\begin{table}%T1
 \caption{\label{AspectData}Aspect data for 2006~RH$_{120}$. }
  \small%\centerline
{
\begin{tabular}{lrrrrrl}
\hline
\hline%---------------------------------------------------------
\multicolumn{1}{c}{Date     } & 
   \multicolumn{1}{c}{$r$}      & 
 \multicolumn{1}{c}{$\Delta$} & 
                        Phase & 
\multicolumn{1}{c}{$\lambda$} &
  \multicolumn{1}{c}{$\beta$} & 
                             \\
\multicolumn{1}{c}{2007}      &
                              & 
                              & 
                        angle & 
  \multicolumn{2}{c}{(J2000)} &
                             \\
     \multicolumn{1}{c}{(UT)} & 
     \multicolumn{1}{c}{(AU)} & 
     \multicolumn{1}{c}{(AU)} & 
\multicolumn{1}{c}{$(\degr)$} & 
\multicolumn{1}{c}{$(\degr)$} & 
\multicolumn{1}{c}{$(\degr)$} & 
                             \\
\hline
Mar. 11.87 & 0.995 & 0.0058 & 74.7 & 105.9 & --52.4 \\
Mar. 15.85 & 0.996 & 0.0047 & 74.2 & 104.5 & --37.1 \\
Mar. 16.84 & 0.996 & 0.0044 & 74.3 & 104.2 & --31.9 \\ 
Mar. 17.81 & 0.996 & 0.0041 & 74.4 & 104.0 & --26.2 \\
\hline
\end{tabular}}
\smallskip
Note: Due to its small geocentric
  distance, topocentric coordinates related to IAU station B31 (SALT) 
  were used: $\lambda$ and $\beta$ are the ecliptic longitude and latitude, 
  while $r$ and $\Delta$ are the distances of the asteroid from
  the Sun and the observer, respectively. 
\end{table}