  Dark matter is required in galaxies at galactocentric radii that are larger
than the $a_0$-radius, which is where the gravitational acceleration generated
by baryons of the galaxy equals the constant $a_0=1.2\times 10^{-10}$ms$^{-2}$
known as the galactic acceleration scale. It was found previously for massive
early-type galaxies that the radial number-density profiles of their globular
cluster (GC) systems follow broken power laws and the breaks occur at the
$a_0$-radii. We have newly analyzed the distribution of GCs around galaxies in
the Fornax cluster in existing photometric catalogs. We found that 1) the
coincidence between $a_0$-radii and the break radii of globular cluster systems
is valid for early-type galaxies of all masses and, 2) this also applies to the
red and blue sub-populations of GCs separately.
