EduKG
← Back

pendulum periods and oscillation energy

Learning objectives

  • Outcome

    Compute the period of small oscillations of a simple pendulum with T=2πL/gT=2\pi\sqrt{L/g} for given LL and gg.

  • Outcome

    Justify the independence of the period from the bob mass and, at small angles, from the amplitude, stating the condition for sin⁡θ≈θ\sin\theta\approx\theta.

  • Outcome

    Calculate the total energy and the speed of a pendulum at a given point using E=12kA2E=\tfrac12 kA^2 and E=mgL(1−cos⁡θ0)E=mgL(1-\cos\theta_0).

Understand the idea

Pendulum Periods and Oscillation Energy

Text

A simple pendulum is a bob of mass mm on a massless string of length LL; at an angle θ\theta the restoring force is −mgsin⁡θ-mg\sin\theta.

For small angles sin⁡θ≈θ\sin\theta\approx\theta, so F≈−mgLxF\approx-\frac{mg}{L}x — a quasi-elastic force with stiffness k=mg/Lk=mg/L, and from the harmonic-oscillator dynamics T=2πm/kT=2\pi\sqrt{m/k} it follows that T=2πLg.T=2\pi\sqrt{\frac{L}{g}}.

The period contains neither the mass nor (at small angles) the amplitude: it is set only by the string length and the free-fall acceleration. The oscillation energy is described by the same model: E=12kA2=12mω2A2E=\tfrac12 kA^2=\tfrac12 m\omega^2 A^2, where the amplitude along the arc is A=Lθ0A=L\theta_0 and ω=2π/T\omega=2\pi/T. During the motion energy passes from potential to kinetic and back, while the total energy stays constant: E=mgL(1−cos⁡θ0)≈12mgLθ02E=mgL(1-\cos\theta_0)\approx\tfrac12 mgL\theta_0^2. The maximum speed occurs at the lowest point: vmax⁡=ωA=θ0gLv_{\max}=\omega A=\theta_0\sqrt{gL}; above roughly 15∘15^\circ the approximation sin⁡θ≈θ\sin\theta\approx\theta worsens and the period starts to grow with amplitude.

Worked examples

Direct

Problem

A simple pendulum has length L=1.00L=1.00 m. Find the period of its small oscillations for g=9.81g=9.81 m/s². Does the answer depend on the bob mass?

Solution

Substitute the values into the period formula:

T=2πLg=2π1.009.81=2π0.1019=2π⋅0.3193≈2.01 s.T=2\pi\sqrt{\frac{L}{g}}=2\pi\sqrt{\frac{1.00}{9.81}}=2\pi\sqrt{0.1019}=2\pi\cdot0.3193\approx2.01\ \text{s}.

The mass does not appear in the formula, so for m=0.05m=0.05 kg and for m=5m=5 kg the period stays the same: it depends only on LL and gg.

Application

Problem

A pendulum of length L=0.50L=0.50 m with a bob of mass m=0.20m=0.20 kg is released from θ0=8.0∘\theta_0=8.0^\circ (0.1400.140 rad). Find the arc amplitude, the maximum speed, and the total oscillation energy.

Solution
  1. Angular frequency: ω=g/L=9.81/0.50=4.43\omega=\sqrt{g/L}=\sqrt{9.81/0.50}=4.43 rad/s.
  2. Arc amplitude: A=Lθ0=0.50⋅0.140=0.070A=L\theta_0=0.50\cdot0.140=0.070 m.
  3. Maximum speed (at the lowest point): vmax⁡=ωA=4.43⋅0.070=0.31v_{\max}=\omega A=4.43\cdot0.070=0.31 m/s.
  4. Total energy:

E=12mvmax⁡2=12⋅0.20⋅0.312≈9.6⋅10−3 J.E=\tfrac12 m v_{\max}^2=\tfrac12\cdot0.20\cdot0.31^2\approx9.6\cdot10^{-3}\ \text{J}.

Check via potential energy: E=mgL(1−cos⁡θ0)=0.20⋅9.81⋅0.50⋅(1−cos⁡8∘)≈9.5⋅10−3E=mgL(1-\cos\theta_0)=0.20\cdot9.81\cdot0.50\cdot(1-\cos8^\circ)\approx9.5\cdot10^{-3} J — agreement within rounding error.

Transfer

Problem

A pendulum of length L=1.00L=1.00 m is released from θ0=6.0∘\theta_0=6.0^\circ.

