  We employ recently published measurements of the velocity dispersions in the
newly discovered dwarf satellite galaxies of Andromeda to test our previously
published predictions of this quantity. The data are in good agreement with our
specific predictions for each dwarf made a priori with MOND, with reasonable
stellar mass-to-light ratios, and no dark matter, while Newtonian dynamics
point to quite large mass discrepancies in these systems. MOND distinguishes
between regimes where the internal field of the dwarf, or the external field of
the host, dominates. The data appear to recognize this distinction, which is a
unique feature of MOND not explicable in LCDM.
