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MPEC 1997-N18 : 1996 TS66

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M.P.E.C. 1997-N18                                Issued 1997 July 12, 15:27 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.

             BMARSDEN@CFA.HARVARD.EDU or GWILLIAMS@CFA.HARVARD.EDU
                 URL http://cfa-www.harvard.edu/cfa/ps/mpc.html

                                   1996 TS66

                           Revision to MPEC 1997-N12

Observations:
     J96T66S  C1997 07 11.41135 02 14 20.62 +20 42 12.2                      696
     J96T66S  C1997 07 11.45336 02 14 20.70 +20 42 13.4                      696
     J96T66S  C1997 07 12.43955 02 14 23.35 +20 42 36.1          21.8 R      696

Observer details:
696 Whipple Observatory, Mt. Hopkins.  Observer C. W. Hergenrother.
    1.2-m reflector + CCD.

First and last observations above in comparison with prediction:
Residuals in seconds of arc and reference
970711 696 25.4+  7.4+    970712 696 24.8+  7.5+    MPEC 1997-N12

Orbital elements:
1996 TS66
Epoch 1997 June 1.0 TT = JDT 2450600.5                  Marsden
M 330.93308              (2000.0)            P               Q
n   0.00335397     Peri.  149.36810     +0.25354743     -0.95944208
a  44.2007845      Node   285.70523     +0.85953846     +0.28189748
e   0.1441125      Incl.    7.35430     +0.44374242     +0.00216872
P 294              H    6.0           G   0.15           U   6
Residuals in seconds of arc
961012 568  0.2+  0.3+    961117 696  0.5+  0.1-    961215 696  0.0   0.1-
961012 568  0.2+  0.1+    961117 696  0.3-  0.6-    970201 696  0.2-  0.3+
961012 568  0.0   0.1+    961118 696  0.5-  0.1+    970711 696  0.4+  0.1-
961014 568  0.1+  0.0     961118 696  0.2-  0.3+    970711 696  0.1-  0.1+
961014 568  0.1-  0.3-    961118 696  0.1-  0.1+    970712 696  0.3-  0.1-
961014 568  0.1-  0.2-    961215 696  0.6+  0.1+

Ephemeris:
1996 TS66                a,e,i = 44.20, 0.14, 7                  q = 37.831
Date    TT    R. A. (2000) Decl.     Delta      r     Elong.  Phase     V
1997 07 11    02 14.32   +20 42.0   39.214   38.888    70.6     1.4    22.1
1997 07 21    02 14.71   +20 45.6   39.050   38.886    80.0     1.5    22.1
1997 07 31    02 14.93   +20 48.5   38.881   38.884    89.4     1.5    22.1
1997 08 10    02 14.98   +20 50.5   38.712   38.881    98.9     1.5    22.1
1997 08 20    02 14.87   +20 51.6   38.547   38.879   108.4     1.4    22.1
1997 08 30    02 14.59   +20 51.9   38.391   38.877   118.1     1.3    22.1
1997 09 09    02 14.15   +20 51.2   38.249   38.874   127.8     1.2    22.0
1997 09 19    02 13.58   +20 49.7   38.126   38.872   137.5     1.0    22.0
1997 09 29    02 12.90   +20 47.3   38.023   38.870   147.2     0.8    22.0
1997 10 09    02 12.12   +20 44.2   37.946   38.867   156.9     0.6    22.0
1997 10 19    02 11.28   +20 40.4   37.897   38.865   166.2     0.4    21.9
1997 10 29    02 10.41   +20 36.1   37.877   38.863   172.8     0.2    21.9
1997 11 08    02 09.54   +20 31.5   37.887   38.860   169.0     0.3    21.9
1997 11 18    02 08.71   +20 26.6   37.928   38.858   160.0     0.5    21.9
1997 11 28    02 07.95   +20 21.8   37.997   38.856   150.2     0.7    22.0
1997 12 08    02 07.29   +20 17.1   38.093   38.854   140.1     0.9    22.0
1997 12 18    02 06.76   +20 12.9   38.212   38.851   130.0     1.1    22.0
1997 12 28    02 06.37   +20 09.1   38.351   38.849   119.8     1.3    22.0
1998 01 07    02 06.15   +20 06.0   38.505   38.847   109.6     1.4    22.1
1998 01 17    02 06.11   +20 03.8   38.670   38.844    99.5     1.4    22.1
1998 01 27    02 06.24   +20 02.4   38.840   38.842    89.4     1.5    22.1
1998 02 06    02 06.55   +20 01.9   39.009   38.840    79.4     1.4    22.1
1998 02 16    02 07.03   +20 02.4   39.173   38.837    69.5     1.4    22.1

Brian G. Marsden             (C) Copyright 1997 MPC           M.P.E.C. 1997-N18

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