Euler's equations of rigid body motion for the Cartesian rotation rate
s omega(i) are normally derived directly from Newton's second law rath
er than from a Lagrangian formulation. The reason is that a set of f i
ndependent velocities omega(i) that are defined by linear transformati
ons on time rates of change of group parameters is generally nonintegr
able and therefore cannot be integrated to yield a set of f generalize
d coordinates. We analyze and answer the following related question: w
hen can a particular parameterization of a continuous group be used as
a set of generalized coordinates? An understanding of the distinction
between holonomic and nonholonomic coordinates via elementary Lie the
ory paves the way toward a more qualitatively complete understanding o
f the idea of integrability of a Hamiltonian dynamical system.