\begin{table}%t4
\caption{\label{table:4}Interior surviving planets at 170~000~years compared with
the four currently known "hot Neptune'' systems. Data include the
closest giant planet.}  
%\centering
\par
\begin{tabular}{c| c c c c c}
 \hline\hline  
Scenario & ID & Mass~(${M}_{\oplus}$) & $a$~(AU) & $e$ & Resonances\\
 \hline 
I & OLI8 & 15.65 & 0.055 & 0.052 & None\\
& GIA1 & 160.3 & 0.100 & 0.003 & \\
 II & OLI9 & 2.33 & 0.047 & 0.148 & 5:4 with ICE9, 5:3 with ICE1\\
& ICE9 & 6.69 & 0.054 & 0.071 & 4:3 with ICE1\\
& ICE1 & 5.58 & 0.065 & 0.022 & \\
& GIA1 & 160.9 & 0.100 & 0.005 & \\
 III & ICE1 & 4.89 & 0.023 & 0.110 & None\\
& GIA1 & 160.3 & 0.100 & 0.001 & \\
 IV & OLI28 & 2.86 & 0.036 & 0.035 & None\\
& GIA1 & 159.8 & 0.100 & 0.002 & \\
 \hline 
\object{GJ~436} & b & 21.3 $\sin i$ & 0.028 & 0.12 & None\\
 \object{55~Cancri} & e & 14.3 $\sin i$ & 0.038 & 0.174 & None\\
& b & 267.3 $\sin i$ & 0.11 & 0.02 & \\
 \object{$\mu$~Arae} & d & 13.4 $\sin i$ & 0.09 & 0.0 & None\\
& b & 541.0 $\sin i$ & 1.5 & 0.31 & \\
\object{GJ~876} & d & 5.89 $\sin i$ & 0.021 & 0.0 & None\\
& c & 177.9 $\sin i$ & 0.13 & 0.27 & \\
 \hline
\end{tabular}
\end{table}