These equations, called Euler’s equations of motion, may be used to analyse the motion of a rigid
body about its mass center.
Three differential equations of motion of the mass center together with above Euler’s equations
form a system of six differential equations. Given appropriate initial conditions, these differential
equations have a unique solution.
Thus, the motion of a rigid body is completely defined by the sum and the total moment about the
mass center of the external force system acting on it.