(a) Using energy conservation, find the speed of the bob when the string makes an angle θ=3.0∘\theta=3.0^\circ with the vertical.

(b) By what factor does the period change if the same pendulum is taken to the Moon, where gM=1.62g_{\text{M}}=1.62 m/s²?

Solution

(a) The speed is largest at the lowest point, and ω=g/L=9.81/1.00=3.13\omega=\sqrt{g/L}=\sqrt{9.81/1.00}=3.13 rad/s.
Arc amplitude: A=Lθ0=1.00⋅0.1047=0.1047A=L\theta_0=1.00\cdot0.1047=0.1047 m; displacement at the required point: x=Lθ=1.00⋅0.0524=0.0524x=L\theta=1.00\cdot0.0524=0.0524 m.
From energy conservation 12mv2=12mω2(A2−x2)\tfrac12 m v^2=\tfrac12 m\omega^2(A^2-x^2), hence

v=ωA2−x2=3.130.10472−0.05242≈0.28 m/s.v=\omega\sqrt{A^2-x^2}=3.13\sqrt{0.1047^2-0.0524^2}\approx0.28\ \text{m/s}.

Check via heights: v2=2gL(cos⁡θ−cos⁡θ0)=2⋅9.81⋅(cos⁡3∘−cos⁡6∘)≈0.081v^2=2gL(\cos\theta-\cos\theta_0)=2\cdot9.81\cdot(\cos3^\circ-\cos6^\circ)\approx0.081 m²/s², so v≈0.28v\approx0.28 m/s.

(b) The period is proportional to 1/g1/\sqrt{g}, therefore

TMTE=ggM=9.811.62=6.06≈2.46.\frac{T_{\text{M}}}{T_{\text{E}}}=\sqrt{\frac{g}{g_{\text{M}}}}=\sqrt{\frac{9.81}{1.62}}=\sqrt{6.06}\approx2.46.

The period on the Moon is about 2.52.5 times longer: TM≈2.46⋅2.01≈4.94T_{\text{M}}\approx2.46\cdot2.01\approx4.94 s.

Practice

Text

Simulation (safe self-study plan): open the PhET Pendulum Lab or an equivalent simulation.

  1. Set L=1.00L=1.00 m, m=0.20m=0.20 kg, θ0=5∘\theta_0=5^\circ. Time 10 full oscillations and find TT.
  2. Repeat for L=0.25, 0.50, 1.00, 2.00L=0.25,\ 0.50,\ 1.00,\ 2.00 m. For each value compute L\sqrt{L} and plot TT versus L\sqrt{L} — you should get a straight line through the origin.
  3. At fixed length vary the mass (0.05, 0.20, 1.000.05,\ 0.20,\ 1.00 kg) and confirm that the period does not change.
  4. Vary θ0=5∘, 15∘, 45∘\theta_0=5^\circ,\ 15^\circ,\ 45^\circ and note at which angle the measured period noticeably exceeds 2πL/g2\pi\sqrt{L/g}.
  5. Turn on the energy display and describe how kinetic and potential energy exchange over one period: where EkE_k is maximal, where EpE_p is maximal, and what their sum equals.

Visual reference

Purpose

Show that the period of small oscillations is set only by the length (the graph of TT versus L\sqrt{L} is a straight line) and illustrate the exchange of kinetic and potential energy within one period.

Representation

Sketch and graphs.

  1. On the left, the pendulum in three positions: far left (θ0\theta_0, v=0v=0), bottom (00, v=vmax⁡v=v_{\max}), far right (−θ0-\theta_0, v=0v=0); arrows show the velocity and the restoring force mgsin⁡θmg\sin\theta.
  2. In the middle, energy bars for these three points: at the extremes all energy is potential (Ep=EE_p=E), at the bottom all is kinetic (Ek=EE_k=E); the sum of the bars stays constant.
  3. On the right, a graph of the period TT versus L\sqrt{L}: the data points fall on the straight line T=2πgLT=\frac{2\pi}{\sqrt{g}}\sqrt{L} with slope 2π/g2\pi/\sqrt{g}.

