• MPC Preparation (Info)

  • MPEC 2006-B27 : COMET 73P/SCHWASSMANN-WACHMANN (component B assumed)

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    M.P.E.C. 2006-B27                                Issued 2006 Jan. 23, 21:57 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
    
                    COMET 73P/SCHWASSMANN-WACHMANN  (component B assumed)
    
    Observations:
    0073P      b  C2006 01 06.47878 12 41 58.76 +10 54 11.5          18.8 R EB027H02
    0073P      b  C2006 01 06.48259 12 41 59.04 +10 54 10.1          18.8 R EB027H02
    0073P      b  C2006 01 06.48640 12 41 59.37 +10 54 10.0          18.6 R EB027H02
    0073P      b  C2006 01 06.49022 12 41 59.67 +10 54 09.4          18.8 R EB027H02
    0073P      b  C2006 01 06.49403 12 42 00.02 +10 54 09.4          18.7 R EB027H02
    0073P      b  C2006 01 06.49784 12 42 00.32 +10 54 08.8          18.8 R EB027H02
    0073P      b  C2006 01 07.50299 12 43 25.62 +10 52 17.9          19.0 R EB027H02
    0073P      b  C2006 01 07.50681 12 43 25.93 +10 52 17.0          18.9 R EB027H02
    0073P      b  C2006 01 07.51061 12 43 26.23 +10 52 16.2          19.0 R EB027H02
    0073P      b  C2006 01 07.51442 12 43 26.51 +10 52 16.2          19.1 R EB027H02
    0073P      b  C2006 01 07.51824 12 43 26.88 +10 52 15.7          19.0 R EB027H02
    0073P      b  C2006 01 07.52205 12 43 27.23 +10 52 15.9          18.9 R EB027H02
    0073P      b  C2006 01 09.38924 12 46 05.41 +10 49 09.5          17.7 R EB027H02
    0073P      b  C2006 01 09.39304 12 46 05.85 +10 49 09.7          17.7 R EB027H02
    0073P      b  C2006 01 09.39685 12 46 06.14 +10 49 09.3          17.8 R EB027H02
    0073P      b  C2006 01 23.45735 13 05 41.42 +10 42 07.1          18.1 V EB027703
    0073P      b  C2006 01 23.46453 13 05 41.78 +10 42 09.0          17.8 V EB027703
    0073P      b  C2006 01 23.47159 13 05 42.54 +10 42 07.4          18.1 V EB027703
    0073P      b  C2006 01 23.47867 13 05 43.04 +10 42 07.4          18.1 V EB027703
    0073P      b  C2006 01 23.48770 13 05 43.65 +10 42 09.5          17.6 V EB027703
    0073P      b  C2006 01 23.49607 13 05 44.37 +10 42 09.6          17.9 V EB027703
    0073P      b  C2006 01 23.50447 13 05 44.95 +10 42 10.2          17.7 V EB027703
    0073P      b  C2006 01 23.51284 13 05 45.78 +10 42 10.9          18.0 V EB027703
    
    Observer details:
    703 Catalina Sky Survey.  Observer R. Hill.  0.68-m Schmidt + CCD
    H02 Sulphur Flats Observatory, La Cueva.  Observer J. A. Farrell.  0.41-m
        f/8.4 reflector + CCD.
    
    Orbital elements:
      73P/Schwassmann-Wachmann  (component B assumed; cf. IAUC 8659)
    Epoch 2006 May 25.0 TT = JDT 2453880.5
    T 2006 June 7.93879 TT                                  MPC
    q   0.9391230            (2000.0)            P               Q
    n   0.18394412     Peri.  198.80470     -0.02870951     +0.98221160
    a   3.0620488      Node    69.89227     -0.88990146     +0.05943516
    e   0.6933024      Incl.   11.39751     -0.45524845     -0.17812306
    P   5.36
    From 71 observations 1995 Dec. 23-2006 Jan. 23, mean residual 0".92.  Non-
       gravitational parameters A1 = +0.87 +/- 0.32, A2 = +0.1981 +/- 0.1086.
    
