MPEC 2003-W02 : 2003 VS2
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M.P.E.C. 2003-W02 Issued 2003 Nov. 16, 14:50 UT The Minor Planet Electronic Circulars contain information on unusual minor planets and routine data on comets. They are published on behalf of Commission 20 of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Supported in part by the Steven and Michele Kirsch Foundation Prepared using the Tamkin Foundation Computer Network MPC@CFA.HARVARD.EDU URL http://cfa-www.harvard.edu/iau/mpc.html ISSN 1523-6714 2003 VS2 Observations: K03V02S C1998 11 16.45070 02 35 50.61 +30 48 00.5 18.7 R 566 K03V02S C2001 09 21.39082 03 04 47.97 +32 13 27.7 18.9 R 644 K03V02S C2001 09 21.41215 03 04 47.93 +32 13 27.5 19.4 R 644 K03V02S C2001 09 21.43354 03 04 47.84 +32 13 27.8 19.8 R 644 K03V02S C2002 01 05.11977 02 55 40.03 +31 35 32.7 19.6 R 644 K03V02S C2002 01 05.14249 02 55 39.99 +31 35 31.6 19.6 R 644 K03V02S C2002 10 13.46083 03 11 14.21 +32 33 11.0 18.9 R 644 K03V02S C2002 10 13.47132 03 11 14.18 +32 33 11.0 19.0 R 644 K03V02S C2002 10 13.48171 03 11 14.11 +32 33 11.1 19.2 R 644 K03V02S C2002 11 13.39655 03 08 08.40 +32 24 59.7 19.5 V 644 K03V02S C2002 11 13.42199 03 08 08.21 +32 24 59.6 19.4 V 644 K03V02S C2002 11 13.44322 03 08 08.09 +32 24 58.9 19.6 V 644 K03V02S C2002 11 25.37731 03 06 53.47 +32 19 41.1 19.4 V 644 K03V02S C2002 11 25.40656 03 06 53.23 +32 19 39.8 18.9 V 644 K03V02S C2002 11 25.43196 03 06 53.09 +32 19 39.3 20.1 V 644 K03V02S C2002 12 03.39188 03 06 05.72 +32 15 39.1 20.0 V 644 K03V02S C2002 12 03.41352 03 06 05.57 +32 15 38.9 19.5 V 644 K03V02S C2002 12 03.44380 03 06 05.36 +32 15 37.8 20.3 V 644 K03V02S* C2003 11 14.46332 03 16 12.12 +32 43 50.5 19.2 644 K03V02S C2003 11 14.48460 03 16 11.99 +32 43 50.0 19.3 644 K03V02S C2003 11 14.50581 03 16 11.86 +32 43 49.9 19.5 644 K03V02S C2003 11 15.01553 03 16 08.64 +32 43 37.7 18.9 R 176 K03V02S C2003 11 15.09468 03 16 08.11 +32 43 35.4 19.2 R 176 K03V02S C2003 11 15.22176 03 16 07.32 +32 43 33.0 18.5 R 673 K03V02S C2003 11 15.23889 03 16 07.25 +32 43 32.5 673 K03V02S C2003 11 15.28750 03 16 06.93 +32 43 31.4 673 K03V02S C2003 11 15.30139 03 16 06.76 +32 43 30.8 673 K03V02S C2003 11 15.46269 03 16 05.75 +32 43 27.5 18.9 644 K03V02S C2003 11 15.46476 03 16 05.76 +32 43 26.8 19.3 R 926 K03V02S C2003 11 15.48171 03 16 05.63 +32 43 26.8 19.4 R 926 K03V02S C2003 11 15.48324 03 16 05.60 +32 43 26.7 19.0 644 K03V02S C2003 11 15.50370 03 16 05.49 +32 43 26.1 19.1 644 K03V02S C2003 11 15.82404 03 16 03.49 +32 43 18.8 557 K03V02S C2003 11 15.87407 03 16 03.18 +32 43 18.2 246 K03V02S C2003 11 15.87752 03 16 03.15 +32 43 18.0 246 K03V02S C2003 11 15.88185 03 16 03.12 +32 43 17.0 246 K03V02S C2003 11 15.88458 03 16 03.07 +32 43 17.6 246 K03V02S C2003 11 15.88905 03 16 03.06 +32 43 17.4 246 K03V02S C2003 11 15.91299 03 16 02.84 +32 43 17.2 557 K03V02S C2003 11 16.24120 03 16 00.81 +32 43 08.9 19.1 R 926 K03V02S C2003 11 16.29057 03 16 00.49 +32 43 07.8 19.5 R 926 K03V02S C2003 11 16.33203 03 16 00.20 +32 43 06.3 19.2 R 926 Observer details: 176 Observatori Astronomic de Consell. Observers A. Lopez, R. Pacheco. 0.41-m f/4 reflector + CCD. 246 Klet Observatory-KLENOT. Observers J. Ticha, M. Tichy. 1.06-m KLENOT Telescope + CCD. 557 Ondrejov. Observer P. Kusnirak. 