Circular motion occurs when an object moves along a circular path. The centripetal force equation, \( F = \frac{mv^2}{R} \), is essential for understanding this motion.
Key concepts include:
- \textbf{Centripetal force}: This inward force keeps the object moving in a circle and points towards the center of rotation.
- \textbf{Centripetal acceleration}: The rate at which the object's velocity changes direction as it travels around the circle.
For an object to maintain circular motion, there must be a force acting towards the center of the circle. This is what keeps the object from flying off in a straight line due to inertia. The centripetal force formula captures the relationship between mass, velocity, radius, and force, making it easier to predict and measure these physical phenomena.