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Science

Pendulum Period Calculator (T = 2π√L/g)

A simple pendulum is the textbook idealisation of a small bob hanging from a massless string, swinging under gravity. Under the small-angle approximation (< 15°) the period T depends only on the pendulum length L and the local gravitational acceleration g — not on the bob mass or amplitude. This tool computes the period, frequency and angular frequency, and can reverse-solve for the length needed to hit a target period (e.g. the famous one-metre "seconds pendulum" ticks roughly every two seconds).

Period T

seconds / swing

Frequency f

hertz (Hz)

Angular ω

rad / s

Inverse: length needed for a target period

Length required

Uses the small-angle formula T = 2π·√(L/g) (accurate to ~0.1 % for swings under 15°). Large amplitudes require an elliptic-integral correction.

Formula

T = 2π · √(L / g) // period in seconds f = 1 / T // frequency in Hz ω = √(g / L) = 2π / T // angular frequency in rad/s L = g · (T / 2π)² // inverse: required length Standard gravity g₀ = 9.80665 m/s² // BIPM SI Brochure

Frequently asked

Why does the pendulum period not depend on the bob's mass?

In the equation of motion, the restoring force m·g·sinθ and the inertia m·a both contain mass, so the m cancels out: a = g·sinθ. That's why a brass bob and a lead bob of the same length swing at exactly the same rate. Galileo noticed this watching the cathedral lamps swing in Pisa in 1602, and Huygens turned it into the first pendulum clock in 1656.

How long should a pendulum be to tick once per second?

A "seconds pendulum" — one that ticks once per second on each half-swing, meaning a full period T = 2 s — needs L = g·(T/2π)² ≈ 9.80665 × (2/2π)² ≈ 0.9939 m under standard gravity. That is the pendulum length of traditional grandfather clocks. The adjustment screw at the bottom of the bob fine-tunes this effective length when the clock runs fast or slow.

How would the same pendulum behave on the Moon?

Lunar surface gravity is about 1.625 m/s² — roughly one-sixth of Earth's. Since T ∝ 1/√g, the same pendulum on the Moon would swing √(9.80665 / 1.625) ≈ 2.46 times slower. A grandfather clock that ticks once per second on Earth would tick once every 2.46 seconds on the Moon — Apollo astronauts famously did a related experiment dropping a hammer and a feather to verify lunar gravity.

How accurate is the formula at large swing angles?

The error in T = 2π√(L/g) grows with amplitude: roughly 0.05 % at 5°, 0.5 % at 15°, 1.7 % at 30°, 4 % at 45°, 7.3 % at 60°, and 18 % at 90°. The exact period uses the first complete elliptic integral K(sin(θ/2)): T_exact = T_small × (2/π)·K(sin(θ/2)). Precision clocks intentionally keep the swing very small (typically 1°–3°) so the simple formula is accurate enough.

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