Classical Mechanics
Fall 2016
This first course in the physics curriculum introduces classical mechanics. Historically, a set of core concepts—space, time, mass, force, momentum, torque, and angular momentum—were introduced in classical mechanics in order to solve the most famous physics problem, the motion of the planets. The principles of mechanics successfully described many other phenomena encountered in the world. Conservation laws involving energy, momentum and angular momentum provided a second parallel approach to solving many of the same problems. In this course, we will investigate both approaches: Force and conservation laws. Our goal is to develop a conceptual understanding of the core concepts, a familiarity with the experimental verification of our theoretical laws, and an ability to apply the theoretical framework to describe and predict the motions of bodies.
Readings
- Worked Example on Pulleys and Ropes Constraints Conditions: Chapter 8, Example 8.9
- Worked examples on massive ropes: Chapter 8, Examples 8.3–8.4
- Worked Example-Capstan: Chapter 8, Example 8.1
- Worked Example - Free Fall with Air Drag: Chapter 8, Example 8.12
- Solved Examples: Chapter 10.9 and Chapter 10, Example 10.6
- Solved Example: Chapter 10, Example 10.5
- Collision Theory: Chapter 15
- Static Equilibrium: Chapter 18
- Kinematics of translation and rotation: Chapter 20
- Dynamics of translation and rotation: Chapter 21
Sources
- Course catalogue ↗Historical OpenCourseWare
- MIT OCW syllabus ↗
- MIT OCW readings ↗
- Historical MIT OpenCourseWare offering. Named reading entries and schedule topics are automatically extracted from the linked source pages.