Centripetal Force Calculator

Calculate centripetal force and acceleration from mass, velocity, and radius. Solve from linear or angular velocity, orbital periods. Find g-force, banking angle, and minimum loop speed.

Centripetal Force (N)
Centripetal Acceleration (m/s²)
G-Force
Extended More scenarios, charts & detailed breakdown
Centripetal Force F = mv²/r (N)
Centripetal Acceleration (m/s²)
G-Force
Professional Full parameters & maximum detail

Core Results

Centripetal Force (N)
Centripetal Acceleration (m/s²)
G-Force

Engineering Applications

Ideal Banking Angle (degrees)
vs Gravitational Force
Min Speed for Vertical Loop (m/s)
Orbital Velocity at this Radius (m/s)

How to Use This Calculator

  1. Enter mass (kg), velocity (m/s), and radius (m) for instant centripetal force and acceleration.
  2. Use From Angular Velocity if you know ω (rad/s) instead of linear speed.
  3. Use Orbital tab for satellite/orbital calculations using period and radius.
  4. Switch to Professional for g-force, ideal banking angle, minimum loop speed, and gravitational force comparison.

Formula

F = mv²/r (from linear velocity)

F = mω²r (from angular velocity)

a = v²/r = ω²r

Banking angle θ = arctan(v²/rg)

Min loop speed v = √(gr)

Example

Example: 2 kg mass, 10 m/s, 5 m radius. a = 10²/5 = 20 m/s². F = 2 × 20 = 40 N. G-force = 20/9.81 = 2.04 g.

Frequently Asked Questions

  • Centripetal force is the net force that keeps an object moving in a circular path, directed toward the center. F = mv²/r, where m = mass, v = velocity, r = radius. It is not a separate force — it is the name for the net inward force (gravity, tension, friction, etc.).
  • Centripetal force is real — it is the inward force that causes circular motion. Centrifugal force is a fictitious force felt in a rotating reference frame (the apparent "outward push"). In an inertial frame, only centripetal force exists.
  • If you know angular velocity ω (rad/s): F = mω²r and a = ω²r. Linear velocity v = ωr. Use the "From Angular Velocity" tab for this calculation.
  • θ = arctan(v²/rg). For a car at 20 m/s on a curve of radius 50 m: θ = arctan(400/490) ≈ 39.3°. This angle eliminates the need for friction to maintain the curve.
  • At the top of a loop, centripetal force must at least equal gravity: mv²/r ≥ mg, so v_min = √(gr). Below this speed, the object falls away from the circular path.

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