Grounds and applications of Bargmann-Michel-Telegdi equations for the
precession of the polarization vector of relativistic particles are co
nsidered. A critical question in the discussion is the orientation of
the rest frame reference vectors. Moller reference frames which keep c
onstant the mutual orientation of the two infinitely close in time res
t frames are shown to have a special role. The generally covariant for
m of the equations is discussed. The assertion that the principle of r
elativity is violated in the phenomenon of spin precession is proved t
o be untrue.