Centripetal Force — F = mv²/r
The centripetal force formula F = mv²/r explained: why circular motion needs an inward force, and a worked car-cornering example.
What it means
Anything moving in a circle is accelerating toward the center — even at constant speed — because its velocity direction keeps changing. Centripetal force is the name for whatever net inward force causes that acceleration: friction for a cornering car, tension for a whirling ball on a string, gravity for an orbiting satellite. The dependence is the striking part: doubling the speed demands four times the inward force, which is why fast corners are treacherous. There is no outward 'centrifugal force' in an inertial frame — what you feel pressed against the car door is your body's inertia resisting the inward acceleration.
Variables
| Symbol | Name | Unit | Meaning |
|---|---|---|---|
| Centripetal force | N | Net inward force causing circular motion | |
| Mass | kg | Mass of the circulating object | |
| Speed | m/s | Tangential speed along the circle | |
| Radius | m | Radius of the circular path |
Assumptions
- Speed is constant (uniform circular motion)
- Circular path of fixed radius r
- Net force considered — individual forces like friction provide it
Derivation
In uniform circular motion the velocity vector rotates at angular speed . The rate of change of velocity is directed toward the center. Newton's second law then gives .
Worked example
A 1000 kg car takes a flat curve of radius 50 m at 15 m/s. What centripetal force keeps it on the curve?
Given:
- m = 1000 kg
- v = 15 m/s
- r = 50 m
Write the formula:
Substitute:
Calculate: , so
The tires must supply 4500 N of inward grip — about 0.46 g of lateral acceleration. If the road is wet and friction cannot provide it, the car slides outward: not because a force pushes it out, but because nothing pulls it in.