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Circular motion. Centripetal acceleration and force

08/06/2026

The online centripetal acceleration and force simulations on this page will allow you to know and understand much better how are the forces acting in the circular motion of an object. In particular, you will learn what centripetal acceleration and centripetal force are.

This Thematic Unit is part of our Physics collection

STEM OnLine mini dictionary

Centrifugal Force

Apparent force that tends to move a body away from the center of rotation when observed from an accelerated system.

Centripetal Acceleration

Quantity that measures the change in velocity direction of a body following a curved path.

Centripetal Force

Net force directed toward the center of the trajectory that forces a body to follow a curve.

Tangent

Trigonometric ratio defined as the quotient between the opposite side and the adjacent side to an angle.

Tension

Force exerted by a rope or cable that acts as the physical cause of centripetal acceleration.

What are the forces and accelerations of circular motion

Why is a force needed to move in circles? Imagine you’re riding in a car and the driver suddenly swerves to the left. Instantly, you feel your body being pushed toward the right door. Why does this happen? The answer lies in Newton’s First Law, or the principle of inertia: all objects tend to keep moving in a straight line at a constant speed unless something stops them. In circular motion, even though the speedometer always reads the same number (constant speed), the direction of motion changes every millisecond. For a body to stop moving in a straight line and curve its path continuously, it is absolutely necessary to apply a constant force that pulls it toward the center. Without that force, inertia would win out and the object would be flung off in a straight line, following a path tangent to the curve. In physics, we study this phenomenon through the dynamics of circular motion: there can be no rotation without a force to cause it.

Centripetal force and centripetal acceleration

The word “centripetal” comes from Latin and literally means “tending toward the center.” In physics, centripetal force is not a new or mysterious type of force (such as gravity or magnetism), but rather the role that any force plays in causing a body to rotate.

To understand how it works, we must look at Newton’s Second Law. This law tells us that if there is a net force, an acceleration is necessarily generated in that same direction. In a turn, that force pulling toward the center continuously causes centripetal acceleration. It is important to clarify a concept: this acceleration does not make the object go faster or slower, but rather is solely responsible for changing the direction of the velocity vector at every point along the path.

Depending on the specific situation we are analyzing, centripetal force “disguises” itself as various forces of nature:

  • The tension in a rope. When you spin a stone tied to a string, it is the tension in the string that pulls the stone toward your hand.
  • Gravity. It is the centripetal force that keeps the Moon orbiting the Earth or the planets revolving around the Sun.
  • Friction. When a car takes a curve, the friction of the tires against the asphalt is the centripetal force that prevents the vehicle from skidding and veering straight ahead.

 Centripetal Force vs. Centrifugal Force

The most common mistake when studying rotational dynamics is to think that both are real forces that cancel each other out. You’ve surely felt the “force” pushing you outward when riding a fairground ride or in a car taking a sharp turn. We commonly call this centrifugal force (“fleeing from the center”). However, in classical physics, centrifugal force does not exist as a real force.

The fundamental difference between the two boils down to one concept: the observer’s perspective.

Centripetal force

Centripetal force is real. It always exists. It is the force that someone would see from outside the car (an external observer). The observer sees how the asphalt pushes the wheels toward the center of the track to force the car to curve its path.

Centrifugal force

Centrifugal force is apparent (or fictitious). It is experienced only by the passenger inside the rotating system. It is not a real force caused by any object; it is simply the visual effect caused by the inertia of your own body, which resists turning and wants to keep moving in a straight line.

When the car turns left, your body tries to keep going straight due to inertia, causing you to hit the right door. It’s not that some mysterious force is pushing you to the right; it’s that the car is moving to the left beneath you.

The centripetal force formula and its variables

To accurately calculate how much force is needed to keep an object on a circular path, physicists use the fundamental equation of rotational dynamics. This formula relates the body’s mass, its velocity, and the radius of the curve it is tracing:

Fc = m  (v² / r)

To understand how each variable affects the motion (and what will happen when you modify them in the virtual lab), we can analyze the formula as follows:

  • Mass (m). It is directly proportional to the force. If you double the mass of the rotating object, you will need exactly twice the centripetal force to keep it on the same path. Heavier bodies have a harder time rotating due to their greater inertia.
  • Velocity (v). Watch out for this variable! It is squared (v²), which means that velocity is the most critical factor. If you double the speed of a car in a curve, the required centripetal force does not double, but quadruples. This is why high-speed curves are so dangerous.
  • The radius (r). It is inversely proportional to the force because it is on the denominator. The smaller the radius (a very tight curve or a very short line), the greater the centripetal force you must apply. Conversely, very wide curves (large radius) require much less force.

