Physics·Core Principles

Motion of Centre of Mass — Core Principles

NEET UG
Version 1Updated 22 Mar 2026

Core Principles

The center of mass (CM) is a hypothetical point representing the average position of all the mass in a system. Its motion is fundamental to understanding the overall translational dynamics of a collection of particles or an extended body.

The key principle is that the velocity and acceleration of the center of mass are determined solely by the net external force acting on the system. Internal forces, which are forces between particles within the system, always cancel out in pairs and thus do not affect the motion of the CM.

The velocity of the CM is given by VCM=1Mmivi\vec{V}_{CM} = \frac{1}{M} \sum m_i \vec{v}_i, where MM is the total mass and vi\vec{v}_i are individual particle velocities. Similarly, its acceleration is ACM=1Mmiai\vec{A}_{CM} = \frac{1}{M} \sum m_i \vec{a}_i.

Newton's second law for a system of particles states Fext=MACM\vec{F}_{ext} = M \vec{A}_{CM}. If Fext=0\vec{F}_{ext} = 0, then VCM\vec{V}_{CM} is constant, implying conservation of the system's total linear momentum.

This concept simplifies problems involving explosions, collisions, and relative motion within a system.

Important Differences

vs Motion of Individual Particles

AspectThis TopicMotion of Individual Particles
Governing ForcesMotion of Centre of MassMotion of Individual Particles
Complexity of DescriptionMotion of Centre of MassMotion of Individual Particles
Conservation LawsMotion of Centre of MassMotion of Individual Particles
Physical RealityMotion of Centre of MassMotion of Individual Particles
The motion of the center of mass provides a simplified, holistic view of a system's translational dynamics, being influenced only by external forces. It acts as a representative point for the entire system's mass. In contrast, the motion of individual particles is often far more intricate, affected by both internal interactions with other particles within the system and external forces. While the CM's motion can be smooth and predictable (e.g., parabolic under gravity), individual particles might follow highly erratic paths, especially during events like explosions or collisions. This distinction is crucial for applying conservation laws effectively.
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