Table 1: Orbital elements of the prograde satellites of Jupiter and the stage during Jupiter's mass growth at which the satellites could have been captured (last two columns).
Satellite a₀ e₀ I₀ Jupiter's mass

$({R}_{\jupiter})$ (10⁵ yr) $\qquad$ (10⁷ yr)

Themisto 105.00 0.24 43.08 $\hbox{$^\circ$ }$ $39\%{-}42\% \quad 38\%{-}44\%$

Leda 156.17 0.16 27.46 $\hbox{$^\circ$ }$ $53\%{-}56\% \quad 53\%{-}57\%$

Himalia 160.31 0.16 27.50 $\hbox{$^\circ$ }$ $53\%{-}56\% \quad 56\%{-}59\%$

Lysithea 163.89 0.11 28.30 $\hbox{$^\circ$ }$ $55\%{-}57\% \quad 51\%{-}58\%$

Elara 164.23 0.22 26.63 $\hbox{$^\circ$ }$ $56\%{-}58\% \quad 55\%{-}60\%$

S2000 J11 175.61 0.25 28.30 $\hbox{$^\circ$ }$ $52\%{-}61\% \quad 61\%{-}63\%$

S2003 J20 239.19 0.30 55.10 $\hbox{$^\circ$ }$ $65\%{-}81\% \quad 75\%{-}84\%$

**Table 1:** Orbital elements of the prograde satellites of Jupiter and the stage during Jupiter's mass growth at which the satellites could have been captured (last two columns).
Satellite	a₀	e₀	I₀	Jupiter's mass
	$({R}_{\jupiter})$			(10⁵ yr) $\qquad$ (10⁷ yr)
Themisto	105.00	0.24	43.08 $\hbox{$^\circ$ }$	$39\%{-}42\% \quad 38\%{-}44\%$
Leda	156.17	0.16	27.46 $\hbox{$^\circ$ }$	$53\%{-}56\% \quad 53\%{-}57\%$
Himalia	160.31	0.16	27.50 $\hbox{$^\circ$ }$	$53\%{-}56\% \quad 56\%{-}59\%$
Lysithea	163.89	0.11	28.30 $\hbox{$^\circ$ }$	$55\%{-}57\% \quad 51\%{-}58\%$
Elara	164.23	0.22	26.63 $\hbox{$^\circ$ }$	$56\%{-}58\% \quad 55\%{-}60\%$
S2000 J11	175.61	0.25	28.30 $\hbox{$^\circ$ }$	$52\%{-}61\% \quad 61\%{-}63\%$
S2003 J20	239.19	0.30	55.10 $\hbox{$^\circ$ }$	$65\%{-}81\% \quad 75\%{-}84\%$

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