Real-world examples

Playground swing

Scenario

A child of mass 30 kg30\ \text{kg} sits on a swing with suspension length L=2.5 mL=2.5\ \text{m}. The child is pulled back so the arc length from the lowest point is 0.60 m0.60\ \text{m} and released. The deflection angle θ=s/L=0.60/2.5=0.24 rad\theta = s/L = 0.60/2.5 = 0.24\ \text{rad} is small, so the period is T=2πL/g=2π2.5/9.81=3.17 sT = 2\pi\sqrt{L/g} = 2\pi\sqrt{2.5/9.81} = 3.17\ \text{s}. Ten full oscillations take 31.7 s31.7\ \text{s}. The rise height is h=L(1−cos⁡θ)=2.5(1−cos⁡0.24)=0.0717 mh = L(1-\cos\theta) = 2.5(1-\cos 0.24) = 0.0717\ \text{m}, the maximum speed is vmax⁡=2gh=1.19 m/sv_{\max} = \sqrt{2gh} = 1.19\ \text{m/s}, and the maximum kinetic energy is Ek=12mvmax⁡2=21.1 JE_k = \frac12 m v_{\max}^2 = 21.1\ \text{J}; it equals the maximum potential energy Ep=mgh=21.1 JE_p = mgh = 21.1\ \text{J}.

Connection

This exercises the simple-pendulum period formula T=2πL/gT=2\pi\sqrt{L/g} and conservation of mechanical energy Ek+Ep=constE_k + E_p = \text{const}; the period is independent of mass and, for small angles, of amplitude.

Grandfather clock pendulum

Scenario

A grandfather clock pendulum is adjusted to a period T=2.00 sT=2.00\ \text{s}, so each half-oscillation lasts 1.00 s1.00\ \text{s}. From T=2πL/gT=2\pi\sqrt{L/g} the length is L=g(T/2π)2=9.81(2/(2π))2=0.994 mL = g(T/2\pi)^2 = 9.81(2/(2\pi))^2 = 0.994\ \text{m}. The bob mass is m=0.50 kgm=0.50\ \text{kg}, and the amplitude is θ0=2.0∘=0.0349 rad\theta_0 = 2.0^\circ = 0.0349\ \text{rad}. The rise height is h=L(1−cos⁡θ0)=0.994(1−cos⁡2∘)=6.06⋅10−4 mh = L(1-\cos\theta_0) = 0.994(1-\cos 2^\circ) = 6.06\cdot10^{-4}\ \text{m}, the maximum potential energy is Ep=mgh=2.97⋅10−3 J=2.97 mJE_p = mgh = 2.97\cdot10^{-3}\ \text{J} = 2.97\ \text{mJ}, the maximum speed is vmax⁡=2gh=0.109 m/sv_{\max} = \sqrt{2gh} = 0.109\ \text{m/s}, and the maximum kinetic energy is equal: Ek=12mvmax⁡2=2.97 mJE_k = \frac12 m v_{\max}^2 = 2.97\ \text{mJ}. Friction and air-drag losses each half-oscillation are replaced by the falling drive weight.

Connection

This applies T=2πL/gT=2\pi\sqrt{L/g} and h=L(1−cos⁡θ0)h = L(1-\cos\theta_0) together with the Ep↔EkE_p \leftrightarrow E_k conversion in a pendulum; the small angle 2∘2^\circ justifies the harmonic approximation.

Wrecking ball on a construction site

Scenario

A wrecking ball of mass m=1200 kgm=1200\ \text{kg} hangs on a cable of length L=15 mL=15\ \text{m} and is pulled aside by an angle θ0=10.0∘\theta_0 = 10.0^\circ. Its period is T=2πL/g=2π15/9.81=7.77 sT = 2\pi\sqrt{L/g} = 2\pi\sqrt{15/9.81} = 7.77\ \text{s}. The rise height is h=L(1−cos⁡10∘)=15(1−0.9848)=0.228 mh = L(1-\cos 10^\circ) = 15(1-0.9848) = 0.228\ \text{m}, and the maximum potential energy is Ep=mgh=1200⋅9.81⋅0.228=2.68⋅103 J=2.68 kJE_p = mgh = 1200\cdot9.81\cdot0.228 = 2.68\cdot10^3\ \text{J} = 2.68\ \text{kJ}. At the lowest point the speed is vmax⁡=2gh=2.12 m/sv_{\max} = \sqrt{2gh} = 2.12\ \text{m/s}, and the kinetic energy is Ek=12mvmax⁡2=2.68 kJE_k = \frac12 m v_{\max}^2 = 2.68\ \text{kJ}; this energy is transferred to the wall on impact.

Connection

The same period formula T=2πL/gT=2\pi\sqrt{L/g} and energy conservation are used; the period depends only on LL and gg, not on mm, while the impact energy is set by the height h=L(1−cos⁡θ0)h=L(1-\cos\theta_0).