Centripetal force is the force that keeps an object moving in a circular path. It is always directed towards the center of the circle. This force allows an object to continuously change direction without changing its speed.
Key Concepts
Centripetal Force: The force that keeps an object moving in a circular path.
Centripetal Force Equation: Fc = mv^2/r, where Fc is the centripetal force, m is the mass of the object, v is the velocity, and r is the radius of the circular path.
Examples of Centripetal Force: Examples include the gravitational force that keeps planets in orbit around the Sun, the tension in a string that keeps a ball moving in a horizontal circle, and the frictional force on a car's tires as it rounds a curve.
Study Guide
Here are some key points to remember when studying centripetal force:
Understand the concept of centripetal force and how it is related to circular motion.
Be able to calculate the centripetal force using the equation Fc = mv^2/r.
Identify and explain examples of centripetal force in real-life situations.
Explain how Earth's fluid outer core creates the magnetosphere and how this helps protect both humans and technology (such as satellites) from solar winds.