This lecture covers the concept of angular momentum for rotational motion around a point, explaining how it can be calculated similarly to torque. It discusses examples of uniform circular motion and rectilinear motion, emphasizing the constant angular momentum in circular motion. Additionally, it explores Kepler's laws, focusing on the second law which states that the areal velocity of a planet is constant. The lecture concludes by examining the implications of this law and verifying it for circular trajectories.
This video is available exclusively on Mediaspace for a restricted audience. Please log in to MediaSpace to access it if you have the necessary permissions.
Watch on Mediaspace