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Mechanics

Pendulum Period Calculator

Calculate pendulum period (T = 2\u03C0\u221A(L/g)), frequency, length, gravity, oscillation timing, or compare periods on different planets.

Interactive calculator

Pendulum Period Calculator

Calculate pendulum period, frequency, length, gravity, oscillation timing, or compare periods on different planets.

Try an example

Pendulum length (pivot to centre of mass)

Your result will appear here.

Choose a calculation mode, fill in the known values, and click Calculate.

Quick Guide

  • Choose: period, frequency, length, gravity, counter, or planet comparison.
  • Enter pendulum length and/or gravity.
  • Click Calculate for period and related values.

Key Takeaways

  • T = 2π√(L/g) — period depends only on length and gravity.
  • Period is independent of mass and amplitude (for small angles).
  • A 1 m pendulum on Earth has T ≈ 2.006 s.
  • The ‘seconds pendulum’ (T = 2 s) is 0.994 m long.
  • Period increases with length and decreases with gravity.
  • Pendulums can measure local gravity with high precision.

What Is a Simple Pendulum?

A simple pendulum is a mass (bob) suspended from a pivot by a massless, inextensible string. When displaced from its equilibrium position, it swings back and forth under gravity. For small angles, the motion is approximately simple harmonic.

T = 2π√(L/g)

T=2πL/gT = 2\pi\sqrt{L / g}

The period T depends only on the string length L and gravitational acceleration g. Remarkably, it does not depend on the bob’s mass or the amplitude (for small oscillations).

Pendulum Diagram

θLm

A simple pendulum: mass m hangs from a fixed pivot by a string of length L. The angle θ measures the displacement from vertical.

Pendulum on Other Planets

Bodyg (m/s²)1 m pendulum T
Earth9.812.01 s
Moon1.624.93 s
Mars3.713.27 s
Jupiter24.791.26 s
Pluto0.627.99 s

How to Use the Calculator

  1. Select the calculation mode.
  2. Enter length, period, gravity, or oscillation count.
  3. Click Calculate.
  4. Review period, frequency, and related values.

Example Calculations

1 m pendulum on Earth

T = 2π√(1/9.81) = 2.006 s

Seconds pendulum (T = 2 s)

L = 9.81 × 4 / (4π²) = 0.994 m

1 m on Moon (g = 1.62)

T = 2π√(1/1.62) = 4.93 s (2.46× Earth)

Common Mistakes

  • Using the formula for large angles (> 15°) without correction.
  • Measuring to the bottom of the bob instead of its centre of mass.
  • Thinking mass or amplitude changes the period.
  • Confusing period (time for full swing) with half-period (time to one side).

Accuracy and Limitations

T = 2π√(L/g) is the small-angle approximation. For angles above 15°, correction terms are needed: T ≈ T₀(1 + θ²/16 + ...). The formula also assumes a point mass, rigid support, massless string, and no air drag.

FAQ

Does mass affect pendulum period?

No. For a simple pendulum with small oscillations, the period depends only on length and gravity, not mass. This was first noted by Galileo.

Does amplitude affect the period?

For small angles (< ~15°), the period is nearly constant. For large angles, the period increases slightly. This is the ‘small-angle approximation’.

What is a seconds pendulum?

A pendulum with a 2-second period (1 second each way). On Earth, its length is approximately 0.994 m (~1 metre).

How does a pendulum measure gravity?

Measure the pendulum’s length and period, then compute g = 4π²L/T². This method was historically used to measure g before modern accelerometers.

Would a pendulum work in space?

No. A pendulum requires gravity to provide the restoring force. In microgravity (ISS), a pendulum would not swing.

Why is the period longer on the Moon?

The Moon’s gravity (1.62 m/s²) is weaker than Earth’s (9.81 m/s²). Since T ∝ 1/√g, weaker gravity means longer periods.

What about a physical (compound) pendulum?

For a real pendulum with distributed mass, the formula uses the moment of inertia: T = 2π√(I/(mgh)). The simple pendulum formula is a special case.

Sources

Manish Kumar

Author & technical reviewer

Manish Kumar

PhysicsCalcs tools are reviewed with an educational focus: clear formulas, transparent assumptions, and practical context for students and science learners.

Learn more about Manish