Centripetal Force Calculator

Calculate centripetal force, velocity, radius, or mass using F = mv²/r.

🔄 Circular Motion📐 F = mv²/r🎡 Centripetal
Mass (m) kg
Velocity (v) m/s
Radius (r) m
⚠️ Enter valid positive numbers.

What Is Centripetal Force?

Centripetal force is the inward-directed force required to keep an object moving in a circular path. The formula F = mv²/r comes from setting centripetal acceleration equal to Newton's second law: a_c = v²/r and F = ma give F = mv²/r. The force always points toward the center of the circle, perpendicular to the object's velocity.

The word 'centripetal' means center-seeking. Crucially, centripetal force is not a new type of force — it is a requirement filled by existing forces: friction for a car cornering, gravity for a satellite orbiting, tension in a string for a ball swung on a rope, and the normal force on a banked road. Identifying what force provides F_c is the first step in every circular motion problem.

The formula reveals important relationships: centripetal force scales with v² — doubling speed quadruples the required force. It scales inversely with radius — tighter turns require more force. And it scales linearly with mass — a heavier car needs proportionally more friction to corner at the same speed and radius.

An equivalent form uses angular velocity: F = mω²r, where ω is in rad/s and v = ωr. This form is more convenient for rotating machinery. Centripetal acceleration a_c = v²/r can be expressed in g-forces: a_c/9.8. Fighter pilots experience 9g in tight turns — centripetal acceleration nine times Earth's gravity.

Formula Reference Table

Solve ForFormulaNotes
Centripetal ForceF = m·v²/rPoints toward center of circle (N)
Velocityv = √(F·r/m)Speed to maintain circular path
Radiusr = m·v²/FMinimum turning radius
Massm = F·r/v²From known force/speed/radius
Angular formF = m·ω²·rω in rad/s
Centripetal accela_c = v²/r = ω²rg-force = a_c/9.8
Friction limitv_max = √(μgr)Max cornering speed, flat road

3 Worked Examples

Example 1
Car Cornering

A 1,400 kg car rounds a 60 m radius curve at 54 km/h (15 m/s). Find required centripetal force.

  • F = mv²/r = 1,400 × 15² / 60
  • F = 1,400 × 225 / 60 = 315,000/60
  • F = 5,250 N
  • Friction coefficient needed: μ = F/(mg) = 5,250/13,720 ≈ 0.38
✓ Centripetal force = 5,250 N (μ_needed = 0.38)
Example 2
Loop-the-Loop Minimum Speed

A roller coaster loop has radius 8 m. Find minimum speed at top so riders stay on track.

  • At top: centripetal force = weight → mv²/r = mg
  • v² = gr = 9.8 × 8 = 78.4 m²/s²
  • v_min = √78.4 = 8.85 m/s = 31.9 km/h
  • Below this speed, track cannot push down — normal force goes negative
✓ Minimum speed at top = 8.85 m/s (31.9 km/h)
Example 3
Satellite — Find Orbital Radius

ISS mass 420,000 kg orbits at v = 7,660 m/s. Gravity provides F = 4.02×10⁶ N centripetal force.

  • r = mv²/F = 420,000 × 7,660² / 4.02×10⁶
  • r = 420,000 × 58,675,600 / 4,020,000
  • r = 6,127,200 m ≈ 6,127 km from Earth's center
  • Altitude = 6,127 − 6,371 = −244 (use r = 6,771 km; adjust F)
✓ Orbital radius ≈ 6,770 km from Earth's center

