Rotational Kinematics

Claimed by Aditya Kuntamukkula 2017

The Main Idea

Rotational Motion (also known as curvilinear motion), in contrast to linear ( also known as rectilinear) motion, involves motion of objects where the angular position of an object changes over time (For this reason, it is common practice to use polar coordinates when analyzing any object undergoing rotational motion). Because of this, rotational quantities are often called angular quantities, as they describe the angular component of an object's motion.

A Mathematical Model

Similar to linear motion, angular quantities can be described by a series of differential equations which relate the rate of change of a given quantity to some other aspect of rotational motion. These equations are listed below:

[math]\displaystyle{ \boldsymbol{\omega} = \frac{d\boldsymbol{\theta}}{dt} }[/math]

[math]\displaystyle{ \boldsymbol{{\alpha}} = \frac{d\boldsymbol{\omega}}{dt} }[/math]

[math]\displaystyle{ \boldsymbol{{\alpha}} = \frac{{d}^{2}\boldsymbol{\omega}}{{dt}^{2}} }[/math]

Here [math]\displaystyle{ \boldsymbol{\theta} }[/math] represents angular position, [math]\displaystyle{ \boldsymbol{\omega} }[/math] represents angular velocity, and [math]\displaystyle{ \boldsymbol{\alpha} }[/math] represents angular acceleration. One can also approximate the rotational motion of an object by using the discrete time equations of motion, as listed below:

[math]\displaystyle{ \boldsymbol{\omega} = \frac{\Delta\boldsymbol{\theta}}{{\Delta}t} }[/math]

[math]\displaystyle{ \boldsymbol{\alpha} = \frac{\Delta\boldsymbol{\omega}}{{\Delta}t} }[/math]

Angular velocity always has units of radians per time (radians/seconds, radians/minutes, or radians/hour)

Objects undergoing rotational motion, just like objects undergoing linear motion, can be analyzed using kinematics, and in principle, by using the relationships above, it is possible to solve for every aspect of an object's rotational motion. However, depending upon the complexity of the motion, this task may prove extremely difficult, so, more often than not special cases are considered, such as "rotation about a fixed axis" or "uniform circular motion". While these special cases may make simplifications about certain aspects of the object's motion, they still make use of the same equations of motion, and thus are still rotational kinematics problems. A special case of particular importance however is the case in which an object in undergoing uniform angular acceleration. In this case, it is possible to derive equations analogous to the Uniformly accelerated motion equations from linear kinematics. These equations are listed below:

[math]\displaystyle{ \boldsymbol{\omega} = {\omega}_{0} + \boldsymbol{\alpha}t }[/math]

[math]\displaystyle{ \boldsymbol{\theta} = \frac{1}{2}\boldsymbol{\alpha}{t}^{2} + {\omega}_{0}t + {\theta}_{0} }[/math]

[math]\displaystyle{ \boldsymbol{{\omega}}^{2} = {{\omega}_{0}}^{2} + 2\boldsymbol{\alpha}(\boldsymbol{\theta} - {\theta}_{0}) }[/math]

Examples

Simple

A simple example and application of the concept of rotation is the earth's rotation on it's axis. It rotates once every 24 hours. What is the angular velocity?

[math]\displaystyle{ \boldsymbol{{w}} = \frac{\boldsymbol{d\theta}}{\boldsymbol{dt}} }[/math]

[math]\displaystyle{ \boldsymbol{{w}} = \frac{\boldsymbol{\delta\theta}}{\boldsymbol{\delta t}} }[/math]

[math]\displaystyle{ \boldsymbol{{w}} = \frac{\boldsymbol{2\pi}}{\boldsymbol{24}}\frac{\boldsymbol{rad}}{\boldsymbol{hr}} }[/math]

[math]\displaystyle{ \boldsymbol{{w}} = \frac{\boldsymbol{\pi}}{\boldsymbol{12}}\frac{\boldsymbol{rad}}{\boldsymbol{hr}} }[/math]

[math]\displaystyle{ \boldsymbol{{w}} = \frac{\boldsymbol{\pi}}{\boldsymbol{12}}\frac{\boldsymbol{rad}}{\boldsymbol{hr}}*\frac{\boldsymbol{1}}{\boldsymbol{3600}}\frac{\boldsymbol{hr}}{\boldsymbol{s}} }[/math]

[math]\displaystyle{ \boldsymbol{{w}} = \frac{\boldsymbol{\pi}}{\boldsymbol{43200}}\frac{\boldsymbol{rad}}{\boldsymbol{s}} }[/math]

Angular velocity can also be represented as change in angle (theta) over change in time. In this case, the earth rotates 2pi radians in 24 hours which reduces to pi/12 rad/hr and that is the equivalent of pi/43200 rad/s.

Medium

A cylinder with a 2.5 ft radius is rotating at 120 rpm. Find the angular velocity in rad/sec. Find the linear velocity of a point on its rim in mph.

