\begin{table}%t5
\caption{\label{tab:s3}Orbital parameters of an orbit close to the center of libration of
the 5:1~mean motion resonance.}
%\centering
\par
\begin{tabular}{llcc}
\hline\hline \noalign{\smallskip}
   Param. & S3 & Inner & Outer \\
\hline
   $a$ & [AU] & 0.8050 & 2.5113\\
   $i$ & [deg] & 90 & 90 \\
   $e$ & & 0.439 & 0.071 \\
   $M+\omega$ & [deg] & 239.25 & 247.30 \\
   $\omega$ & [deg] & 161.81 & 78.19 \\
   $\Omega$ & [deg] & 0 & 0 \\
   $m$ & [$M_{\rm Jup}$] & 16.59 & 2.179 \\
\hline
   Date & [JD-2~400~000] & \multicolumn{2}{c}{53~000.00} \\
   $\rsc$ & & \multicolumn{2}{c}{1.553} \\[2pt]
\hline
\end{tabular}
\tablefoot {This orbit was obtained from S2 (Table~\ref{tab:90_stable}) at the sixth iteration.
We expect that the actual system will be closer to this orbit as dissipative processes will have dampened the resonant mode.}
\end{table}