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Physics · Ch 6 — System of Particles and Rotational Motion

Centre of Mass

6.2

Centre of Mass

6.2 Centre of Mass

The Core Idea

When we study the motion of a system of particles — whether it's two atoms or a spinning cricket bat — we quickly realise that tracking every single particle is impractical. The centre of mass is the single point that behaves as if the entire mass of the system were concentrated there, and as if all external forces acted at that point. For a rigid body undergoing pure translation, every particle moves exactly as the centre of mass moves. For more complex motion that includes rotation, the centre of mass still follows a simple translational path, while the body rotates about it.


Two-Particle System Along a Line

Consider two particles of masses m1m_1 and m2m_2 lying on the xx-axis. Let their positions be x1x_1 and x2x_2 measured from some origin O. The centre of mass of this two-particle system is the point C whose coordinate XX is given by

X=m1x1+m2x2m1+m2X = \frac{m_1 x_1 + m_2 x_2}{m_1 + m_2}

This is a mass-weighted average of the positions. If the two masses are equal (m1=m2=mm_1 = m_2 = m), then

X=mx1+mx22m=x1+x22X = \frac{m x_1 + m x_2}{2m} = \frac{x_1 + x_2}{2}

so the centre of mass lies exactly midway between the two particles.

Note

The centre of mass is not necessarily the geometric centre — it is pulled toward the heavier particle. Only when masses are equal does it coincide with the midpoint.


Generalisation to nn Particles on a Line

For nn particles of masses m1,m2,…,mnm_1, m_2, \dots, m_n placed along the xx-axis at positions x1,x2,…,xnx_1, x_2, \dots, x_n, the centre of mass coordinate XX is

X=m1x1+m2x2+⋯+mnxnm1+m2+⋯+mn=∑i=1nmixi∑i=1nmiX = \frac{m_1 x_1 + m_2 x_2 + \dots + m_n x_n}{m_1 + m_2 + \dots + m_n} = \frac{\sum_{i=1}^n m_i x_i}{\sum_{i=1}^n m_i}

The denominator is the total mass M=∑miM = \sum m_i. Using summation notation,

X=∑mixiMX = \frac{\sum m_i x_i}{M}


Centre of Mass in a Plane

For three particles not lying on a straight line, we set up xx and yy axes in their plane. Let the particles have masses m1,m2,m3m_1, m_2, m_3 and coordinates (x1,y1),(x2,y2),(x3,y3)(x_1, y_1), (x_2, y_2), (x_3, y_3). The centre of mass is at (X,Y)(X, Y) where

X=m1x1+m2x2+m3x3m1+m2+m3X = \frac{m_1 x_1 + m_2 x_2 + m_3 x_3}{m_1 + m_2 + m_3}

Y=m1y1+m2y2+m3y3m1+m2+m3Y = \frac{m_1 y_1 + m_2 y_2 + m_3 y_3}{m_1 + m_2 + m_3}

If all three masses are equal (m1=m2=m3=mm_1 = m_2 = m_3 = m), then

X=m(x1+x2+x3)3m=x1+x2+x33X = \frac{m(x_1 + x_2 + x_3)}{3m} = \frac{x_1 + x_2 + x_3}{3}

Y=m(y1+y2+y3)3m=y1+y2+y33Y = \frac{m(y_1 + y_2 + y_3)}{3m} = \frac{y_1 + y_2 + y_3}{3}

These are precisely the coordinates of the centroid of the triangle formed by the three particles. For equal masses, the centre of mass coincides with the centroid.


Centre of Mass in Space: The Vector Form

For nn particles distributed in three-dimensional space, with the iith particle of mass mim_i at (xi,yi,zi)(x_i, y_i, z_i), the centre of mass coordinates are

X=∑mixiM,Y=∑miyiM,Z=∑miziMX = \frac{\sum m_i x_i}{M}, \quad Y = \frac{\sum m_i y_i}{M}, \quad Z = \frac{\sum m_i z_i}{M}

where M=∑miM = \sum m_i is the total mass.

These three scalar equations combine elegantly into a single vector equation. Let ri=xii^+yij^+zik^\mathbf{r}_i = x_i \hat{\mathbf{i}} + y_i \hat{\mathbf{j}} + z_i \hat{\mathbf{k}} be the position vector of the iith particle, and let R=Xi^+Yj^+Zk^\mathbf{R} = X \hat{\mathbf{i}} + Y \hat{\mathbf{j}} + Z \hat{\mathbf{k}} be the position vector of the centre of mass. Then

R=∑miriM\mathbf{R} = \frac{\sum m_i \mathbf{r}_i}{M}

R=1M∑i=1nmiri\mathbf{R} = \frac{1}{M} \sum_{i=1}^n m_i \mathbf{r}_i

If we choose the centre of mass itself as the origin of our coordinate system, then R=0\mathbf{R} = \mathbf{0}, which gives

∑miri=0\sum m_i \mathbf{r}_i = 0

This condition is often useful in derivations.


Continuous Mass Distribution

A rigid body is a system of closely packed particles — so many that summing over individual atoms is impossible. Instead, we treat the body as a continuous distribution of mass.

