Rotation around a fixed axis

Classical mechanics
$\mathbf{F} = m \mathbf{a}$ Newton's Second Law
History of classical mechanics · Timeline of classical mechanics
Branches Statics · Dynamics / Kinetics · Kinematics · Applied mechanics · Celestial mechanics · Continuum mechanics · Statistical mechanics
Formulations Newtonian mechanics (Vectorial mechanics) Analytical mechanics: Lagrangian mechanics Hamiltonian mechanics
Fundamental concepts Space · Time · Velocity · Speed · Mass · Acceleration · Gravity · Force · Impulse · Torque / Moment / Couple · Momentum · Angular momentum · Inertia · Moment of inertia · Reference frame · Energy · Kinetic energy · Potential energy · Mechanical work · Virtual work · D'Alembert's principle
Core topics Rigid body · Rigid body dynamics · Euler's equations (rigid body dynamics) · Motion · Newton's laws of motion · Newton's law of universal gravitation · Euler's laws of motion · Equations of motion · Inertial frame of reference · Non-inertial reference frame · Rotating reference frame · Fictitious force · Linear motion · Mechanics of planar particle motion · Displacement (vector) · Relative velocity · Friction · Simple harmonic motion · Harmonic oscillator · Vibration · Damping · Damping ratio · Rotational motion · Circular motion · Uniform circular motion · Non-uniform circular motion · Centripetal force · Centrifugal force · Centrifugal force (rotating reference frame) · Reactive centrifugal force · Coriolis force · Pendulum · Rotational speed · Angular acceleration · Angular velocity · Angular frequency · Angular displacement
Scientists Galileo Galilei · Isaac Newton · Jeremiah Horrocks · Leonhard Euler · Jean le Rond d'Alembert · Alexis Clairaut · Joseph Louis Lagrange · Pierre-Simon Laplace · William Rowan Hamilton · Siméon-Denis Poisson

Rotation around a fixed axis is a special case of rotational motion. The fixed axis hypothesis exclude the possibility of a moving axis, and cannot describe such phenomena as wobbling or precession. According to Euler's rotation theorem, simultaneous rotation around more than one axis at the same time is impossible. If two rotations are forced at the same time, a new axis of rotation will appear.

The kinematics and dynamics of rotation around a fixed axis of a rigid body are mathematically much simpler than those for free rotation of a rigid body; they are entirely analogous to those of linear motion along a single fixed direction, which is not true for free rotation of a rigid body. The expressions for the kinetic energy of the object, and for the forces on the parts of the object, are also simpler for rotation around a fixed axis, than for general rotational motion. For these reasons, rotation around a fixed axis is typically taught in introductory physics courses after students have mastered linear motion; the full generality of rotational motion is not usually taught in introductory physics classes.

1 Translation and rotation
2 Kinematics
3 Dynamics
4 Vector expression
5 Examples and applications
- 5.1 Constant angular speed
- 5.2 Centripetal force
6 See also
7 References
8 Further reading

Translation and rotation

Kinematics

Angular Displacement

Main article: Angular displacement

A particle moves in a circle of radius $r$ . Having moved an arc length $s$ , its angular position is $\theta$ relative to its original position, where $\theta=\frac{s}{r}$ .

In mathematics and physics it is usual to use the natural unit radians rather than degrees or revolutions. Units are converted as follows:

$1 \mathrm{\ rev} = 360^{\circ} = 2\pi \mathrm{\ rad}\mathrm{, and}$

$1 \mathrm{\ rad} = 180^{\circ}/{\pi} \approx 57.3^{\circ}.$ ^[1]

An angular displacement is a change in angular position:

$\Delta \theta = \theta_{2} - \theta_{1}, \!$

where $\Delta \theta$ is the angular displacement, $\theta_1$ is the initial angular position and $\theta_2$ is the final angular position.

^[1]

Angular speed and angular velocity

Main article: Angular velocity

Angular velocity is the change in angular displacement per unit time. The symbol for angular velocity is $\omega$ and the units are typically rad s^-1. Angular speed is the magnitude of angular velocity.

$\overline{\omega} = \frac{\Delta \theta}{\Delta t} = \frac{\theta_2 - \theta_1}{t_2 - t_1}.$

The instantaneous angular velocity is given by

$\omega(t) = \frac{d\theta}{dt}.$

Using the formula for angular position and letting $v = \frac{ds}{dt}$ , we have also

$\omega=\frac{d\theta}{dt} = \frac{v}{r},$

where $v$ is the translational speed of the particle.

Angular velocity and frequency are related by

$\omega = {2 \pi f} \!$ .

Angular acceleration

Main article: Angular acceleration

A changing angular velocity indicates the presence of an angular acceleration in rigid body, typically measured in rad s⁻². The average angular acceleration $\overline{\alpha}$ over a time interval Δt is given by

$\overline{\alpha} = \frac{\Delta \omega}{\Delta t} = \frac{\omega_2 - \omega_1}{t_2 - t_1}.$

The instantaneous acceleration α(t) is given by

$\alpha(t) = \frac{d\omega}{dt} = \frac{d^2\theta}{dt^2}.$

Thus, the angular acceleration is the rate of change of the angular velocity, just as acceleration is the rate of change of velocity.

