Physics Lab
Physics Lab
IntroductionStudy
Guide
Practice
Problems
AP®-Style
Questions
LessonExample
Problems
Other
Resources
Help
  Complete and Continue  

Orbital Motion

Introduction

We learned that all objects attract each other with a gravitational force. The earth and the moon attract each other, the earth and the sun attract each other, and so on. If that's the case, why doesn't the moon crash into the earth? Is there another force pushing the moon away from the earth?

Now that we've learned about gravity, uniform circular motion and centripetal force, let's take a look at something that combines these concepts: orbital motion.

An orbit is the circular or elliptical path of an object as it moves around another object, with only the force of gravity acting on it. The moon and thousands of satellites are in orbit around the earth, and the earth and the other planets are in orbit around the sun. Since gravity is the only force involved, we'll see how objects in orbit are really in projectile motion or free fall and have zero apparent weight.

If an orbit is a circle, gravity is the centripetal force causing the circular motion. That means we can combine the equations for gravitational force and centripetal force to find the object's orbital radius, speed and period.

We'll cover orbital motion energy in another lesson.

Study Guide

Download:Orbital Motion - Study Guide.pdf
Practice Problems

Download:Orbital Motion - Practice Problems.pdf
Orbital Motion
Orbital motion practice problem 1
Show answer
Orbital motion practice problem answer 1Orbital motion practice problem 2
Show answer
Orbital motion practice problem answer 2Orbital motion practice problem 3
Show answer
Orbital motion practice problem answer 3
AP®-Style Questions

Multiple-Choice Questions

Preview of the AP Physics 1 multiple choice questions (MCQ) for orbital motion and circular orbits
Lesson
Example Problems
Other Resources
Help
Complete and Continue