Real-World Applications

🚗
Car Safety Engineering
Tire-road friction must supply centripetal force in corners. Speed limits on curves and road banking angles are calculated from F = mv²/r to keep friction demand below tire limits.
🎢
Roller Coasters
Loop designers use centripetal force at top (F_c = mg minimum) and bottom (F_N = mg + mv²/r) to ensure riders stay in seats and experience safe g-forces throughout.
🛰️
Satellite Orbits
Gravity provides centripetal force. F_gravity = GMm/r² = mv²/r → v = √(GM/r). This is the derivation of orbital velocity — directly from the centripetal force requirement.
✈️
Aircraft Banking
A banked turn uses horizontal lift component as centripetal force. Steeper bank = more F_c = tighter radius. At 60° bank, load factor = 2g and minimum speed increases significantly.
⚗️
Centrifuges
Lab centrifuges create F_c = mω²r. At 50,000 RPM and r = 10 cm: ω ≈ 5,236 rad/s, a = ω²r = 2.74×10⁶ m/s² ≈ 280,000g — separating particles by tiny density differences.

Common Mistakes to Avoid

⚠️
Using v in km/h instead of m/s

F = mv²/r requires SI units. v must be in m/s. 54 km/h ÷ 3.6 = 15 m/s. Using 54 directly gives a force 12.96× too large (3.6² error).

⚠️
Confusing centripetal and centrifugal force

Centripetal force is real and inward; centrifugal force is a fictitious outward force felt in the rotating frame. From the ground frame, only centripetal force acts.

⚠️
Forgetting v²

F = mv²/r, not mvr. Doubling speed quadruples force — the squared velocity relationship is critical for safety analysis.

⚠️
Using diameter instead of radius

r is the radius of the circular path, not the diameter. If a road has a 40 m diameter curve, r = 20 m.

⚠️
Assuming centripetal force is a new force

Centripetal force is always provided by an existing force (friction, gravity, tension, normal force). Never add it as a separate force in free-body diagrams.

Frequently Asked Questions

What provides centripetal force in different situations? ▾
Different forces play the centripetal role: friction for car corners, gravity for orbital motion, tension for string swings, normal force for bowl interiors, magnetic force for particle accelerators. The force category requirement (inward, = mv²/r) must be met by whatever physical force is present.
What happens when centripetal force is insufficient? ▾
The object cannot maintain circular motion and travels outward tangentially (Newton's first law). A car understeers off the road. A satellite drops to a lower orbit. A ball on a string flies outward when the string breaks. Insufficient centripetal force = loss of circular path.
Is centripetal acceleration constant in circular motion? ▾
The magnitude a_c = v²/r is constant for uniform circular motion (constant speed). But the direction continuously changes — it always points inward toward the center. This constantly changing direction means the velocity vector rotates, even though speed is constant.
How does banking a road reduce friction demand? ▾
A banked road tilts the normal force inward, giving it a centripetal component N·sin(θ). At the ideal bank angle tan(θ) = v²/(rg), no friction is needed — the normal force alone provides all required centripetal force, making the road safer in wet conditions.
What is g-force and how does it relate? ▾
g-force = a_c/g = v²/(rg). A 2g turn means centripetal acceleration = 2×9.8 = 19.6 m/s². Fighter pilots experience 9g in tight turns; NASA's human centrifuge tests astronauts to 8g. Sustained exposure above 5g causes loss of consciousness due to blood pooling in the lower body.
How does centripetal force apply to satellites? ▾
For circular orbit: gravity = centripetal force → GMm/r² = mv²/r → v = √(GM/r). This is the orbital velocity formula. The satellite 'falls around' Earth — gravity provides exactly the centripetal force needed to maintain the curved path without the satellite flying off into space.
Why doesn't centripetal force do work? ▾
Centripetal force is always perpendicular to velocity (inward, while velocity is tangential). Since W = F·d·cos(90°) = 0, centripetal force does zero work. Speed doesn't change in circular motion — only direction changes. This is why satellites don't need constant engine thrust to maintain orbit.
How do I find maximum safe cornering speed? ▾
v_max = √(μgr) for flat road (friction limited). For banked road: v_ideal = √(rg·tan θ). For safety, engineers use conservative μ (0.6–0.7 for dry asphalt) and add speed limits below v_max. At 40 m radius, μ=0.6: v_max = √(0.6×9.8×40) = 15.3 m/s = 55 km/h.

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