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   » » Wiki: Angular Displacement
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The angular displacement (symbol θ, , or φ) – also called angle of rotation, rotational displacement, or rotary displacement – of a is the (with the unit , degree, turn, etc.) through which the body (revolves or spins) around a centre or axis of rotation. Angular displacement may be signed, indicating the sense of rotation (e.g., ); it may also be greater (in ) than a full turn.


Context
When a body rotates about its axis, the motion cannot simply be analyzed as a particle, as in it undergoes a changing velocity and acceleration at any time. When dealing with the rotation of a body, 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 body's 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.


Example
In the example illustrated to the right (or above in some mobile versions), a particle or body P is 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 .


Definition and units
Angular displacement may be expressed with the unit or degree. Using the radian provides a very simple relationship between distance traveled around the circle ( ) and the distance r from the centre ( ):
\theta = \frac{s}{r} \mathrm{rad}

For example, if a body rotates 360° around a circle of radius r, the angular displacement is given by the distance traveled around the circumference - which is 2π r - divided by the radius: \theta= \frac{2\pi r}r which easily simplifies to: \theta=2\pi. Therefore, 1 revolution is 2\pi radians.

The above definition is part of the International System of Quantities (ISQ), formalized in the international standard ISO 80000-3 (Space and time), [1] (11 pages) and adopted in the International System of Units (SI). Https://nvlpubs.nist.gov/nistpubs/Legacy/SP/nistspecialpublication811e2008.pdf" target="_blank" rel="nofollow">[2]

Angular displacement may be signed, indicating the sense of rotation (e.g., ); it may also be greater (in ) than a full turn. In the ISQ/SI, angular displacement is used to define the number of revolutions, , a ratio and hence a quantity of dimension one.


In 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 about that axis (using the to determine direction). This entity is called an .

Despite having direction and magnitude, angular displacement is not a vector because it does not obey the for addition.

(1973). 9780070350489, McGraw-Hill. .
Nevertheless, when dealing with infinitesimal rotations, second order infinitesimals can be discarded and in this case commutativity appears.


Rotation matrices
Several ways to describe rotations exist, like or . See charts on SO(3) for others.

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 . When this product is performed having a very small difference between both frames we will obtain a matrix close to the identity.

In the limit, we will have an infinitesimal rotation matrix.


Infinitesimal rotation matrices

See also


Sources
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