
The lecture shows gravitational potential energy is negative, with zero at infinity and Earth's surface as the reference, and that energy increases as distance grows.
Explore how gravity and centrifugal force from Earth's rotation shape weight on the surface. Learn why the Earth bulges at the equator and why gravity varies from pole to pole.
Explore how Earth's rotation creates a non inertial frame where gravity is opposed by centrifugal force, yielding gravity at the poles (9.83 m/s^2) and at the equator (9.78 m/s^2).
This course in physics explains gravitational interactions. In these lessons, you will learn everything about the law of universal gravitation, its relationship with the laws of dynamics, the Third Law of Kepler, and you will understand why gravitational forces are the weakest that exist in our natural world. This course includes the derivation of all formulas with step-by-step unit conversions and values. Each topic is explained using detailed examples with helpful animations.