Skip to content
Exercises · 13.16

Q.A simple pendulum of length ll and having a bob of mass MM is suspended in a car. The car is moving on a circular track of radius RR with a uniform speed vv. If the pendulum makes small oscillations in a radial direction about its equilibrium position, what will be its time period?

Arunachal CbseNCERTSubjective· 3mImportance★★★★★est
36% · 24/66 Questions
🔒 Locked · start free trial →

You're viewing a preview — the full solution, concept, methods & PYQ mapping are locked.

Start your 14-day free trial to unlock the full solution →

The pendulum’s effective gravity is the vector sum of actual gravity and the centrifugal acceleration from the car’s circular motion. The time period is T=2πlg2+(v2/R)2T = 2\pi \sqrt{\frac{l}{\sqrt{g^2 + (v^2/R)^2}}}.

The key insight here is that the pendulum is not in an inertial frame. The car is moving on a circular track, so from the car’s perspective (the non-inertial frame where the pendulum is observed), there is a centrifugal force acting on the bob. This force modifies the effective gravity that determines the pendulum’s restoring torque.

When the pendulum oscillates in the radial direction (i.e., along the line joining the car to the centre of the track), the centrifugal acceleration acts horizontally outward, perpendicular to the actual gravity. The bob therefore experiences a resultant acceleration that is the vector sum of gg downward and v2/Rv^2/R outward.

Let’s work through the steps.

  1. Identify the forces in the car’s frame.

    In the car’s frame, the bob feels:

    • Its weight MgMg downward.
    • A centrifugal force Mv2/RM v^2 / R outward (radially away from the track’s centre). There is no Coriolis force because the pendulum oscillates radially and the car’s rotation is uniform — but even if there were, for small oscillations the Coriolis effect is negligible in the radial direction.
  2. Find the effective gravity.

    The two accelerations are perpendicular: gg vertical, v2/Rv^2/R horizontal. The magnitude of the effective gravitational acceleration geffg_\text{eff} is:

geff=g2+(v2R)2.g_\text{eff} = \sqrt{g^2 + \left(\frac{v^2}{R}\right)^2}.

The direction of geffg_\text{eff} is at an angle θ0\theta_0 from the vertical, where tan⁡θ0=v2Rg\tan\theta_0 = \frac{v^2}{Rg}. This is the equilibrium position of the pendulum — it hangs tilted outward.

  1. Small oscillations about the new equilibrium.

    For small angular displacements from this tilted equilibrium, the restoring torque is provided by the component of geffg_\text{eff} perpendicular to the string. The situation is exactly like a simple pendulum in a uniform effective gravity geffg_\text{eff}. The length remains ll, and the mass cancels out.

  2. Write the time period. …

Unlock everything free for 14 days

  • Full step-by-step solutions
  • Concept-first explanations
  • Methods, shortcuts & mistakes
  • PYQ mapping + timed mock tests

Full access for 14 days. No credit card required.