# Circular Motion & Gravitation — AP Physics 1
Circular motion and gravitation connect Newton's laws to the motion of planets, satellites, and everyday objects moving in curves. AP Physics 1 tests your understanding of centripetal acceleration, the forces that produce circular motion, Newton's law of universal gravitation, and the basics of orbital mechanics.
Key Concepts
Uniform Circular Motion
An object moving in a circle at constant speed has a continuously changing velocity direction, meaning it accelerates.
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Centripetal acceleration (directed toward the center):
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Centripetal force (net force toward center):
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Period:
Centripetal force is not a new type of force — it is the net inward force provided by tension, gravity, friction, normal force, etc.
Newton's Law of Universal Gravitation
where .
Gravitational Field Strength
At Earth's surface, .
Orbital Motion
For a satellite in circular orbit, gravity provides the centripetal force:
Kepler's Third Law
Worked Example
Problem: A car travels around a flat circular track of radius at . What minimum coefficient of static friction is needed?
Solution:
The friction force provides centripetal force:
Normal force on flat ground: .
Practice Questions
1. A ball on a string swings in a horizontal circle with period . What is the centripetal acceleration?
. .
2. Calculate the gravitational force between Earth () and a person on the surface ().
.
3. A satellite orbits Earth at altitude above the surface. What is its orbital speed? (Use )
. .
4. If the orbital radius doubles, by what factor does the orbital period change?
. Factor = .
Want to check your answers and get step-by-step solutions?
Summary
- Centripetal acceleration is , always directed toward the center.
- Centripetal force is the net inward force — identify which real force(s) provide it.
- Gravity follows an inverse-square law: .
- Orbital speed depends on the central mass and orbital radius, not the satellite's mass.
