Angular velocity, acceleration, including centripetal and coriolis acceleration

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In order to define angular velocity, consider a particle P moving in a XOY reference plane, as diagramed in Figure 1. Let x be the projection of P on the OX axis, y the projection of P on the OY axis, r the length of OP, and \theta the \angle{POX} angle.

Figure 1
Figure 1

We can then write that:

x = r\cos\theta

y = r\sin\theta

By differentiating these equations with respect to time, we have:

\dot x = \frac{dx}{dt} = \dot r \cos\theta - r\dot \theta \sin\theta
(5)
\dot y = \frac{dy}{dt} = \dot r \sin\theta + r\dot \theta \cos\theta
(6)

We can write the tangential component of velocity, v_T, which is the component of velocity perpendicular to OP, as:

v_T = \dot y \cos\theta - \dot x \sin\theta

and, by using the expressions of \dot x and \dot y from equations (#1) and (#2) respectively, we obtain:

v_T = r \dot \theta
(7)

We define the angular velocity \omega as the rate of change of \theta with respect to time:

\omega = \frac{d\theta}{dt}
(8)

Using (#4) in (#3) we get that:

v_T = r\omega

from which the angular velocity becomes:

\omega = \frac{v_T}{r}

In order to define the acceleration, we first have to calculate \ddot x and \ddot y. To do this we differentiate equations (#1) and (#2) with respect to time, when we obtain that:

\ddot x = \ddot r \cos\theta - \dot r \sin\theta - r\ddot \theta^2 \cos\theta - r \ddot \theta \sin\theta
(9)
\ddot y = \ddot r \sin\theta + \dot r \dot \theta \cos\theta + r \dot \theta^2 \sin\theta +r \ddot \theta \cos\theta
(10)

We can write the radial component of acceleration, a_r, which is the component of acceleration in the direction of OP, as:

a_r = \ddot x \cos\theta + \ddot y \sin\theta

and, by using the expressions of \ddot x and \ddot y from equations (#5) and (#6) respectively, we get:

a_r = \ddot r - r \dot \theta^2
(11)

We can also write (#7), by using (#4), as:

a_r = \dot v - r\omega^2

where \dot v is the rate of change of velocity, while the r\omega^2 term is called the centripetal acceleration (a_c).

The tangential component of acceleration on the other hand, a_T, can be written as:

a_T = \ddot y \cos\theta - \ddot x \sin\theta

and, again by replacing \ddot x and \ddot y from equations (#5) and (#6) respectively, we obtain:

a_T = r \ddot \theta + 2 \dot r \dot \theta
(12)

We define the angular acceleration \alpha as the rate of change of the angular velocity \omega with respect to time:

\alpha = \frac{d\omega}{dt} = \ddot \theta
(13)

Equation (#8) can also be written, by taking into account (#9), as:

a_T = r \alpha + 2v\omega where the 2v\omega term is called the compound supplementary acceleration, or the Coriolis component of acceleration a_C.

Example 1 [imperial]
Problem

Consider that the hard disk of a computer is circular and rotates with an angular velocity of 7200 revolutions per minute.

Calculate the linear velocity (in miles per hour) of a particle which is found 2 inches away from the center of the hard disk.

Workings

The angular velocity of the hard disk expressed in SI units is:

\omega = 7200 \cdot \frac{2\pi}{60} = 240\pi \; \frac{rad}{s}

As the linear velocity can be defined as v=\omega r, we obtain the linear velocity of the particle as:

v = 240\pi\cdot 2 = 1507.2 \;\frac{inch}{s}

or, by converting it in miles per hour:

Solution

v = 85.63 \; mph

Reference

For an application of angular velocity to mechanics, also see the reference page on Velocity and Acceleration of a Piston .