We present an analysis of the orbital properties of nine intermediate-redsh
ift clusters of the Canadian Network for Observational Cosmology (CNOCl) su
rvey and compare them to a control sample of 12 nearby clusters. Similar to
the nearby elliptical galaxies, the bulge-dominated galaxies in clusters a
t redshifts similar to 0.1-0.4 present orbits that are more eccentric than
those of disk-dominated galaxies. However, the orbital segregation is less
significant than that found for elliptical and spiral galaxies in nearby cl
usters. The strongest orbital segregation is found when galaxies are separa
ted by colors [red galaxies with colors in the rest frame (U-V)(0) > 1.4, b
lue galaxies with (U-V)(0) less than or equal to 1.4]. Therefore, the segre
gation we find seems to modify the star formation activity more efficiently
than the internal shape of the galaxies. When we compare the orbits of ear
ly-type galaxies at intermediate redshift with those for z = 0, they seem t
o develop significant changes, becoming much more eccentric. A different be
havior is observed in the late-type galaxies, which present no significant
evolution in their orbit shapes.