\begin{table}%t4
\caption{Time development of orbital variability near stability boundary
for S-type orbits.}\label{tab4}
%\centerline
{
\begin{tabular}{c c c c c c c c}
\hline
\hline
$M_{\rm B}/M_{\rm A}$ & $R_{\rm B}/R_{\rm A}$
             & 1~K      & 10~K     & 50~K     & 75~K     & 100~K    & 150~K \\
\omit & \omit & [\%]    & [\%]     & [\%]     & [\%]     & [\%]     & [\%]  \\
\noalign{\smallskip}
\hline
0.10 &  0.44 &  5.11929	&  5.10191 &  5.10581 &  5.10811 &  5.10752 &  5.106775 \\
0.15 &  0.39 &  5.21648	&  5.21112 &  5.21076 &  5.20963 &	5.20931 &  5.210078 \\
0.33 &  0.32 &  5.19342	&  5.19629 &  5.19107 &  5.19522 &	5.19489 &  5.195642 \\
0.50 &  0.28 &  5.13434	&  5.11435 &  5.12381 &  5.12558 &	5.11732 &  5.117495 \\
0.60 &  0.27 &  5.63816	&  5.62302 &  5.63053 &  5.62834 &	5.62294 &  5.625883 \\
0.90 &  0.24 &  5.99959	&  6.03042 &  6.01998 &  6.02526 &	6.02137 &  6.015876 \\
\hline
\end{tabular}}
\medskip
Note: Simulations were performed for giant planets with $M_{\rm G}$~= 1~$M_{\rm Jup}$.
\end{table}