Atwood Machine


Introduction

The Atwood machine is one of the most elegant and instructive devices in classical mechanics. Invented by English mathematician George Atwood in 1784, it consists of two masses connected by a light, inextensible string draped over a frictionless pulley. When the two masses are unequal, the heavier side accelerates downward while the lighter side rises, and the system provides a clear, measurable demonstration of Newton's second law. Because the acceleration produced is much smaller than free fall, Atwood originally used the machine to slow down gravitational motion enough to study it with the limited timing instruments of his era. Today it remains a cornerstone of introductory physics education.


The Physics Explained

To understand the Atwood machine, start by identifying the forces acting on each mass. Gravity pulls each mass downward with a force equal to its weight — mass multiplied by the gravitational acceleration g. The string pulls each mass upward with a tension force T. Because the string is assumed to be inextensible and the pulley massless and frictionless, the tension is the same throughout the string and both masses have the same magnitude of acceleration, just in opposite directions.

Applying Newton's second law separately to each mass gives two equations. For the heavier mass m1, the net downward force is its weight minus the tension: m1 times g minus T equals m1 times a. For the lighter mass m2, the net upward force is the tension minus its weight: T minus m2 times g equals m2 times a. Adding these two equations eliminates T and yields an expression for the acceleration a of the system. The acceleration depends only on the difference between the two masses divided by their sum, multiplied by g.

This result is physically intuitive. If the two masses are equal, the difference is zero and the acceleration is zero — the system stays put. As the mass difference grows, the acceleration approaches g, which would be free fall. The tension in the string can be found by substituting the acceleration back into either of the original equations. Notably, the tension is always less than the weight of the heavier mass and always greater than the weight of the lighter mass — the string supports each mass partially against gravity without fully cancelling it out.

In a real Atwood machine, the pulley has rotational inertia and the string has mass, both of which reduce the actual acceleration slightly compared to the ideal prediction. Friction at the pulley axle also plays a role. The ideal model is nevertheless an excellent approximation when a low-mass pulley and lightweight string are used, and it captures all the essential physics cleanly.


Key Equations

Newton's second law for m1 (heavier, moving down)m1 * g - T = m1 * a
Newton's second law for m2 (lighter, moving up)T - m2 * g = m2 * a
Acceleration of the systema = (m1 - m2) * g / (m1 + m2)
Tension in the stringT = 2 * m1 * m2 * g / (m1 + m2)
Velocity after time t (starting from rest)v = a * t
Displacement after time t (starting from rest)d = 0.5 * a * t^2

Key Variables

Symbol Unit Description
m1kgMass of the heavier object on one side of the string
m2kgMass of the lighter object on the other side of the string
gm/s^2Gravitational acceleration, approximately 9.81 m/s^2 near Earth's surface
am/s^2Acceleration of the system; both masses accelerate at this magnitude
TNTension in the string; equal throughout under ideal conditions
vm/sSpeed of either mass at a given instant in time
tsTime elapsed since the system was released from rest
dmDistance travelled by either mass from its starting position
FNNet force acting on the system, equal to (m1 - m2) * g

Real World Examples


How the Simulation Works

The simulation presents two hanging masses connected by a string over a central pulley. Two sliders allow you to set the value of mass 1 and mass 2 independently. When you press the Launch button, the simulation applies the Atwood machine equations at every time step: it computes the net force on the system as the difference in weights, divides by the total mass to find the acceleration, and then updates the velocity and position of each mass accordingly using standard kinematic integration.

The heavier mass descends while the lighter mass rises at the same rate. Readouts beside each mass display the current velocity, and a central panel shows the computed acceleration and string tension in real time. If the masses are set equal, the system remains stationary, confirming that zero net force means zero acceleration. You can reset the simulation at any time, adjust the masses, and relaunch to explore how the ratio of the two masses affects how quickly or slowly the system accelerates. This makes it easy to build intuition for Newton's second law in a controlled, visible way.


Further Reading