Physic Labs

Oscillations and waves

The simple pendulum

Measure gravitational acceleration with a simple pendulum at small angles: track the period T against length l and verify T≈2πl/gT \approx 2\pi\sqrt{l/g}, hence g=4π2l/T2g = 4\pi^2 l/T^2.

High school

Equipment

  • Virtual simple pendulum with a small bob and light inextensible string
  • Length slider l (20–200 cm)
  • Sliders for initial angle and g value
  • T²-versus-l plot and a period readout

Procedure

  1. Measure the period at different lengths

    Keep the initial angle small, drag l through 4–5 values, and read T at each point. Plotting T2T^2 versus l gives a straight line of slope 4π2/g4\pi^2/g, matching T≈2πl/gT \approx 2\pi\sqrt{l/g}.

  2. Test the small-angle condition

    Hold l fixed and increase the initial angle from ~5° upward: the period grows slightly beyond the 2πl/g2\pi\sqrt{l/g} prediction, since sin⁡θ≈θ\sin\theta \approx \theta holds only at small angles. Record the deviation to see the approximation's limit.

  3. Infer and change g

    From a measured (l, T) pair, compute g=4π2l/T2g = 4\pi^2 l/T^2 and compare with the g slider value. Then change g (e.g., another planet): the period must scale as T∝1/gT \propto 1/\sqrt{g} — halving g raises T by 2\sqrt{2}; predict before checking.

Simulation

Experiment history

Galileo Galilei noticed a chandelier swinging in Pisa Cathedral had a period nearly independent of amplitude — the isochronism of the pendulum (c. 1581–1602). He also noted the period depends only on string length; in the Discorsi (1638) he wrote that period scales as the square root of length. In 1656 Christiaan Huygens built the first practical pendulum clock and, in Horologium Oscillatorium (1673), gave the formula T=2πl/gT = 2\pi\sqrt{l/g} geometrically. Pendulum methods then offered the most accurate g measurements for two centuries — Kater's reversible pendulum (1818) reached six significant figures.

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