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NCERT Exemplar · Q22

Q.When will the motion of a simple pendulum be simple harmonic?

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A simple pendulum executes simple harmonic motion (SHM) only when its angular displacement is small (typically θ≲10∘\theta \lesssim 10^\circ or 0.170.17 rad), because only then does the restoring torque become directly proportional to the displacement. The period is then T=2πL/gT = 2\pi\sqrt{L/g}.

Why the pendulum is not always simple harmonic

A simple pendulum consists of a point mass mm attached to a massless, inextensible string of length LL, swinging under gravity. The restoring force that pulls the bob back toward the equilibrium position comes from the tangential component of gravity.

When the bob is displaced by an angle θ\theta from the vertical, the gravitational force mgmg splits into two components:

  • Radial: mgcos⁡θmg\cos\theta (tension balances this)
  • Tangential: mgsin⁡θmg\sin\theta (this is the restoring force)

The tangential force is F=−mgsin⁡θF = -mg\sin\theta, where the minus sign indicates it always points opposite to the displacement. For the motion to be simple harmonic, the restoring force must be directly proportional to the displacement — that is, F∝−θF \propto -\theta (or F∝−xF \propto -x for linear displacement).

Here lies the catch: sin⁡θ\sin\theta is not proportional to θ\theta for large angles.

Watch out

Many students mistakenly write F=−mgθF = -mg\theta directly. This is only valid when θ\theta is small enough that sin⁡θ≈θ\sin\theta \approx \theta (in radians). For θ=30∘\theta = 30^\circ (0.520.52 rad), sin⁡θ=0.5\sin\theta = 0.5 while θ=0.52\theta = 0.52 — a 4% error that grows rapidly with larger angles.

The small-angle approximation

For small angles measured in radians, the Taylor expansion of sin⁡θ\sin\theta gives:

sin⁡θ=θ−θ33!+θ55!−⋯\sin\theta = \theta - \frac{\theta^3}{3!} + \frac{\theta^5}{5!} - \cdots

When θ≪1\theta \ll 1 radian, the higher-order terms become negligible, and we can write:

sin⁡θ≈θ\sin\theta \approx \theta

This approximation is excellent for θ<0.17\theta < 0.17 rad (about 10∘10^\circ), where the error is less than 0.5%.

F≈−mgθfor small θF \approx -mg\theta \quad \text{for small } \theta

Since the arc length s=Lθs = L\theta, the linear displacement x≈s=Lθx \approx s = L\theta (for small angles, the arc is nearly straight), so θ=x/L\theta = x/L. Substituting:

F≈−mg(xL)=−(mgL)xF \approx -mg\left(\frac{x}{L}\right) = -\left(\frac{mg}{L}\right)x

This is exactly Hooke's law: F=−kxF = -kx with effective spring constant k=mg/Lk = mg/L. The motion is therefore simple harmonic.

Deriving the period

Using Newton's second law for rotational motion, the torque about the pivot is:

τ=−mgLsin⁡θ\tau = -mgL\sin\theta

For small θ\theta, τ≈−mgLθ\tau \approx -mgL\theta. Since τ=Iα\tau = I\alpha and the moment of inertia of a point mass at distance LL is I=mL2I = mL^2:

mL2d2θdt2=−mgLθmL^2\frac{d^2\theta}{dt^2} = -mgL\theta

d2θdt2=−gLθ\frac{d^2\theta}{dt^2} = -\frac{g}{L}\theta

This is the SHM equation d2θdt2=−ω2θ\frac{d^2\theta}{dt^2} = -\omega^2\theta, where ω=g/L\omega = \sqrt{g/L}.

Tip

You don't need to re-derive this every time. The angular frequency ω=g/L\omega = \sqrt{g/L} is the key result — memorize it, and the period follows directly. …

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