57 minutes
- Introduction
- Lecture 01
- Lecture 02
- Lecture 03
- Lecture 3, Part 1: Introduction
- Lecture 3, Part 2: Where Were We
- Lecture 3, Part 3: Vector Components in Detail
- Lecture 3, Part 4: Scalar Component Description
- Lecture 3, Part 5: Example of Finding Scalar Components
- Lecture 3, Part 6: Scalar Component Addition
- Lecture 3, Part 7: Scalar Addition Example
- Lecture 3, Part 8: Motion Diagrams
- Lecture 04
- Lecture 05
- Lecture 5, Part 01: Introduction
- Lecture 5, Part 02: Where Were We
- Lecture 5, Part 03: Big Picture: 1D Kinematics
- Lecture 5, Part 04: Kinematic Problem Solving Steps
- Lecture 5, Part 05: Example 1
- Lecture 5, Part 06: Example 2
- Lecture 5, Part 07: Example 3
- Lecture 5, Part 08: Free Fall
- Lecture 5, Part 09: Free Fall and Kinematic Equations
- Lecture 5, Part 10: Example 4
- Lecture 5, Part 11: Example 5
- Lecture 06
- Lecture 07
- Lecture 08
- Lecture 09
- Lecture 10
- Lecture 11
- Lecture 11, Part 1: Introduction
- Lecture 11, Part 2: Where Were We
- Lecture 11, Part 3: Free Body Diagram and Vector Nature of Newton’s 2nd Law
- Lecture 11, Part 4: Common Forces: Weight
- Lecture 11, Part 5: Common Forces: Tension
- Lecture 11, Part 6: Common Forces: Normal Force
- Lecture 11, Part 7: Common Forces: Friction
- Lecture 11, Part 8: Problem Solving Steps
- Lecture 11, Part 9: Example
- Lecture 12
- Lecture 13
- Lecture 13, Part 1: Introduction and Where Were We?
- Lecture 13, Part 2: Why/When Do We Need Newton’s Third Law?
- Lecture 13, Part 3: Newton’s 3rd Law
- Lecture 13, Part 4: Changes To Our Problem-Solving Steps
- Lecture 13, Part 5: Example 1
- Lecture 13, Part 6: Ropes and Pulleys
- Lecture 13, Part 7: Example 2
- Lecture 13, Part 8: Your Turn
- Lecture 14
- Lecture 14, Part 01: Introduction
- Lecture 14, Part 02: Where Were We ?
- Lecture 14, Part 03: Uniform Circular Motion: What You Need To Know
- Lecture 14, Part 04: Example 1
- Lecture 14, Part 05: Example 2
- Lecture 14, Part 06: Example 3
- Lecture 14, Part 07: Optional Roller Coaster Example
- Lecture 14, Part 08: Satellite Example
- Lecture 14, Part 09: The Universal Law of Gravitation
- Lecture 14, Part 10: Satellite Example Continued
- Lecture 15
- Lecture 15, Part 1: Introduction and Where Were We?
- Lecture 15, Part 2: Energy Conservation: The Basics
- Lecture 15, Part 3: How Do You Calculate the Net Work?
- Lecture 15, Part 4: New Problem Solving Steps
- Lecture 15, Part 5: Example 1
- Lecture 15, Part 6: Example 2
- Lecture 15, Part 7: Last Example
- Lecture 15, Part 8: Final Quiz Questions…
- Lecture 16
- Lecture 16, Part 1: Introduction and Where Were We?
- Lecture 16, Part 2: Defining Our New “Energy Conservation Starting Equation”
- Lecture 16, Part 3: Defining Mechanical Energy
- Lecture 16, Part 4: New Problem Solving Steps
- Lecture 16, Part 5: First Example
- Lecture 16, Part 6: Second Example
- Lecture 16, Part 7: Last Example
- Lecture 16, Part 8: Redo Example From Last Lecture
- Lecture 17
- Lecture 18
- Lecture 19
- Lecture 20
- Lecture 21
- Lecture 22
- Lecture 22, Part 1: Introduction and Where Were We?
- Lecture 22, Part 2: A Net Torque Causes Angular Acceleration
- Lecture 22, Part 3: Torque Example
- Lecture 22, Part 4: Equilibrium Example
- Lecture 22, Part 5: Moment of Inertia
- Lecture 22, Part 6: Non-Equilibrium Example
- Lecture 22, Part 7: Another Example
- Lecture 23
- Lecture 24
- Lecture 25