  We compare the recently published velocity dispersions for seventeen
Andromeda dwarf spheroidals with estimates of the MOND predictions, based on
the luminosities of these dwarfs, with reasonable stellar M/L values, and no
dark matter. We find that the two are consistent within the uncertainties. We
further predict the velocity dispersions of another ten dwarfs for which only
photometric data are currently available.

Cosmology and Nongalactic Astrophysics;General Relativity and Quantum Cosmology;High Energy Physics - Phenomenology