Angular velocity describes the speed of
rotation and the orientation of the instantaneous axis
about which the rotation occurs. The direction of the angular velocity vector will be along the axis of rotation; in this case
(counter-clockwise rotation) the vector points toward the viewer.
In physics, the angular velocity is a vector
quantity (more precisely, a pseudovector) which specifies the angular speed at which an object is rotating along with the direction in which it is rotating. The
SI unit of angular velocity is radians per second,
although it may be measured in other units such as degrees per second, degrees per hour, etc. When measured in cycles or
rotations per unit time (e.g. revolutions per minute), it is often called the
rotational velocity and its magnitude the rotational speed. Angular velocity is usually
represented by the symbol omega (Ω or ω). The direction of the angular velocity
vector is perpendicular to the plane of rotation, in a direction which is usually specified by the right hand rule.
The angular velocity of a particle
Two dimensions
The angular velocity of the particle at P with respect to the origin O is determined by the
perpendicular component of the velocity vector
V .
The angular velocity of a particle in a 2-dimensional plane is the easiest to understand. As shown in the figure on the right,
if we draw a line from the origin (O) to the particle (P), then the velocity vector (
) of the particle will have a component along
the radius (Failed to parse (unknown function\parallel): \mathrm{v}_\parallel\,
- the radial component) and a component perpendicular to the radius (
- the tangential component).
A radial motion produces no rotation of the particle (relative to the origin), so for purposes of finding the angular velocity
the parallel (radial) component can be ignored. Therefore, the rotation is completely produced by the tangential motion (like
that of a particle moving along a circumference), and the angular velocity is completely determined by the perpendicular
(tangential) component.
It can be seen that the rate of change of the angular position of the particle is related to the tangential velocity by:

Defining ω=dφ/dt as the angular velocity, and realizing that
is equal to
where θ is the
angle between vectors r and v yields:

In two dimensions the angular velocity is a single number which has no direction. A single number which has no direction is
either a scalar or a pseudoscalar, the difference being
that a scalar does not change its sign when the x and y axes are exchanged (or inverted), while a
pseudoscalar does. The angle as well as the angular velocity is a pseudoscalar. The positive direction of rotation is taken, by
convention, to be in the direction towards the y axis from the x axis. If the axes are inverted, but the sense of a
rotation does not, then the sign of the angle of rotation, and therefore the angular velocity as well, will change.
It is important to note that the pseudoscalar angular velocity of a particle depends upon the choice of the origin and upon
the orientation of the coordinate axes.
Three dimensions
In three dimensions, the angular velocity becomes a bit more complicated. The angular velocity in this case is generally
thought of as a vector, or more precisely, a pseudovector. It now has not only a magnitude, but a direction as well. The magnitude is the angular speed,
and the direction describes the axis of rotation. The right
hand rule indicates the positive direction of the angular velocity pseudovector, namely:
- If you curl the fingers of your right hand to follow the direction of the rotation, then the direction of the angular
velocity vector is indicated by your right thumb.
Just as in the two dimensional case, a particle will have a component of its velocity along the radius from the origin to the
particle, and another component perpendicular to that radius. The combination of the origin point and the perpendicular component
of the velocity defines a plane of rotation in which the behavior of the particle (for that instant) appears just as it
does in the two dimensional case. The axis of rotation is then a line perpendicular to this plane, and this axis defined the
direction of the angular velocity pseudovector, while the magnitude is the same as the pseudoscalar value found in the
2-dimensional case. Define a unit vector
which points in the direction of the angular velocity pseudovector. The angular velocity may be written in a
manner similar to that for two dimensions:

which, by the definition of the cross product, can be written:

Higher dimensions
In general, the angular velocity in an n-dimensional space is the time derivative of the angular displacement tensor which is
a second rank skew-symmetric tensor. This tensor will have n(n-1)/2 independent components
and this number is the dimension of the Lie algebra of the Lie
group of rotations of an n-dimensional inner product space. [1] It turns out that in three dimensional space angular
velocity can be represented by vector because number of independent components is equal to number of dimensions of space.
Angular velocity of a rigid body
Position of point P located in the rigid body (shown in blue).
Ri is the position with respect to the lab
frame, centered at
O and
ri is the position with respect to the rigid body frame, centered at
O' . The origin of the rigid body frame is at vector position
R from the lab frame.
In order to deal with the motion of a rigid body, it is best to consider a coordinate
system that is fixed with respect to the rigid body, and to study the coordinate transformations between this coordinate and the
fixed "laboratory" system. As shown in the figure on the right, the lab system's origin is at point O, the rigid body system
origin is at O' and the vector from O to O' is R. A particle (i) in the rigid body is located at point P and the
vector position of this particle is Ri in the lab frame, and at position ri in the body
frame. It is seen that the position of the particle can be written:

The defining characteristic of a rigid body is that the distance between any two points in a rigid body is unchanging in time.
This means that the length of the vector
is unchanging. By Euler's rotation theorem, we may
replace the vector
with
where
is a
rotation matrix and
is the position of the particle at some
fixed point in time, say t=0. This replacement is useful, because now it is only the rotation matrix
which is changing in time and not the
reference vector
,
as the rigid body rotates about point O'. The position of the particle is now written as:

Taking the time derivative yields the velocity of the particle:

where Vi is the velocity of the particle (in the lab frame) and V is the velocity of O' (the origin
of the rigid body frame). The velocity of the particle is given by:

Where Ω is the angular velocity tensor. If we take the dual of the angular
velocity tensor, we get the angular velocity pseudovector
![\boldsymbol\omega=[\omega_x,\omega_y,\omega_z]](http://content.answers.com/main/content/wp/en/math/5/8/1/5810838dc3a55cc2da8a4b59194e35fe.png)
and the matrix multiplication is replaced by the cross product, yielding:

It can be seen that the velocity of a point in a rigid body can be divided into two terms - the velocity of a reference point
fixed in the rigid body plus the cross product term involving the angular velocity of the particle with respect to the reference
point. This angular velocity is the "spin" angular velocity of the rigid body as opposed to the angular velocity of the reference
point O' about the origin O.
It is an important point that the spin angular velocity of every particle in the rigid body is the same, and that the
spin angular velocity is independent of the choice of the origin of the rigid body system or of the lab system. In other words,
it is a physically real quantity which is a property of the rigid body, independent of one's choice of coordinate system. The
angular velocity of the reference point about the origin of the lab frame will, however, depend on these choices of coordinate
system. It is often convenient to choose the center of mass of the rigid body as the
origin of the rigid body system, since a considerable mathematical simplification occurs in the expression for the
angular momentum of the rigid body.
See also
References
- ^ Rotations and Angular Momentum on the Classical Mechanics page of the website of John Baez, especially
Questions 1 and 2.
- Symon, Keith (1971). Mechanics. Addison-Wesley, Reading, MA. ISBN
0-201-07392-7.
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