 UT) and by J. Ticha, M. Tichy, and P. Jelinek at Klet (diffuse 11" coma on Oct. 14.9; 10" coma and m_1 = 17.0 on Oct. 15.8). 2001 UT R.A. (2000) Decl. m1 Oct. 14.44977 1 45 17.08 - 8 27 56.7 18.4 The available astrometry (including prediscovery data by LINEAR on Oct. 11) and the following orbital elements appear on MPEC 2001-T58. T = 2002 Jan. 27.323 TT Peri. = 354.305 e = 0.60172 Node = 56.739 2000.0 q = 2.52309 AU Incl. = 19.107 a = 6.33492 AU n = 0.061815 P = 15.94 years 2001 TT R. A. (2000) Decl. Delta r Elong. Phase m1 Oct. 8 1 50.03 - 8 39.7 1.727 2.688 159.9 7.3 15.5 18 1 42.54 - 8 18.3 1.696 2.661 161.9 6.7 15.4 28 1 34.72 - 7 38.2 1.690 2.636 157.6 8.3 15.3 Nov. 7 1 27.56 - 6 38.0 1.710 2.613 149.6 11.1 15.3 17 1 21.93 - 5 18.4 1.753 2.593 140.4 14.1 15.4 2001 QT_297 J. L. Elliot, Massachusetts Institute of Technology, reports on follow-up observations of 'Deep Ecliptic Survey Team' discovery targets as part of an ongoing program initiated by Elliot and S. D. Kern at the 6.5-m Baade telescope at Las Campanas: Observations of 2001 QT_297 (MPEC 2001-T38) obtained by D. J. Osip and S. M. Burles using the MagIC instrument on Oct. 11 and 12 UT (with seeing < 0".45 on both nights) reveal this to be a binary system. The fainter member of the pair lies approximately 0".6 from the brighter member at p.a. 240 deg. The brighter member of the pair is only 0.55 magnitude brighter than the companion. Additional photometric and astrometric observations of 2001 QT_297 are strongly encouraged." (C) Copyright 2001 CBAT 2001 October 15 (7733) Daniel W. E. Green
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