The translational acceleration of a point on the object rotating is given by

$a = r\alpha,\!$

where r is the radius or distance from the axis of rotation. This is also the tangential component of acceleration: it is tangential to the direction of motion of the point. If this component is 0, the motion is uniform circular motion, and the velocity changes in direction only.

The radial acceleration (perpendicular to direction of motion) is given by

$a_{\mathrm{R}} = \frac{v^2}{r} = \omega^2r\!$ .

It is directed towards the center of the rotational motion, and is often called the centripetal acceleration.

The angular acceleration is caused by the torque, which can have a positive or negative value in accordance with the convention of positive and negative angular frequency. The ratio of torque and angular acceleration (how difficult it is to start, stop, or otherwise change rotation) is given by the moment of inertia: $T = Ia$ .

Equations of kinematics

When the angular acceleration is constant, the five quantities angular displacement $\theta$ , initial angular velocity $\omega_i$ , final angular velocity $\omega_f$ , angular acceleration $\alpha$ , and time $t$ can be related by four equations of kinematics:

$\omega_f = \omega_i %2B \alpha t\;\!$

$\theta = \omega_i t %2B \begin{matrix}\frac{1}{2}\end{matrix} \alpha t^2$

$\omega_f^2 = \omega_i^2 %2B 2 \alpha\theta$

$\theta = \tfrac{1}{2} \left(\omega_f %2B \omega_i\right) t$

Dynamics

Moment of inertia

Main article: Moment of inertia

The moment of inertia of an object, symbolized by I or J, is a measure of the object's resistance to changes to its rotation. The moment of inertia is measured in kilogram metre² (kg m²). It depends on the object's mass: increasing the mass of an object increases the moment of inertia. It also depends on the distribution of the mass: distributing the mass further from the centre of rotation increases the moment of inertia by a greater degree. For a single particle of mass $m$ a distance $r$ from the axis of rotation, the moment of inertia is given by

$I = mr^2.$

Torque

Main article: Torque

Torque τ is the twisting effect of a force F applied to a rotating object which is at position r from its axis of rotation. Mathematically,

$\boldsymbol{\tau} = \mathbf{r} \times \mathbf{F},$

where × denotes the cross product. A net torque acting upon an object will produce an angular acceleration of the object according to

$\boldsymbol{\tau} = I\boldsymbol{\alpha},$

just as F = ma in linear dynamics.

The work done by a torque acting on an object equals the magnitude of the torque times the angle through which the torque is applied:

$W = T\theta. \!$

The power of a torque is equal to the work done by the torque per unit time, hence:

$P = T\omega. \!$

Angular Momentum

Main article: Angular momentum

The angular momentum L is a measure of the difficulty of bringing a rotating object to rest. It is given by

$\mathbf{L} = \mathbf{r} \times \mathbf{p}.$

Angular momentum is related to angular velocity by

$\mathbf{L}=I\boldsymbol{\omega},$

just as p = mv in linear dynamics.

Torque and angular momentum are related according to

$\boldsymbol{\tau} = \frac{d\mathbf{L}}{dt},$

just as F = dp/dt in linear dynamics. In the absence of an external torque, the angular momentum of a body remains constant. The conservation of angular momentum is notably demonstrated in figure skating: when pulling the arms closer to the body during a spin, the moment of inertia is decreased, and so the angular velocity is increased.

Kinetic energy

The kinetic energy K_rot due to the rotation of the body is given by

$K_{\mathrm{rot}} = \tfrac{1}{2}I\omega^2,$

just as K_trans = ¹⁄₂mv² in linear dynamics.

Vector expression

Examples and applications

Constant angular speed

Main article: Uniform circular motion

Centripetal force

Main article: Centripetal force

See also: Centrifugal force and Fictitious force

Internal tensile stress provides the centripetal force that keeps a spinning object together. A rigid body model neglects the accompanying strain. If the body is not rigid this strain will cause it to change shape. This is expressed as the object changing shape due to the "centrifugal force".

Celestial bodies rotating about each other often have elliptic orbits. The special case of circular orbits is an example of a rotation around a fixed axis: this axis is the line through the center of mass perpendicular to the plane of motion. The centripetal force is provided by gravity, see also two-body problem. This usually also applies for a spinning celestial body, so it need not be solid to keep together, unless the angular speed is too high in relation to its density. (It will, however, tend to become oblate.) For example, a spinning celestial body of water must take at least 3 hours and 18 minutes to rotate, regardless of size, or the water will separate. If the density of the fluid is higher the time can be less. See orbital period.

References

^ ^a ^b Fundamentals of Physics Extended 7th Edition by Halliday, Resnick and Walker. ISBN 0-471-23231-9