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In this section we will use our new definitions for rotational variables to generate kinematic equations for rotational motion. In addition, we will examine the vector nature of rotational variables and, finally, relate linear and angular variables.

Because our equations defining rotational and translational variables are mathematically equivalent, we can simply substitute our rotational variables into the kinematic equations we have already derived for translational variables. We could go through the formal derivation of these equations, but they would be the same as those derived in One-Dimensional Kinematics. Thus we can simply state the equations, alongside their translational analogues:

v_{f} = v_{o} + at | σ_{f} = σ_{o} + αt | ||

x_{f} = x_{o} + v_{o}t + at^{2} | μ_{f} = μ_{o} + σ_{o}t + αt^{2} | ||

v_{f}^{2} = v_{o}^{2} + 2ax | σ_{f}^{2} = σ_{o}^{2} +2αμ | ||

x = (v_{o} + v_{f})t | μ = (σ_{o} + σ_{f})t |

These equations for rotational motion are used identically as the corollary equations for translational motion. In addition, like translational motion, these equations are only valid when the acceleration,

Now that we have established both equations for our variables and kinematic equations relating them, we can also relate our rotational variables to translational variables. This can sometimes be confusing. It is easy to think that because a particle is engaged in rotational motion, it is not also defined by translational variables. Simply remind yourself that no matter what path a given particle is traveling in, it always has a position, velocity and acceleration. The rotational variables we generated do not substitute for these traditional variables; instead, they simplify calculations involving rotational motion. Thus we can relate our rotational and translational variables.

Recall from our definition of angular displacement that:

s = μr |

Thus the displacement,

=

Thus
v = σr |

Just as linear displacement is equal to angular displacement times the radius,
linear velocity is equal to angular velocity times the radius. We can relate
*α* and *a*, by the same method we used before: differentiating with respect
to time.

= *r*

We must be careful in relating translationa and angular acceleration because
only gives us the change in velocity with respect to time in the
*tangential* direction. We know from
Dynamics that any particle
traveling in a circle experiences a radial force equal to . We
must therefore generate two different expressions for the linear acceleration of
a particle in rotational motion:

a_{T} | = | αr | |

a_{R} | = | ||

= | σ^{2}r |

These two equations may seem a bit confusing, so we shall examine them closely. Consider a particle moving around a circle with a constant speed. The rate at which the particle makes a revolution about the axis is constant, so

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