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.
Parameter

Mass of Jupiter 9.54594307716659D-004

Mass of Io 4.491666410348056D-008

Mass of Europa 2.411981912350972D-008

Mass of Ganymede 7.450567670228471D-008

Mass of Callisto 5.409660246012525D-008

E_r 0.477266151384435377D-03

J₂ 14736.D-06

J₄ -587.D-06

J₆ 31.D-06

$\psi$ 358.070068991729D0

I 25.5020491751445D0

**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.
Parameter
Mass of Jupiter	9.54594307716659D-004
Mass of Io	4.491666410348056D-008
Mass of Europa	2.411981912350972D-008
Mass of Ganymede	7.450567670228471D-008
Mass of Callisto	5.409660246012525D-008
E_r	0.477266151384435377D-03
J₂	14736.D-06
J₄	-587.D-06
J₆	31.D-06
$\psi$	358.070068991729D0
I	25.5020491751445D0

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