Real-life turning situations

To truly understand how forces work in circular motion, it’s best to analyze what happens in two everyday situations where the force vectors change completely:

Banked curve

If you’ve watched car races or cycling velodromes, you’ve probably noticed that the curves are tilted inward. That tilt is called banking. Thanks to the banking, we don’t rely solely on tire friction; it’s the normal force of the ground itself that tilts and helps push the vehicle toward the center of the track. This allows you to take curves at much higher speeds without skidding.

Roller coaster

The vertical loop on a roller coaster is the ultimate physical challenge. When the car is upside down at the highest point of the loop, two forces act in the same direction (toward the ground): gravity and the force exerted by the track itself. To prevent the car from falling straight down, the speed must be high enough so that the required centripetal force is equal to or greater than the car’s own weight.

STEM OnLine mini dictionary

Centrifugal Force

Apparent force that tends to move a body away from the center of rotation when observed from an accelerated system.

Centripetal Acceleration

Quantity that measures the change in velocity direction of a body following a curved path.

Centripetal Force

Net force directed toward the center of the trajectory that forces a body to follow a curve.

Tangent

Trigonometric ratio defined as the quotient between the opposite side and the adjacent side to an angle.

Tension

Force exerted by a rope or cable that acts as the physical cause of centripetal acceleration.

Explore the exciting STEM world with our free, online, simulations and accompanying companion courses! With them you’ll be able to experience and learn hands-on. Take this opportunity to immerse yourself in virtual experiences while advancing your education – awaken your scientific curiosity and discover all that the STEM world has to offer!

Centripetal acceleration and force simulations

Force on straight motion


Angle between force and velocity


This simulation allows you to change the angle between the force and velocity vectors and check how it affects the trajectory.






Centripetal acceleration


Centripetal force


Space station


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Isaac Newton

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Centripetal force is the net force directed toward the center of a circular path. It is not a new or special type of force; rather, it is the resultant of the real forces acting toward the center—such as tension, gravity, friction, or a combination of them. Its purpose is to continuously change the direction of the object’s velocity, keeping it on a curved path instead of moving in a straight line. Without this inward‑directed force, the object would follow a straight trajectory due to inertia. This makes centripetal force essential for understanding systems like orbiting satellites, vehicles taking a curve, rotating machinery, and any situation where an object follows a circular path.
Centripetal force increases with the square of the speed and decreases as the radius becomes larger. This means that even a small increase in speed dramatically raises the force required to maintain the circular path, while a wider curve reduces the demand. This relationship has major practical implications: a vehicle needs much more friction to take a tight curve at high speed; a rotating machine experiences rapidly increasing internal stresses as its angular speed rises; and orbital mechanics depend critically on the balance between speed and radius. Understanding this dependency is key to predicting when a system will remain stable and when it will fail to maintain circular motion.
It makes perfect sense. What you feel is not an outward force but your own inertia. Your body wants to continue moving in a straight line while the car turns underneath you. Because the seat or the door pushes you inward to force you into the curve, you perceive a pressure outward. That sensation is an inertial effect, not a physical force acting away from the center.
If the available centripetal force is smaller than what the motion requires for that speed and radius, the object can no longer follow the curve. At that moment, inertia takes over and the object leaves the circular path along a straight line tangent to the curve. This explains why a car skids outward on a fast turn or why a stone tied to a string shoots off when the string breaks: the inward force becomes insufficient, so the object reverts to straight‑line motion.
It matters a lot because centripetal force depends on the square of the speed. A small increase in speed produces a disproportionately large increase in the force required to maintain the curve. In a tight curve—where the radius is already small—the demand becomes even more extreme. That’s why vehicles must slow down before entering sharp turns: the combination of high speed and small radius multiplies the required inward force beyond what friction or traction can provide.

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