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Boundless Physics
Uniform Circular Motion and Gravitation
Introduction to UCM and Gravitation
Physics Textbooks Boundless Physics Uniform Circular Motion and Gravitation Introduction to UCM and Gravitation
Physics Textbooks Boundless Physics Uniform Circular Motion and Gravitation
Physics Textbooks Boundless Physics
Physics Textbooks
Physics
Concept Version 10
Created by Boundless

Kinematics of UCM

Uniform circular motion is a motion in a circular path at constant speed.

Learning Objective

  • Relate centripetal force and centripetal acceleration to uniform circular motion


Key Points

    • Under uniform circular motion, angular and linear quantities have simple relations. The length of an arc is proportional to the rotation angle and the radius. Also, $v= r \omega$.
    • The acceleration responsible for the uniform circular motion is called centripetal acceleration. It is given as $a_c = r \omega^2 = \frac{v^2}{r}$.
    • Any net force causing uniform circular motion is called a centripetal force. The direction of a centripetal force is toward the center of curvature and its magnitude is $m \frac{v^2}{r} = mr\omega^2$.

Term

  • centripetal

    Directed or moving towards a center.


Full Text

Angular Quantities

Under uniform circular motion, angular and linear quantities have simple relations. When objects rotate about some axis, each point in the object follows a circular arc. The rotation angle is the amount of rotation and is analogous to linear distance. We define the rotation angle $\Delta\theta$ to be the ratio of the arc length to the radius of curvature:

$\displaystyle \Delta \theta = \frac{\Delta s}{r}$ 

Angle $\theta$ and Arc Length $s$

The radius of a circle is rotated through an angle $\Delta\theta$. The arc length $\Delta s$ is described on the circumference.

We define angular velocity $\omega$ as the rate of change of an angle. In symbols, this is $\omega = \frac{\Delta \theta}{\Delta t}$, where an angular rotation $\Delta\theta$ takes place in a time $\Delta t$. From the relation of $s$ and ($\Delta s = r\Delta \theta$), we see:

$\displaystyle v = \frac{\Delta s}{\Delta t} = r \frac{\Delta \theta}{\Delta t} = r \omega$

Under uniform circular motion, the angular velocity is constant. The acceleration can be written as:

$\displaystyle a_c = \frac{dv}{dt} = \omega \frac{dr}{dt} = \omega v = r \omega^2 = \frac{v^2}{r}$

This acceleration, responsible for the uniform circular motion, is called centripetal acceleration.

Centripetal Force

Any force or combination of forces can cause a centripetal or radial acceleration. Just a few examples are the tension in the rope on a tether ball, the force of Earth's gravity on the Moon, friction between roller skates and a rink floor, a banked roadway's force on a car, and forces on the tube of a spinning centrifuge.

Any net force causing uniform circular motion is called a centripetal force. The direction of a centripetal force is toward the center of curvature, the same as the direction of centripetal acceleration. According to Newton's second law of motion, net force is mass times acceleration. For uniform circular motion, the acceleration is the centripetal acceleration: $a = a_c$. Thus, the magnitude of centripetal force $F_c$ is:

$\displaystyle F_c = ma_c = m \frac{v^2}{r} = mr\omega^2$

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