Academy
Formulas/physics/Centre Of Mass/Centre of Mass — Continuous Body

Centre of Mass — Continuous Body

Position of centre of mass of a continuous mass distribution.
Class 11Class JEE
Derivation

From discrete to continuous

For a discrete system: rcm=miriM\vec{r}_{cm} = \frac{\sum m_i \vec{r}_i}{M}

For a continuous body, the sum becomes an integral. Instead of point masses mim_i, we have infinitesimal mass elements dmdm at position r\vec{r}:

rcm=rdmM=rdmdm\vec{r}_{cm} = \frac{\int \vec{r} \, dm}{M} = \frac{\int \vec{r} \, dm}{\int dm}

In components:

xcm=xdmM,ycm=ydmM,zcm=zdmMx_{cm} = \frac{\int x \, dm}{M}, \quad y_{cm} = \frac{\int y \, dm}{M}, \quad z_{cm} = \frac{\int z \, dm}{M}

How to express dmdm

The key step is expressing dmdm in terms of a coordinate variable and the density.

Linear mass density λ\lambda (mass per unit length, for rods, wires, arcs):

dm=λdldm = \lambda \, dl

Surface mass density σ\sigma (mass per unit area, for laminas, shells):

dm=σdAdm = \sigma \, dA

Volume mass density ρ\rho (mass per unit volume, for solid bodies):

dm=ρdVdm = \rho \, dV

For uniform bodies, λ\lambda, σ\sigma, or ρ\rho are constant and can be taken outside the integral.

General method

  1. Choose a coordinate system with origin at a convenient point (often a symmetry point)
  2. Choose an appropriate mass element dmdm (strip, shell, disc, etc.)
  3. Express dmdm in terms of the coordinate variable
  4. Set up and evaluate the integral
  5. Divide by total mass MM

Example: Uniform rod of length LL

Take the left end as origin. Linear mass density λ=M/L\lambda = M/L (uniform).

dm=λdx=MLdxdm = \lambda \, dx = \frac{M}{L} dx

xcm=1M0LxMLdx=1L0Lxdx=1LL22=L2x_{cm} = \frac{1}{M}\int_0^L x \cdot \frac{M}{L} dx = \frac{1}{L}\int_0^L x \, dx = \frac{1}{L} \cdot \frac{L^2}{2} = \frac{L}{2}

CM is at the midpoint — expected by symmetry.

Example: Uniform triangular lamina

For a triangle with base bb and height hh, base along the xx-axis:

At height yy, the width of the strip is b(1yh)b\left(1 - \frac{y}{h}\right) (by similar triangles).

dm=σb(1yh)dydm = \sigma \cdot b\left(1 - \frac{y}{h}\right) dy

ycm=0hyσb(1yh)dyσ12bhy_{cm} = \frac{\int_0^h y \cdot \sigma b\left(1-\frac{y}{h}\right) dy}{\sigma \cdot \frac{1}{2}bh}

Numerator: σb0h(yy2h)dy=σb[h22h23]=σbh26\sigma b \int_0^h \left(y - \frac{y^2}{h}\right) dy = \sigma b \left[\frac{h^2}{2} - \frac{h^2}{3}\right] = \frac{\sigma b h^2}{6}

ycm=σbh2/6σbh/2=h3y_{cm} = \frac{\sigma b h^2/6}{\sigma b h/2} = \frac{h}{3}

CM is at h/3h/3 from the base — consistent with the triangle result.

Symmetry shortcut

For bodies with a line or plane of symmetry, the CM lies on that symmetry element. This can eliminate one or more integrals entirely.

A semicircular disc has a line of symmetry along the yy-axis → xcm=0x_{cm} = 0. Only ycmy_{cm} needs to be computed.

Remember
Always exploit symmetry before integrating. For uniform bodies with bilateral symmetry, the CM lies on the symmetry axis. The integral is only needed for the non-symmetric direction.