    Residuals in seconds of arc
    951223 568  0.6+  1.4+    960206 118  0.1-  1.7-    060106 H02  0.3-  0.7+
    951223 568  0.8+  0.9+    960206 118  0.3+  2.3-    060106 H02  0.8-  0.3-
    951224 568  1.0-  0.8+    960206 118  0.8-  3.1-    060106 H02  0.6-  0.1+
    951224 568  0.6-  2.3+    960209 711  0.5-  0.6-    060106 H02  0.9-  0.1-
    951225 568  0.8-  0.8+    960209 711  0.2-  0.4-    060106 H02  0.4-  0.3+
    951225 568  1.0-  0.8+    960210 711  0.2-  0.6-    060106 H02  0.6-  0.2+
    951227 691  2.0-  0.6-    960210 711  1.1-  1.3-    060107 H02  0.4+  0.3+
    951227 691  1.4-  0.3-    960215 693  1.6+  0.5+    060107 H02  0.3+  0.1-
    960111 360  1.9+  0.3+    960215 693  0.2+  0.6-    060107 H02  0.0   0.5-
    960111 360  2.0+  0.2+    960215 693  0.4-  0.9-    060107 H02  0.5-  0.1-
    960111 360  1.2+  0.2+    960216 693  0.5+  0.3+    060107 H02  0.3+  0.2-
    960113 118  0.4+  0.7-    960216 693  1.5+  0.9+    060107 H02  0.8+  0.4+
    960114 118  0.4+  1.9-    960910 809  0.7-  0.2+    060109 H02  0.2-  0.6-
    960119 691  0.7-  1.0-    960913 809  0.1-  0.4+    060109 H02  1.6+  0.0
    960119 691  0.9-  0.9-    960914 809  0.1-  0.1+    060109 H02  1.2+  0.1-
    960119 691  1.0-  0.8-    960914 809  0.1-  0.1+    060123 703  1.9+  0.8-
    960121 695  1.5+  1.6+    960915 809  0.4-  0.2+    060123 703  1.3-  0.8+
    960121 695  0.4+  0.8+    960915 809  0.2-  0.1+    060123 703  1.5+  1.0-
    960121 695  0.7+  1.6+    961118 696  2.0+  0.9-    060123 703  0.5+  1.3-
    960121 695  0.1+  1.3+    961118 696  0.7-  0.2-    060123 703  1.2-  0.4+
    960126 413  0.9+  0.4-    961119 696  0.5+  0.2+    060123 703  0.5-  0.2+
    960126 413  0.5+  0.7+    961214 695  1.4-  0.2+    060123 703  1.8-  0.5+
    960127 413  0.2+  0.3-    961214 695  0.2+  0.4+    060123 703  0.5+  0.9+
    960127 413  0.4-  0.4-    961214 695  0.2-  1.7+
    
    Ephemeris:
      73P/Schwassmann-Wachmann (B)    [Mag. = 14.0 + 5 log Delta + 10 log r]
    Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase  Mag.
    2006 01 15    12 53.96   +10 42.8    1.542    2.044   105.9    27.6  18.0
    2006 01 20    13 00.91   +10 41.0    1.447    1.999   109.2    27.7  17.8
    2006 01 25    13 07.80   +10 43.4    1.353    1.953   112.4    27.8  17.6
    2006 01 30    13 14.60   +10 50.2    1.262    1.908   115.6    27.7  17.3
    2006 02 04    13 21.31   +11 01.9    1.173    1.862   118.9    27.6  17.0
    2006 02 09    13 27.92   +11 18.8    1.088    1.815   122.0    27.4  16.8
    2006 02 14    13 34.42   +11 41.2    1.005    1.769   125.2    27.2  16.5
    2006 02 19    13 40.80   +12 09.7    0.925    1.722   128.2    26.8  16.2
    2006 02 24    13 47.06   +12 44.6    0.849    1.674   131.1    26.4  15.9
    2006 03 01    13 53.20   +13 26.3    0.775    1.627   133.9    26.0  15.6
    2006 03 06    13 59.20   +14 15.2    0.705    1.580   136.5    25.6  15.2
    2006 03 11    14 05.12   +15 11.3    0.639    1.533   138.8    25.3  14.9
    2006 03 16    14 10.99   +16 15.0    0.576    1.486   140.7    25.1  14.5
    2006 03 21    14 16.87   +17 26.6    0.516    1.439   142.2    25.1  14.1
    2006 03 26    14 22.88   +18 46.6    0.459    1.392   143.1    25.5  13.7
    2006 03 31    14 29.16   +20 15.3    0.406    1.346   143.3    26.3  13.3
    2006 04 05    14 36.02   +21 53.0    0.355    1.301   142.8    27.7  12.9
    2006 04 10    14 43.94   +23 41.2    0.307    1.257   141.6    29.7  12.4
    2006 04 15    14 53.69   +25 42.6    0.261    1.214   139.5    32.5  11.9
    2006 04 20    15 06.63   +28 02.4    0.218    1.172   136.5    36.2  11.4
    2006 04 25    15 25.37   +30 49.6    0.177    1.133   132.5    40.9  10.8
    2006 04 30    15 55.59   +34 16.6    0.138    1.095   126.9    47.4  10.1
    2006 05 05    16 51.13   +38 23.2    0.103    1.061   118.2    56.9   9.3
    2006 05 10    18 42.01   +40 36.0    0.0759   1.030   103.4    72.5   8.5
    2006 05 15    21 23.29   +31 00.5    0.0671   1.003    81.1    95.1   8.1
    
         The observations for the above solution were selected according to the
    assessment of component B (vs. E and F) by Sekanina (2006, IAUC 8659; 2005,
    ICQ 27, 229, Table 2).
    
    Daniel W. E. Green           (C) Copyright 2006 MPC           M.P.E.C. 2006-B27
    

    Read MPEC 2006-B26 Read MPEC 2006-B28


    MPEC number:

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