We have calculated the root-mean-square residuals of the observations
in the form of inter-satellite and
measures. In Table 5
we present the statistics for Tethys, Dione, Rhea and Titan. The rejection level
was
. For comparison, we give the same statistics for the observations
published in
Harper et al. (1997). The orbital models are those of
Harper & Taylor (1993).
![]() |
Copyright The European Southern Observatory (ESO)