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.