\begin{table}%t1
\caption{\label{params}Target information.}
\par
%%\centering

\par
\begin{tabular}{lcccccc} 
\hline \hline \noalign{\smallskip}
Parameter	&	 (52872) 	& (73480)  	&	 (90482)  	\\
&	 Okyrhoe 	&	 2002 PN$_{34}$  	&	Orcus  	\\
\hline
Orbit	&	 Jupiter-Coupled\tablefootmark{a} 	&	Scattered Disk 	&	 Resonant (3:2) 	\\
Albedo (\%)\tablefootmark{b}	&	  $\rm 2.49^{+0.81}_{-0.55}$	&	  $\rm 4.25^{+0.83}_{-0.65}$	&	$\rm 19.72^{+3.40}_{-2.76}$ 	\\
Diam. (km)	&	  $\rm 52.1^{+6.9}_{-6.9}$  	&	  $\rm 119.5^{+10.3}_{-10.2}$   	&	 $\rm 946.3^{+74.1}_{-72.3}$ 	\\
$a$ (AU)\tablefootmark{c}	&	8.4	&	31.2	&	39.2	\\
$e$ 	&	0.31	&	0.57	&	0.23	\\
$i$ (deg)	&	15.7	&	16.6	&	20.6	\\
Taxonomy\tablefootmark{d} & BR & BR, BB & BB \\
\hline
\end{tabular}
\tablefoot {\tablefoottext{a}{Some classify object 52872 as a Centaur, but because its Tisserand parameter~$T_{\rm J}$ is less than 3.05 ($T_{\rm J}$~=~2.95) it is ``rapidly perturbed by Jupiter'' according to \citet{Gladman2008}.}\\
\tablefoottext{b}{From \citet{Stansberry2008}.}\\
\tablefoottext{c}{$a$, $e$, and $i$ are the orbital elements semi-major axis, eccentricity and inclination, respectively.}\\
\tablefoottext{d}{Classifications are performed using the taxonomic system designed by \citet{Barucci2005}. The designation comes from \citet{Fulchignoni2008} for Okyrhoe and Orcus and from \citet{Perna2010} for (73480) 2002 PN$_{34}$.}}
\end{table}