Calculate centripetal force (F = mv²/r) for circular motion. Solve for force, mass, velocity, or radius with G-force analysis and real-world examples.
Centripetal force is the real, inward-directed force that keeps an object moving in a circular path. Without it, the object would fly off in a straight line due to inertia (Newton's first law). For a car on a curve, friction provides the centripetal force; for a satellite in orbit, gravity provides it; for a ball on a string, tension provides it.
This calculator solves the centripetal force equation F = mv²/r for any unknown variable: force, mass, velocity, or radius. It also computes centripetal acceleration, G-force loading, angular velocity, orbital period, and kinetic energy. Presets include cars on curves, satellites, roller coasters, and particle physics.
A speed comparison table shows how centripetal force changes at different velocities (force scales with v²), and a real-world examples table puts the results into engineering and physics context.
Use the preset examples to load common values instantly, or type in custom inputs to see results in real time. The output updates as you type, making it practical to compare different scenarios without resetting the page.
Centripetal force calculations are fundamental in vehicle dynamics (safe curve speeds), amusement park engineering (ride forces), aerospace (orbital mechanics), and physics education. The four-variable solver eliminates manual algebra.
The G-force context, speed comparison table, and real-world examples table make it easy to validate results and understand whether a circular motion scenario is physically realistic or approaching limits.
F = mv²/r = mω²r. Centripetal acceleration a = v²/r. Angular velocity ω = v/r. Period T = 2πr/v = 2π/ω. G-force = a / 9.81.
Result: 12,000 N (0.82 G)
A 1,500 kg car traveling at 20 m/s (72 km/h) on a curve of 50 m radius needs 12,000 N of centripetal force — provided by tire friction. The 0.82 G lateral acceleration is near the adhesion limit of standard tires on dry road (about 0.8-1.0 G).
Highway curve design uses the centripetal force equation to determine safe speeds. The maximum speed for a flat curve is v = √(μgr), where μ is the friction coefficient. Banked curves add a normal force component, raising the safe speed to v = √(r × g × tan(θ + arctan(μ))). Modern highway design typically uses 4-8% superelevation combined with friction.
For any orbit, centripetal force equals gravitational force: mv²/r = GMm/r². This gives the orbital velocity v = √(GM/r) and the orbital period T = 2π√(r³/GM) — Kepler's third law. Every satellite, planet, and star system obeys this balance between gravity and centripetal acceleration.
Charged particles in a magnetic field follow circular paths with F = qvB providing the centripetal force. The radius r = mv/(qB) directly reveals the particle's momentum, which is how bubble chambers and tracking detectors measure particle properties. The Large Hadron Collider uses 8.3 Tesla superconducting magnets to bend 7 TeV protons around a 27 km ring.
Different physical forces provide centripetal force in different scenarios: friction for a car on a curve, gravity for an orbiting satellite, tension for a ball on a string, normal force for a banked turn, and electromagnetic force for charged particles in a magnetic field. Use this as a practical reminder before finalizing the result.
No. Centripetal force is a real force directed toward the center of the circle. Centrifugal force is an apparent (fictitious) force felt in the rotating reference frame, directed outward. They have the same magnitude but centripetal is real and centrifugal exists only in non-inertial frames.
Doubling speed quadruples the force because faster objects have more inertia to overcome per unit time, and the required direction change rate also increases. This is why speeding on curves is so dangerous — centripetal force demand grows much faster than speed.
The object moves outward from the circular path. For a car, this means skidding off the curve. For an orbiting object, it means spiraling outward. The maximum centripetal force available sets the maximum safe speed for a given turn radius.
A banked road tilts the normal force inward, providing a component of centripetal force without relying entirely on friction. The ideal banking angle θ satisfies tan(θ) = v²/(rg), allowing the turn at one specific speed with zero friction needed.
At the equator, the centripetal acceleration from Earth's rotation is about 0.034 m/s² (0.0035 G) — tiny compared to gravity. This is why you don't feel it, but it does slightly reduce your effective weight at the equator compared to the poles.