We divide the body into nn small elements of mass Δm1,Δm2,…,Δmn\Delta m_1, \Delta m_2, \dots, \Delta m_n, each located approximately at (xi,yi,zi)(x_i, y_i, z_i). The centre of mass coordinates are approximately

X≈∑(Δmi)xi∑Δmi,Y≈∑(Δmi)yi∑Δmi,Z≈∑(Δmi)zi∑ΔmiX \approx \frac{\sum (\Delta m_i) x_i}{\sum \Delta m_i}, \quad Y \approx \frac{\sum (\Delta m_i) y_i}{\sum \Delta m_i}, \quad Z \approx \frac{\sum (\Delta m_i) z_i}{\sum \Delta m_i}

As we take nn larger and each Δmi\Delta m_i smaller, these approximations become exact. The sums become integrals:

∑Δmi→∫dm=M\sum \Delta m_i \to \int dm = M

∑(Δmi)xi→∫x dm\sum (\Delta m_i) x_i \to \int x \, dm

and similarly for yy and zz. The exact centre of mass coordinates are therefore

X=1M∫x dm,Y=1M∫y dm,Z=1M∫z dmX = \frac{1}{M} \int x \, dm, \quad Y = \frac{1}{M} \int y \, dm, \quad Z = \frac{1}{M} \int z \, dm

The vector form is

R=1M∫r dm\mathbf{R} = \frac{1}{M} \int \mathbf{r} \, dm

If the centre of mass is taken as the origin, then R=0\mathbf{R} = \mathbf{0}, which implies

∫r dm=0\int \mathbf{r} \, dm = 0

or equivalently

∫x dm=∫y dm=∫z dm=0\int x \, dm = \int y \, dm = \int z \, dm = 0


Symmetry and the Centre of Mass of Homogeneous Bodies

For homogeneous bodies (uniform mass distribution) of regular shape — rings, discs, spheres, rods — the centre of mass lies at the geometric centre. This follows from reflection symmetry. …

Figure 6.7Locating the centre of mass C of a two-particle system on the x-axis.
Fig. 6.7 — Locating the centre of mass C of a two-particle system on the x-axis.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your NCERT textbook's own diagram.

The figure shows a straight horizontal line — the x-axis — with two points labelled m1m_1 and m2m_2 placed at positions x1x_1 and x2x_2 respectively. A third point, labelled C (the centre of mass), lies somewhere between them at coordinate XX. A dashed vertical line drops from C down to the axis, marking its location clearly. The origin O is at the left end of the axis, and a vertical y-axis is drawn through O, though the figure is essentially one-dimensional.

The physical idea is simple: if you have two masses on a line, there is a single point — the centre of mass — that behaves as if the entire mass of the system were concentrated there. For two particles, this point always lies on the line joining them, closer to the heavier mass. The figure makes this concrete by placing m1m_1 and m2m_2 at known coordinates and showing C at the weighted average of their positions.

The textbook uses this diagram to derive the formula for the centre of mass of a two-particle system. The key step is to require that the total torque about the centre of mass is zero — or equivalently, that the centre of mass is the point where the weighted sum of distances from any reference point equals the total mass times the distance to that reference point. From the figure, with the origin at O, the definition gives:

X=m1x1+m2x2m1+m2X = \frac{m_1 x_1 + m_2 x_2}{m_1 + m_2}

Here m1m_1 and m2m_2 are the masses of the two particles, x1x_1 and x2x_2 are their positions on the x-axis, and XX is the x-coordinate of the centre of mass C. The denominator m1+m2m_1 + m_2 is the total mass MM of the system.

Important

The centre of mass is the mass-weighted average position of the particles. For two particles on a line, it always lies between them — exactly at the midpoint only if the masses are equal, and closer to the heavier mass otherwise.

If you choose the origin at the centre of mass itself (so X=0X = 0), the formula rearranges to m1x1+m2x2=0m_1 x_1 + m_2 x_2 = 0, which says that the two particles balance each other about that point — a direct visual takeaway from the figure: the dashed line at C is the balance point. …

Figure 6.8Determining the CM of a thin rod.
Fig. 6.8 — Determining the CM of a thin rod.

Drawn by us to help you understand the concept clearly, and verified to make sure it's accurate. For exams, practice from your NCERT textbook's own diagram.

The figure shows a thin rod placed along the x-axis with its centre at the origin O. The rod itself is drawn as a dashed line, indicating it is a continuous object, not a collection of discrete particles. Two small mass elements, each labelled dmdm, are marked at symmetric positions: one at +x+x and one at −x-x. The entire rod extends from x=−L/2x = -L/2 to x=+L/2x = +L/2, so its total length is LL.

The physical idea is straightforward: to find the centre of mass of a continuous object, you cannot sum over individual particles because there are infinitely many. Instead, you imagine cutting the rod into infinitesimally small pieces of mass dmdm, each located at some coordinate xx. The centre of mass is then the weighted average of all these positions, where the weight is the mass of each piece. The symmetry of the figure — two equal mass elements at opposite positions — hints that the centre of mass must lie at the origin. But the textbook uses this setup to derive the general formula.

The key formula developed from this figure is the centre of mass of a continuous body:

xCM=1M∫x dmx_{\text{CM}} = \frac{1}{M} \int x \, dm

Here, MM is the total mass of the rod, xx is the position coordinate of a mass element dmdm, and the integral runs over the entire length of the rod. For the thin rod, the mass per unit length λ=M/L\lambda = M/L is constant, so dm=λ dx=(M/L) dxdm = \lambda \, dx = (M/L) \, dx. Substituting this into the integral gives:

xCM=1M∫−L/2+L/2x⋅ML dx=1L∫−L/2+L/2x dxx_{\text{CM}} = \frac{1}{M} \int_{-L/2}^{+L/2} x \cdot \frac{M}{L} \, dx = \frac{1}{L} \int_{-L/2}^{+L/2} x \, dx

The integral of xx over symmetric limits is zero because the positive and negative contributions cancel exactly. Hence xCM=0x_{\text{CM}} = 0, confirming that the centre of mass of a uniform rod is at its geometric centre. …