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  • MPEC 2019-T136 : S/2004 S 29

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    M.P.E.C. 2019-T136                              Issued 2019 October 7, 18:12 UT
    
         The Minor Planet Electronic Circulars contain information on unusual
             minor planets and routine data on comets.  They are published
        on behalf of Division F of the International Astronomical Union by the
              Minor Planet Center, Smithsonian Astrophysical Observatory,
                              Cambridge, MA 02138, U.S.A.
    
                 Prepared using the Tamkin Foundation Computer Network
    
                                  MPC@CFA.HARVARD.EDU
                URL https://www.minorplanetcenter.net/    ISSN 1523-6714
    
                                   S/2004 S 29                               
    
    
    Observations:
        SK04S290* C2004 12 12.43730 07 50 58.570+21 03 14.83         24.4 RcET136568
        SK04S290  C2004 12 12.49310 07 50 57.684+21 03 16.99               cET136568
        SK04S290  C2004 12 14.59914 07 50 23.597+21 04 39.15               cET136568
        SK04S290  C2004 12 14.63843 07 50 22.942+21 04 40.80               cET136568
        SK04S290  C2005 01 05.59973 07 43 18.153+21 21 21.56         25.2 RcET136568
        SK04S290  C2005 01 05.62207 07 43 17.689+21 21 22.75               cET136568
        SK04S290  C2005 02 07.41846 07 31 59.958+21 45 34.66               cET136568
        SK04S290  C2005 02 07.43404 07 31 59.667+21 45 35.25               cET136568
        SK04S290  C2005 02 08.33118 07 31 43.823+21 46 06.66               cET136568
        SK04S290  C2005 02 08.37024 07 31 43.109+21 46 08.00               cET136568
        SK04S290  C2005 03 05.36304 07 26 18.961+21 56 09.23               cET136568
        SK04S290  C2005 03 05.39380 07 26 18.707+21 56 09.64               cET136568
        SK04S290  C2005 03 09.34132 07 25 52.000+21 56 52.51               cET136568
        SK04S290  C2005 03 09.37347 07 25 51.789+21 56 52.68               cET136568
        SK04S290  C2005 03 11.24888 07 25 41.754+21 57 08.08         25.1 RcET136568
        SK04S290  C2005 03 11.34101 07 25 41.280+21 57 08.70         24.8 RcET136568
        SK04S290  C2006 01 05.60628 08 51 20.405+18 50 28.37         25.8 RcET136568
        SK04S290  C2006 01 05.66257 08 51 19.450+18 50 32.85               cET136568
        SK04S290  C2007 01 16.39014 09 45 54.080+15 03 34.59         25.2 RcET136568
        SK04S290  C2007 01 16.40820 09 45 53.772+15 03 35.72               cET136568
        SK04S290  C2007 01 16.42270 09 45 53.520+15 03 37.35               cET136568
        SK04S290  C2007 01 17.42015 09 45 36.798+15 05 04.51               cET136568
    
    Observer details:
    568 Mauna Kea.  Observers S. S. Sheppard, D. C. Jewitt, J. Kleyna.  Measurers 
       S. S. Sheppard, B. Marsden.  8.2-m reflector + CCD, 10-m Keck + CCD.
    
    Orbital elements:
    S/2004 S 29
    Epoch 2019 Apr. 27.0 TT = JDT 2458600.5                 Williams
    M 341.97044              (2000.0)            P               Q
    n   0.43573766     Peri.  339.34541     -0.56606656     -0.69141989
    a   0.1135142      Node   140.67546     +0.82014590     -0.52734028
    e   0.4401244      Incl.   45.10152     +0.08324271     +0.49381248
    P   2.26           H   15.8           P/d   826.19
    From 22 observations 2004 Dec. 12-2007 Jan. 17, mean residual 0".25.
    
    Residuals in seconds of arc
    041212 568  0.2+  0.1+    050208 568  0.1+  0.1-    060105 568  0.1+  0.2+
    041212 568  0.5+  0.1+    050208 568  0.0   0.1-    060105 568  0.1-  0.1-
    041214 568  0.0   0.2-    050305 568  0.1+  0.1-    070116 568  0.3+  0.0
    041214 568  0.1+  0.1-    050305 568  0.0   0.1-    070116 568  0.2+  0.4-
    050105 568  0.4-  0.4-    050309 568  0.0   0.1+    070116 568  0.1+  0.0
    050105 568  0.1-  0.3-    050309 568  0.1-  0.0     070117 568  0.7-  0.8+
    050207 568  0.0   0.0     050311 568  0.2-  0.4+
    050207 568  0.1-  0.0     050311 568  0.0   0.4+
    
    
    A. U. Tomatic                (C) Copyright 2019 MPC           M.P.E.C. 2019-T136
    


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