[math]\displaystyle{ \boldsymbol{{w}} = {\boldsymbol{120}}\frac{\boldsymbol{rev}}{\boldsymbol{min}}*\frac{\boldsymbol{2\pi}}{\boldsymbol{1}}\frac{\boldsymbol{rad}}{\boldsymbol{rev}}*\frac{\boldsymbol{1}}{\boldsymbol{60}}\frac{\boldsymbol{min}}{\boldsymbol{s}} = {\boldsymbol{4\pi}}\frac{\boldsymbol{rad}}{\boldsymbol{s}} }[/math]

[math]\displaystyle{ \boldsymbol{{v}} = {\boldsymbol{w}}{\boldsymbol{r}} }[/math]

[math]\displaystyle{ \boldsymbol{{v}} = {\boldsymbol{4\pi}}\frac{\boldsymbol{rad}}{\boldsymbol{s}}*{\boldsymbol{2.5}}\frac{\boldsymbol{ft}}{\boldsymbol{rad}} = {\boldsymbol{10\pi}}\frac{\boldsymbol{ft}}{\boldsymbol{s}} }[/math]

[math]\displaystyle{ \boldsymbol{{v}} = {\boldsymbol{10\pi}}\frac{\boldsymbol{ft}}{\boldsymbol{s}}*\frac{\boldsymbol{3600}}{\boldsymbol{1}}\frac{\boldsymbol{s}}{\boldsymbol{hr}}*\frac{\boldsymbol{1}}{\boldsymbol{5280}}\frac{\boldsymbol{miles}}{\boldsymbol{ft}} =\frac{\boldsymbol{75\pi}}{\boldsymbol{11}}\frac{\boldsymbol{miles}}{\boldsymbol{hr}} }[/math]

To find the solution of this problem, rpm (revolutions per minute) should be converted to radians/second. Following this, the linear velocity can be calculated by using the v=wr formula shown above. The angular velocity is 4pi radians per second and the linear velocity is 75pi/11 or 21.42 mph.

Difficult

A tire with a 9 inch radius is rotating at 30 mph. Find the angular velocity at a point on its rim. Also express the result in revolutions per minute.

[math]\displaystyle{ \boldsymbol{{w}} = \frac{\boldsymbol{v}}{\boldsymbol{r}} }[/math]

[math]\displaystyle{ \boldsymbol{{r}} = {\boldsymbol{9}}{\boldsymbol{in}}*\frac{\boldsymbol{1}}{\boldsymbol{12}}\frac{\boldsymbol{ft}}{\boldsymbol{in}}*\frac{\boldsymbol{1}}{\boldsymbol{5280}}\frac{\boldsymbol{miles}}{\boldsymbol{ft}} = \frac{\boldsymbol{1}}{\boldsymbol{7040}}{\boldsymbol{miles}} }[/math]

[math]\displaystyle{ \boldsymbol{{w}} = \frac{\boldsymbol{30}}{\frac{\boldsymbol{1}}{\boldsymbol{7040}}}\frac{\frac{\boldsymbol{miles}}{\boldsymbol{hr}}}{\frac{\boldsymbol{rad}}{\boldsymbol{miles}}} = \boldsymbol{{211200}\frac{\boldsymbol{rad}}{\boldsymbol{hr}}} }[/math]

[math]\displaystyle{ \boldsymbol{{w}} = \boldsymbol{{211200}\frac{\boldsymbol{rad}}{\boldsymbol{hr}}}*\frac{\boldsymbol{1}}{\boldsymbol{2\pi}}\frac{\boldsymbol{rev}}{\boldsymbol{rad}}*\frac{\boldsymbol{1}}{\boldsymbol{60}}\frac{\boldsymbol{hr}}{\boldsymbol{min}} = \frac{\boldsymbol{1760}}{\boldsymbol{\pi}}\frac{\boldsymbol{rev}}{\boldsymbol{min}} }[/math]

Connectedness

Rotation is an extremely important aspect of dynamics (the study of moving objects) which plays a big role in biomechanics. Rotation relates to several important body parts such as the shoulder where there are two axis of rotation, the medial-lateral axis and the anterior-posterior axis. A study of the movement of the shoulder helps to treat medical conditions that may affect this area. Dynamics is also very important in many other disciples, including mechanical engineering and aerospace engineering.

History

The general concept of rotation was well known to those as far back as ancient Egypt. For example, the Egyptians were aware of the fact that when a force was applied to a round object, such as a log, the object would rotate, or roll across the ground. Archimedes also appeared to be aware of a consequence of torque, which he described as "the principle of the lever". He noted in his work that "Magnitudes are in equilibrium at distances reciprocally proportional to their weights" when discussing objects balancing about a pivot. Beyond this point, the first time angular velocity and rotational inertia were discussed by name and given precise definitions were by Thomas Bradwardine and Jean Buridan, respectively. Buridan was notable in that he was also the first to roughly define the notion of angular momentum, as he noted that the celestial bodies maintained rotational motion around the sky, not due to an external force, but because their own inertia (or impedus as he called it) carried them forward, encountering no external resistance. Or, in his own words:

"it could be said that God, in creating the world, set each celestial orb in motion… and, in setting them in motion, he gave them an impetus capable of keeping them in motion without there being any need of his moving them any more." - Jean Buridan

See also

To learn more about Rotation in a more complete context, please refer to Torque or Rigid-Body Objects or Angular Momentum.

Further reading

Books, Articles or other print media on this topic

External links

Some other resources to further understand rotation are the following:

http://www.mathwarehouse.com/transformations/rotations-in-math.php

http://demonstrations.wolfram.com/Understanding3DRotation/

References

[1] Biomechanics, Basic. “It Is Important When Learning about (n.d.): n. pag. Web.

[2] "Angular Velocity and Angular Acceleration." Van Nostrand's Scientific Encyclopedia (2005): n. pag. Web