0.65-m f/3.6 reflector + CCD. 566 Haleakala-NEAT/GEODSS. Observers R. Byrd, A. Esquibel, C. Cotton, D. Bascon. Measurer S. Hoenig. 1.2-m reflector + CCD. 644 Palomar Mountain/NEAT. Observers S. Pravdo, D. MacDonald, K. Lawrence, M. Hicks, R. Bambery, E. Helin, R. Thicksten, E. F. Helin, K. Kuluhiwa. Measurers NEAT Team, M. Meyer, S. Hoenig. 1.2-m Schmidt + CCD. 673 Table Mountain Observatory, Wrightwood. Observer J. Young. 0.6-m reflector + CCD. 926 Tenagra II Observatory. Observers P. R. Holvorcem, M. Schwartz. 0.81-m f/7 Ritchey-Chretien + CCD. Orbital elements: 2003 VS2 Epoch 2003 Dec. 27.0 TT = JDT 2453000.5 MPC M 358.13099 (2000.0) P Q n 0.00397286 Peri. 114.10658 +0.51969341 -0.82705899 a 39.4821468 Node 302.86543 +0.66158808 +0.54823373 e 0.0772304 Incl. 14.77627 +0.54057374 +0.12414996 P 248 H 3.9 G 0.15 U 3 Residuals in seconds of arc 981116 566 0.1- 0.3- 021125 644 0.2- 0.4- 031115 926 0.2+ 0.4- 010921 644 0.1- 0.2+ 021203 644 0.2+ 0.5- 031115 926 0.0 0.0 010921 644 0.4+ 0.1- 021203 644 0.2- 0.0 031115 644 0.3- 0.1- 010921 644 0.2+ 0.0 021203 644 0.6- 0.1- 031115 644 0.0 0.2- 020105 644 0.0 1.1+ 031114 644 0.3- 0.1+ 031115 557 0.3+ 0.0 020105 644 0.3+ 0.7+ 031114 644 0.2- 0.1+ 031115 246 0.4+ 0.6+ 021013 644 0.1- 0.1- 031114 644 0.1- 0.5+ 031115 246 0.3+ 0.5+ 021013 644 0.2+ 0.1- 031115 176 0.2+ 0.0 031115 246 0.3+ 0.4- 021013 644 0.0 0.1+ 031115 176 0.0 0.4- 031115 246 0.1- 0.2+ 021113 644 0.1- 0.4- 031115 673 0.0 0.1+ 031115 246 0.1+ 0.1+ 021113 644 0.4- 0.1+ 031115 673 0.6+ 0.0 031115 557 0.7- 0.5+ 021113 644 0.2- 0.0 031115 673 0.5+ 0.0 031116 926 0.1+ 0.1- 021125 644 0.3+ 0.2- 031115 673 0.5- 0.3- 031116 926 0.1+ 0.0 021125 644 0.4- 0.6- 031115 644 0.1- 0.2+ 031116 926 0.2- 0.6- Ephemeris: 2003 VS2 a,e,i = 39.48, 0.08, 15 q = 36.433 Date TT R. A. (2000) Decl. Delta r Elong. Phase V 2003 11 07 03 16.99 +32 46.5 35.492 36.435 161.9 0.5 19.6 2003 11 17 03 15.93 +32 42.8 35.475 36.435 165.9 0.4 19.5 2003 11 27 03 14.88 +32 38.5 35.489 36.435 163.2 0.4 19.6 2003 12 07 03 13.89 +32 33.6 35.532 36.435 156.1 0.6 19.6 2003 12 17 03 12.99 +32 28.3 35.604 36.435 147.2 0.8 19.6 2003 12 27 03 12.21 +32 22.7 35.701 36.435 137.7 1.0 19.6 2004 01 06 03 11.60 +32 17.3 35.822 36.435 128.0 1.2 19.7 2004 01 16 03 11.18 +32 12.0 35.961 36.435 118.1 1.4 19.7 2004 01 26 03 10.96 +32 07.2 36.115 36.435 108.2 1.5 19.7 2004 02 05 03 10.96 +32 02.9 36.278 36.435 98.4 1.5 19.7 2004 02 15 03 11.17 +31 59.3 36.446 36.434 88.6 1.6 19.7 2004 02 25 03 11.59 +31 56.6 36.613 36.434 78.8 1.5 19.7 2004 03 06 03 12.21 +31 54.8 36.775 36.434 69.2 1.5 19.7 2004 03 16 03 13.02 +31 53.9 36.926 36.434 59.7 1.4 19.7 2004 03 26 03 14.00 +31 54.0 37.062 36.434 50.4 1.2 19.7 2004 04 05 03 15.11 +31 55.0 37.180 36.434 41.3 1.0 19.7 2004 04 15 03 16.34 +31 56.9 37.277 36.434 32.4 0.8 19.7 The key precovery observations from Nov.-Dec. 2002 were found by M. Meyer and then the observations from Oct. 2002 and earlier were found by S. Hoenig from the information supplied about the 2003 discovery on The NEO Confirmation Page. The 2:3 Neptune-resonance orbit keeps the object more than 13 AU from Neptune over a 14 000-year period. Brian G. Marsden (C) Copyright 2003 MPC M.P.E.C. 2003-W02


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