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All Tables

- Table 1:
Observations used in L1 fit.
- Table 2:
Initial conditions at the Julian epoch 2 433 282.5 (01/01/1950, 0H00 TT) found after fitting our numerical model to the observations. The positions are
given in ua and the velocities in ua.day
^{-1}.
- Table 3:
Parameters used in our numerical model for fitting the observations (from Campbell & Synnott 1985; Anderson et al. 1996;
Schubert et al. 1994). The masses are given in Solar mass, the Jovian equatorial
radius
*E*_{r}
in ua and the angles in degrees.