Conceptly
LessonsFormulasPricing
Sign inStart free
Conceptly
TermsPrivacyRefunds
© 2026 · Physics for everyone
  1. Home
  2. Lessons
  3. Mechanics
  4. Centre of Mass and Equilibrium
All lessons Mechanics24 min

Centre of Mass and Equilibrium

Complete each stage to unlock the next one.

← Collisions and Conservation of MomentumCircular Motion →
01
Hook
02
Explore
03
Formalize
04
Practice
05
Challenge
Interactive simulation
01

Hook

A tightrope walker 30 m up reaches not for a net but for a long, drooping pole. The pole adds weight high above the wire — so why does it make balancing easier, not harder?

02

Explore

Complete previous stage
03

Formalize

Complete previous stage
04

Practice

Complete previous stage
05

Challenge

Complete previous stage
Spoilers

Centre of Mass and Equilibrium — summary and key formula

ShowHide

The question

A tightrope walker 30 m up reaches not for a net but for a long, drooping pole. The pole adds weight high above the wire — so why does it make balancing easier, not harder?

Every object acts as if all its mass sits at one point: the centre of mass. The pole's sagging ends pull the combined CoM down, often below the wire, and a low CoM is far harder to tip. The same idea explains low-slung race cars and crane counterweights.

The key idea

The centre of mass is the mass-weighted average position of every part of a system — the single point where the net external force acts, and the point a free object spins about. An object stays in stable equilibrium while its CoM lies above (or within) its base of support.

Why the formula is inevitable: to balance a beam, the moments (mass × distance from pivot) on each side must cancel. Solving 'sum of moments = 0' for the pivot gives exactly x = Σ(mᵢxᵢ)/Σmᵢ — the CoM is the point you'd support to stop rotation. Stability: an object stays upright while its CoM sits over its base. Tilt it until the CoM passes the edge and gravity's torque flips from righting it to toppling it. This single idea explains the tightrope walker's drooping pole (lowers the CoM), low-slung race cars (CoM stays inside the wheelbase), crane counterweights, and walking — controlled falling, where each step catches a CoM that has briefly left your base. **All forms:** xcom=(m1x1+m2x2)/(m1+m2)x_{com} = (m_1x_1 + m_2x_2)/(m_1+m_2)xcom​=(m1​x1​+m2​x2​)/(m1​+m2​) rearranges to the balance form m1d1=m2d2m_1d_1 = m_2d_2m1​d1​=m2​d2​ — equal mass-moments either side. **Limiting case:** let m2≫m1m_2 \gg m_1m2​≫m1​ and the centre of mass sits essentially at the heavy body — the Earth–Moon balance point is inside the Earth. **Connect it:** external forces act as if all mass lived at the COM: hurl a spinning hammer and its tumbling is chaos, but its centre of mass draws a perfect parabola.

The formula

xCOM=∑mixi∑mix_{\text{COM}} = \frac{\sum m_i x_i}{\sum m_i}xCOM​=∑mi​∑mi​xi​​
  • ·x_COM = position of the centre of mass (m)
  • ·mᵢ = mass of each part (kg)
  • ·xᵢ = its position along the axis (m)
  • ·Σmᵢ = total mass (kg). Each position is weighted by its mass
  • ·so heavier parts pull the CoM toward themselves. For equal masses this is just the plain average of the positions.

Common mistake

Placing the centre of mass at the geometric middle — it's the mass-WEIGHTED average, so it sits closer to the heavier object.

What to remember

  • ·Centre of mass = Σ(mx) ÷ Σm, the mass-weighted average position.
  • ·It lies nearer the heavier mass, not the geometric centre.
  • ·With no external force, the centre of mass keeps a constant velocity.