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Centripetal Force Equation

Reference from the original Physics I textbook.

Centripetal Force Equation

Radial net force magnitude: F_c = mv²/r. Its direction is inward toward the center.

F→=Force(N)​
m=mass(kg)​
v→=velocity(m/s)​
r=radius(m)

[1Newton=kg⋅m/s2]

Related Glossary Terms

Centripetal Accelerationⓘ, Centripetal Acceleration Equation, Uniform Circular Motion

Index

Chapter 6 - Circular Motion

Chapter 6 - FFR - Rotational Energy

Reviewed physics notes (1)

These corrections keep the original lesson’s purpose while fixing errors in the source edition.

  • Centripetal force equation uses speed squared and a radial direction. — Reference 1

About this edition and its source ↗

Glossary and deeper reading · 2 refreshers

These editorial refreshers supplement the reading. Definitions and examples are added guidance; original source wording and recorded answers remain in their original context.

  • Centripetal force

    Centripetal force names the inward net-force component required for motion along a circular path. It is supplied by actual interactions such as tension, friction, gravity, or normal forces rather than being an additional type of force. For example, gravity supplies the centripetal force on a satellite in a circular orbit.

    Read more: Uniform circular motion →

  • Centripetal acceleration

    Centripetal acceleration is the inward acceleration component that changes the direction of motion along a curved path. For circular motion its magnitude is speed squared divided by the circle’s radius. For example, a car moving at constant speed around a bend still has centripetal acceleration.

    Read more: Uniform circular motion →

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