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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