The centre of mass (CM) of a rigid body is the unique point where the entire mass of the body can be considered concentrated for analysing its translational motion. NCERT Class 11 Physics Chapter 6, page 2 defines it as the mass-weighted average position of all constituent particles.
The formula. For a system of n particles:
R_cm = (Σ m_i r_i) / (Σ m_i)
For a continuous rigid body, the sum becomes an integral: R_cm = (1/M) ∫ r dm, where M is the total mass.
The trap that costs marks. A common confusion is defaulting to the geometric centre — assuming the CM is always at the midpoint of the body. This is true ONLY for uniform, symmetric bodies. When the mass distribution is non-uniform, or when a rigid body is composed of parts with different densities, the CM shifts toward the heavier region. For two particles of unequal mass on a rod, the CM sits closer to the heavier particle: its distance from mass m₁ is m₂L/(m₁ + m₂), not L/2.
Key ideas for NEET.
- For uniform symmetric rigid bodies (sphere, cube, cylinder, ring, disc), the CM is at the geometric centre — this follows from the integral by symmetry.
- For composite bodies (e.g. a disc with a hole), find the CM by treating the removed part as negative mass: R_cm = (m₁r₁ − m₂r₂)/(m₁ − m₂).
- The CM of a rigid body need not lie inside the body (e.g. a uniform ring — the CM is at the centre of the ring, where no material exists).
- External forces act as if applied at the CM for translational motion. Internal forces do not shift the CM.
Watch out: when a problem says "uniform rigid body," that guarantees the geometric centre IS the CM. If "uniform" is absent, check the mass distribution before assuming symmetry.