Many motions, such as the arc of a bird’s flight or Earth’s path around the Sun, are curved. Recall that Newton’s first law tells us that motion is along a straight line at constant speed unless there is a net external force. We will therefore study not only motion along curves, but also the forces that cause it, including gravitational forces. In some ways, this chapter is a continuation of Dynamics: Newton's Laws of Motion as we study more applications of Newton’s laws of motion.
This chapter deals with the simplest form of curved motion, uniform circular motion, motion in a circular path at constant speed. Studying this topic illustrates most concepts associated with rotational motion and leads to the study of many new topics we group under the name rotation. Pure rotational motion occurs when points in an object move in circular paths centered on one point. Pure translational motion is motion with no rotation. Some motion combines both types, such as a rotating hockey puck moving along ice.
Rotation Angle and Angular Velocity
Kinematics of Rotational Motion
Fictitious Forces and Non-inertial Frames: The Coriolis Force
Newton’s Universal Law of Gravitation
Angular Motion Variables
Uniform Circular Motion
Distance or Arc Length
Angular Velocity vs Speed
Rotational Motion
Centripetal Force and Acceleration
Centripetal Acceleration
Centripetal Problem Solving
(All 26 Videos)