  We take the line of sight velocity dispersions as functions of radius for 8
Milky Way dwarf spheroidal galaxies and use Jeans analysis to calculate the
mass-to-light ratios (M/L) in Modified Newtonian Dynamics (MOND). Using the
latest structural parameters, distances and variable velocity anisotropy, we
find 6/8 dwarfs have sensible M/L using only the stellar populations. Sextans
and Draco, however, have M/L=9.2_{-3.0}^{+5.3} and 43.9_{-19.3}^{+29.0}
respectively, which poses a problem. Apart from the need for Sextans'
integrated magnitude to be reviewed, we propose tidal effects intrinsic to
MOND, testable with numerical simulations, but fully orbit dependant, which are
disrupting Draco. The creation of the Magellanic Stream is also re-addressed in
MOND, the scenario being the stream is ram pressure stripped from the SMC as it
crosses the LMC.
