Printer-friendly version

IAU Minor Planet Center

Minor Planet Center

MPEC 2005-U104: 2004 UW10

The following Minor Planet Electronic Circular may be linked-to from your own Web pages, but must not otherwise be redistributed electronically.


Read MPEC 2005-U103 Read MPEC 2005-U105


M.P.E.C. 2005-U104                               Issued 2005 Oct. 31, 22:37 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 Brinson Foundation
                  Supported in part by the TABASGO Foundation
             Prepared using the Tamkin Foundation Computer Network

                              MPC@CFA.HARVARD.EDU
          URL http://cfa-www.harvard.edu/iau/mpc.html  ISSN 1523-6714

                                   2004 UW10

Observations:
     K04U10W* C2004 10 17.17365 01 05 17.02 +05 20 42.3                 EU104304
     K04U10W  C2004 10 17.21834 01 05 16.74 +05 20 40.6                 EU104304
     K04U10W  C2004 10 17.26304 01 05 16.47 +05 20 39.1                 EU104304
     K04U10W 5C2004 12 12.31346 01 01 06.10 +04 58 33.6          25   R EU104568
     K04U10W 5C2004 12 13.32341 01 01 04.28 +04 58 28.6                 EU104568
     K04U10W 5C2004 12 14.31742 01 01 02.71 +04 58 23.6                 EU104568

Observer details:
304 Las Campanas Observatory.  Observers S. S. Sheppard, C. Trujillo.
    Measurer S. S. Sheppard.  6.5-m Baade reflector + CCD.
568 Mauna Kea.  Observers S. S. Sheppard, D. C. Jewitt.  Measurer
    S. S. Sheppard.  8.3-m Subaru reflector + CCD.

Orbital elements:
2004 UW10
Eccentricity assumed
Epoch 2004 Nov. 11.0 TT = JDT 2453320.5                 MPC
M   0.09939              (2000.0)            P               Q
n   0.00397722     Peri.  341.96806     +0.95434074     -0.29506141
a  39.4532760      Node    35.30055     +0.28304305     +0.84329671
e   0.2490847      Incl.    4.62647     +0.09550070     +0.44920977
P 248              H   10.5           G   0.15
From 6 observations 2004 Oct. 17-Dec. 14.

Ephemeris:
2004 UW10                a,e,i = 39.45, 0.25, 5                  q = 29.626
Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase     V
2005 10 27    01 13.58   +06 24.9   28.668   29.632   165.8     0.5    25.2
2005 11 06    01 12.62   +06 19.6   28.727   29.632   155.5     0.8    25.3
2005 11 16    01 11.76   +06 14.9   28.815   29.633   145.3     1.1    25.3
2005 11 26    01 11.03   +06 11.1   28.927   29.633   135.0     1.4    25.4
2005 12 06    01 10.46   +06 08.4   29.061   29.633   124.7     1.6    25.4
2005 12 16    01 10.08   +06 06.8   29.213   29.634   114.4     1.7    25.4
2005 12 26    01 09.90   +06 06.5   29.377   29.634   104.2     1.8    25.4
2006 01 05    01 09.93   +06 07.5   29.549   29.634    94.0     1.9    25.4
2006 01 15    01 10.19   +06 09.9   29.723   29.635    83.9     1.9    25.5
2006 01 25    01 10.66   +06 13.5   29.893   29.635    73.9     1.8    25.5
2006 02 04    01 11.33   +06 18.4   30.056   29.636    63.9     1.7    25.5
2006 02 14    01 12.19   +06 24.3   30.205   29.636    54.0     1.5    25.5
2006 02 24    01 13.21   +06 31.2   30.338   29.636    44.2     1.3    25.5
2006 03 06    01 14.38   +06 38.9   30.449   29.637    34.5     1.1    25.4

     The assumed perihelic 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 2005 MPC           M.P.E.C. 2005-U104

Read MPEC 2005-U103 Read MPEC 2005-U105


Our Web policy. Index to the CBAT/MPC/ICQ pages.


Valid HTML 4.01!