Module 5: Circular Motion and Newtonian Gravity
Introduction
Much of what we have covered so far has involved motion in one dimension. When we have considered two-dimensional motion, we have taken it to be the superposition of two, one-dimensional problems. However, much of the motion we see around us is in the form of circles, and it not easy to separate into x and y axes. Mathematically, motion in circles is rather different from motion in straight lines, but the underlying laws of physics are the same.
Learning Objectives
Upon completion of this module, students will be able to:
- Extrapolate linear motion to circular motion
- Calculate the acceleration of an object moving at uniform speed in a circle
- Identify centripetal forces
- Apply Newton's Universal Law of Gravitation to solve for the force between two masses
- Explain how Newton's Universal Law of Gravitation relates to the orbits of satellites and the uniform value of "g" at the earth's surface
- Explain the concept of "weightlessness"
- Identify how measurements of "weight" can be misleading
- Explain the origin of tides
- Express how circular motion and Newtonian gravity can be seen in daily occurrences
To Do List
1. Watch Video Lectures (links below)
2. Complete the Practice Problems(links below)
3. Take the Module 5 Quiz
4. Complete the Exam Practice Problems for Module 5
Video Lectures
Lesson 5.1 Circular Motion and Centripetal Acceleration
In this lesson the equation, for circular motion at uniform speed is introduced and the centripetal and centrifugal forces are explained.
- Video: Circular Motion Links to an external site.
- Example:Ball on a String Links to an external site.
- Extra Material (will not be tested): Centripetal Acceleration Derivation Links to an external site.
- Practice Problems Download Practice Problems
- Written Solutions Download Written Solutions
- Video Solutions:
- Test Your Understanding!
Lesson 5.2 Newton's Universal Law of Gravitation
Newton's Universal Law of Gravitation, one of the basic laws of physics, is explained. Examples are done to show how this law leads to stable orbits for satellites at any distance from a planet or star as well as explaining our value of "g". The laws of proportionality are shown to be useful in solving problems to do with orbits.
- Video: Introduction to Newtonian Gravity Links to an external site.
- Video: Newton's Universal Law of Gravitation Links to an external site.
- Example: Stable Orbits Links to an external site.
- Extra Material (will not be tested): Newton's Cannon Applet Links to an external site.
- Practice Problems Download Practice Problems
- Written Solutions Download Written Solutions
- Video Solutions:
- Test Your Understanding!
Lesson 5.3 Applications of Universal Law of Gravitation
Weightlessness is a word that we use frequently, but here we discuss the physics meaning of the word. We show examples of a man standing in an elevator standing on a bathroom scales and moving and/or accelerating up or down. Lastly we cover the origin of tides, and how the sun and the moon both affect our tides and why.
- Video: Weightlessness Part 1 Links to an external site.
- Video: Weightlessness Part 2 Links to an external site.
- Video: The Tides Links to an external site.
- Practice Problems Download Practice Problems
- Written Solutions Download Written Solutions
- Video Solutions:
- Test Your Understanding!
Quiz
Once you have watched the lectures and completed the practice problems, you should demonstrate your understanding by taking the Module 5 Quiz. Be sure to submit the quiz before its deadline.
Coming Up
In the next module we will learn about Work and Energy and after that you will have your first exam. The Exam 1 Review is already available.