  The recent SDSS measured velocity distribution of satellite galaxies has been
modelled in the context of MOND. We show that even when the extra constraint of
adhering to the projected satellite number density profile is added, the two
line of sight (los) velocity dispersion profiles presented in Klypin & Prada
(2007) can be matched simply with a radially varying anisotropy. Interestingly,
the anisotropies required to fit the los velocity dispersions are remarkably
similar to the anisotropies generated by dissipationless collapse simulations
in MOND. The mass-to-light ratios of the two host galaxies used are sensible
and positivity of the distribution function is satisfied.
