Rotation of a rigid object P about a fixed object about a fixed axis O.
Angular displacement of a body is the angle in radians (degrees, revolutions) through which a point or line has been rotated in a specified sense about a specified axis. When an object rotates about its axis, the motion cannot simply be analyzed as a particle, since in circular motion it undergoes a changing velocity and acceleration at any time (t). When dealing with the rotation of an object, it becomes simpler to consider the body itself rigid. A body is generally considered rigid when the separations between all the particles remains constant throughout the objects motion, so for example parts of its mass are not flying off. In a realistic sense, all things can be deformable, however this impact is minimal and negligible. Thus the rotation of a rigid body over a fixed axis is referred to as rotational motion.
Example
In the example illustrated to the right, a particle on object P at a fixed distance r from the origin, O, rotating counterclockwise. It becomes important to then represent the position of particle P in terms of its polar coordinates (r, θ). In this particular example, the value of θ is changing, while the value of the radius remains the same. (In rectangular coordinates (x, y) both x and y vary with time). As the particle moves along the circle, it travels an arc length s, which becomes related to the angular position through the relationship:

s=r\theta \,
Measurements of angular displacement
Angular displacement may be measured in radians or degrees. If using radians, it provides a very simple relationship between distance traveled around the circle and the distance r from the centre.

\theta=\frac sr
For example if an object rotates 360 degrees around a circle of radius r, the angular displacement is given by the distance traveled around the circumference  which is 2πr divided by the radius: \theta= \frac{2\pi r}r which easily simplifies to \theta=2\pi. Therefore 1 revolution is 2\pi radians.
When object travels from point P to point Q, as it does in the illustration to the left, over \delta t the radius of the circle goes around a change in angle. \Delta \theta = \Delta \theta_2  \Delta \theta_1 which equals the Angular Displacement.
Three dimensions
In three dimensions, angular displacement is an entity with a direction and a magnitude. The direction specifies the axis of rotation, which always exists by virtue of the Euler's rotation theorem; the magnitude specifies the rotation in radians about that axis (using the righthand rule to determine direction).
Despite having direction and magnitude, angular displacement is not a vector because it does not obey the commutative law for addition.^{[1]}
Matrix notation
Given that any frame in the space can be described by a rotation matrix, the displacement among them can also be described by a rotation matrix. Being A_0 and A_f two matrices, the angular displacement matrix between them can be obtained as dA = A_f . A_0^{1}
References

^ Kleppner, Daniel; Kolenkow, Robert (1973). An Introduction to Mechanics. McGrawHill. pp. 288–89.
See also


Linear/translational quantities


Angular/rotational quantities

time: t
s



time: t
s




displacement, position: x
m



angular displacement, angle: θ
(rad)


frequency: f
s^{−1}, Hz

speed: v, velocity: v
ms^{−1}


frequency: f
s^{−1}, Hz

angular velocity: ω
(rad)s^{−1}



acceleration: a
ms^{−2}



angular acceleration: α
(rad)s^{−2}



jerk: j
ms^{−3}



angular jerk: ζ
(rad)s^{−3}








mass: m
kg



moment of inertia: I
kgm^{2}(rad^{−2})




momentum: p, impulse: J
kgms^{−1}, Ns



angular momentum: L, angular impulse: ΔL
kgm^{2}s^{−1}(rad^{−1})



force: F, weight: F_{g}
kgms^{−2}, N

energy: E, work: W
kgm^{2}s^{−2}, J


torque: τ, moment: M
kgm^{2}s^{−2}(rad^{−1}), Nm

energy: E, work: W
kgm^{2}s^{−2}, J


yank: Y
kgms^{−3}, Ns^{−1}

power: P
kgm^{2}s^{−3}, W


rotatum: P
kgm^{2}s^{−3}(rad^{−1})

power: P
kgm^{2}s^{−3}, W



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