Equilibrium of Rigid Bodies

Physics
NEET UG
Version 1Updated 24 Mar 2026

Equilibrium of rigid bodies refers to the state where a rigid body experiences no net change in its translational or rotational motion. This implies that the net external force acting on the body is zero, ensuring no linear acceleration, and the net external torque acting on the body about any point is also zero, ensuring no angular acceleration. Consequently, a rigid body in equilibrium will eith…

Quick Summary

Equilibrium of rigid bodies is a fundamental concept in mechanics, essential for understanding how objects remain stable or move without acceleration. A rigid body is an idealized object that maintains its shape.

For such a body to be in complete equilibrium, two crucial conditions must be met. Firstly, the net external force acting on the body must be zero (SigmaF=0Sigma \vec{F} = 0). This ensures that the body's center of mass has no linear acceleration, meaning it either remains stationary or moves with a constant linear velocity.

Secondly, the net external torque acting on the body about any point must also be zero (Sigmaτ=0Sigma \vec{\tau} = 0). This condition guarantees that the body has no angular acceleration, meaning it either remains non-rotating or rotates with a constant angular velocity.

Problems typically involve identifying all forces (including weight at the center of gravity, normal forces, friction, tension) and their points of application, drawing a free-body diagram, and then applying these two conditions to form a system of equations to solve for unknown forces or distances.

Choosing a strategic pivot point for torque calculations is key to simplifying the problem.

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Key Concepts

Conditions for Equilibrium

For a rigid body to be in complete equilibrium, it must satisfy two conditions simultaneously. First, the…

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Types of Equilibrium (Stability)

Beyond the conditions for static or dynamic equilibrium, we can classify equilibrium based on its stability:…

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