• MPC Preparation (Info)

  • MPEC 2003-U56 : 2003 UC20 = 1954 XA

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    M.P.E.C. 2003-U56                                Issued 2003 Oct. 23, 20:16 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 UC20 = 1954 XA
    
                               Revision to MPEC 2003-U55
    
    Additional Observations:
         K03U20C  C2003 10 23.45104 08 37 21.26 +06 32 18.0          17.7        704
         K03U20C  C2003 10 23.46330 08 37 19.74 +06 31 59.8          17.9        704
         K03U20C  C2003 10 23.47577 08 37 18.20 +06 31 40.9          17.9        704
         K03U20C  C2003 10 23.48821 08 37 16.61 +06 31 22.5          17.8        704
    
    Observer details:
    704 Lincoln Laboratory ETS, New Mexico.  Observers M. Blythe, F. Shelly,
        M. Bezpalko, R. Huber, L. Manguso, D. Torres, R. Kracke, M. McCleary,
        H. Stange.  Measurers J. Stuart, R. Sayer, J. Evans, J. Kommers.  1.0-m
        f/2.15 reflector + CCD.
    
    Orbital elements:
    2003 UC20 = 1954 XA
    Epoch 2003 Dec. 27.0 TT = JDT 2453000.5                 MPC
    M 218.46897              (2000.0)            P               Q
    n   1.42796046     Peri.   59.19555     -0.37252920     +0.92796344
    a   0.7810136      Node   188.95082     -0.87243912     -0.35397520
    e   0.3369552      Incl.    3.79162     -0.31634156     -0.11655649
    P   0.69           H   19.2           G   0.15           U   1
    Residuals in seconds of arc
    541205 675  0.1+  0.3+    031022 704  0.4+  0.0     031022 673  0.1+  0.1+
    541205 675  0.1-  0.4+    031022 704  0.3-  0.2-    031022 673  0.1+  0.0
    541205 675  0.6+  0.3+    031022 704  0.3-  0.0     031022 673  0.0   0.0
    541211 675(12.1-  7.3-)   031022 704  0.2+  0.0     031022 673  0.0   0.2+
    541211 675  0.5-  1.1-    031022 704  0.4-  0.4-    031023 704  0.0   0.3+
    031021 704  0.2-  0.3-    031022 704  0.3+  0.0     031023 704  0.0   0.4+
    031021 704  0.0   0.8-    031022 926  0.3+  0.2+    031023 673  0.2+  0.3+
    031021 704  0.2-  0.8-    031022 926  0.1-  0.1-    031023 673  0.6+  0.8+
    031021 704  0.0   0.9-    031022 926  0.5-  0.3-    031023 673  0.7+  0.2+
    031022 704  0.3-  0.4+    031022 704  0.0   0.2+    031023 704  0.2+  0.2+
    031022 704  0.1+  0.3-    031022 673  0.1+  0.2+    031023 704  0.1-  0.5+
    031022 704  0.2+  0.3+    031022 673  0.7-  0.4-
    
    Ephemeris:
    2003 UC20                a,e,i = 0.78, 0.34, 4                   q = 0.5178
    Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase     V
    2003 10 18    08 46.95   +08 38.7    0.171    0.959    72.6    97.6    18.8
    2003 10 28    08 28.60   +04 28.9    0.148    0.994    85.9    85.6    18.0
    2003 11 07    08 03.34   -01 20.0    0.123    1.020   100.0    73.2    17.3
    2003 11 17    07 20.25   -09 33.5    0.100    1.036   115.9    59.1    16.4
    2003 11 27    06 03.19   -19 47.9    0.084    1.044   130.6    45.9    15.7
    2003 12 07    04 15.36   -26 38.6    0.085    1.042   130.0    46.4    15.7
    2003 12 17    02 43.65   -26 24.1    0.101    1.031   115.1    59.8    16.4
    2003 12 27    01 48.67   -23 08.9    0.125    1.011    99.2    73.8    17.3
    2004 01 06    01 16.78   -19 53.0    0.149    0.982    85.1    86.2    18.1
    2004 01 16    00 53.99   -17 19.3    0.171    0.944    71.6    98.5    18.8
    
         The linked orbit above is based upon a successful linkage of the
    1954 and 2003 observations by A. Lowe.  Lowe's solution fitted both
    1954 Nov. 11 observations with residuals of +/- 6".  These observations
    have long been known to be problematic.  The above solution includes one
    of these observations, further observations at the current apparition
    will show whether this choice was justified.
    
    Gareth V. Williams           (C) Copyright 2003 MPC           M.P.E.C. 2003-U56
    

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