  We construct mock galaxy catalogues to analyse clustering properties of a
Lambda cold dark matter (LCDM) universe within a cosmological dark matter
simulation of sufficient resolution to resolve structure down to the scale of
dwarfs. We show that there is a strong age-clustering correlation for objects
likely to host luminous galaxies, which includes the satellite halo (subhalo)
population. Older mock galaxies are significantly more clustered in our
catalog, which consists of satellite haloes as well as the central peaks of
discrete haloes, selected solely by peak circular velocity. This age dependence
is caused mainly by the age-clustering relation for discrete haloes, recently
found by Gao et al., acting mostly on field members, combined with the tendency
for older mock galaxies to lie within groups and clusters, where galaxy
clustering is enhanced. Our results suggest that the clustering age dependence
is manifested in real galaxies. At small scales (less than ~5 Mpc/h), the very
simple assumption that galaxy colour depends solely on halo age is inconsistent
with the strength of the observed clustering colour trends, where red galaxies
become increasingly more clustered than blue galaxies toward smaller scales,
suggesting that luminosity weighted galaxy ages do not closely trace the
assembly epoch of their dark matter hosts. The age dependence is present but is
much weaker for satellite haloes lying within groups and clusters than for the
global population.
