\begin{table}%t7
\caption{Time development of orbital variability near stability boundary
for P-type orbits.}\label{tab7}
%\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    & 5~K     & 10~K    & 20~K    & 30~K    & 40~K    \\
\omit & \omit & [\%]   & [\%]    & [\%]    & [\%]    & [\%]    & [\%]    \\
\noalign{\smallskip}
\hline
0.10 &  1.95 & 4.16005 & 4.11282 & 4.08047 & 4.05153 & 4.03336 & 4.04495 \\
0.15 &  2.05 & 4.19949 & 4.19578 & 4.19493 & 4.19248 & 4.19492 & 4.19569 \\
0.33 &  2.25 & 4.81418 & 4.70511 & 4.79329 & 4.79473 & 4.79914 & ...     \\
0.50 &  2.35 & 4.99639 & 4.99501 & 4.99456 & 4.99473 & 4.99439 & ...     \\
0.60 &  2.40 & 4.98571 & 4.98039 & 4.98185 & 4.98188 & 4.98139 & ...     \\
0.90 &  2.45 & 4.99734 & 4.99471 & 4.99501 & 4.99483 & 4.98991 & ...     \\
\hline
\end{tabular}}
\medskip
Note: Simulations were performed for giant planets with $M_{\rm G}$~= 1~$M_{\rm Jup}$.
\end{table}