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Pendulum Calculator

Calculate the period, frequency, and length of a simple pendulum. Uses the formula T = 2π√(L/g), where L is the pendulum length and g is gravitational acceleration.

The simple pendulum is one of the oldest and most instructive systems in physics. A mass on a string, swinging under gravity, has a period that depends only on the string length and gravitational acceleration — not on the mass or (for small angles) the amplitude. This remarkable isochrony was discovered by Galileo in the late 16th century, famously while watching a swinging chandelier in Pisa's cathedral. It laid the foundation for accurate timekeeping for the next 300 years.

The formula T = 2π√(L/g) is elegantly simple. Want to double the period? Quadruple the length. A 1-meter pendulum has a period of about 2 seconds — convenient for clocks where each swing equals one second tick. A grandfather clock pendulum is typically ~0.994 m for exact 2 s period. The 67-meter Foucault pendulum at the Panthéon in Paris had a period of ~16 seconds.

Pendulums also vary with gravity. On the Moon (g = 1.62 m/s²), a 1 m pendulum takes ~4.92 s per cycle — about 2.5× slower than on Earth. Geophysicists have long used pendulums to measure local g (and infer underground density variations). Pierre Bouguer's expeditions in the 1730s used pendulum timing to discover that g varies with latitude (Earth is oblate).

This calculator uses the small-angle approximation valid for swings up to ~10-15°. Larger swings introduce nonlinear corrections — period grows slightly with amplitude. For exact analysis at large amplitudes, an elliptic integral is needed.

Common applications: clock design (grandfather clocks, metronomes), accelerometers (gravity measurement), demonstrations of Earth's rotation (Foucault pendulum), seismometers, physics education, and engineering oscillator design.

Inputs

Results

Period

2.0061 s

Frequency

0.4985 Hz

Angular Freq

3.1321 rad/s

Pendulum Results

ParameterValue
Pendulum Length1 m (100.00 cm)
Gravity9.81 m/s²
Period (T)2.006067 s
Frequency (f)0.498488 Hz
Angular Frequency (ω)3.132092 rad/s
Oscillations/min29.91
FormulaT = 2π√(L/g)
Last updated:

Formula

**Simple pendulum period (small-angle approximation):** T = 2π × √(L/g) Where: - T = period (s) — time for one complete oscillation - L = pendulum length from pivot to center of mass (m) - g = gravitational acceleration (m/s²) **Frequency:** f = 1/T = (1/2π) × √(g/L) **Angular frequency:** ω = √(g/L) **Worked example: 1 m pendulum on Earth** T = 2π × √(1/9.81) T = 2π × √(0.1019) T = 2π × 0.3193 T ≈ 2.006 s A 1-meter pendulum has a period of just over 2 seconds — the classic "seconds pendulum" used in clocks. **Length for given period:** L = g × T² / (4π²) For T = 1 s (1 Hz): L = 9.81 / 39.48 ≈ 0.248 m (25 cm). For T = 2 s (0.5 Hz): L = 9.81 × 4 / 39.48 ≈ 0.994 m (99.4 cm). **Pendulum periods (Earth, g = 9.81):** | Length L | Period T | |---|---| | 0.10 m | 0.63 s | | 0.25 m | 1.00 s | | 0.50 m | 1.42 s | | 1.00 m | 2.01 s | | 2.00 m | 2.84 s | | 5.00 m | 4.49 s | | 10.00 m | 6.35 s | | 25.0 m | 10.04 s | | 67.0 m (Foucault) | 16.43 s | **Length scales as T²:** quadrupling length doubles period. **Pendulum on other bodies (1 m pendulum):** | Body | g (m/s²) | T | |---|---|---| | Moon | 1.62 | 4.93 s | | Mars | 3.71 | 3.26 s | | Mercury | 3.70 | 3.27 s | | Venus | 8.87 | 2.11 s | | Earth | 9.81 | 2.01 s | | Saturn (cloud tops) | 10.4 | 1.95 s | | Jupiter | 24.8 | 1.26 s | | Sun | 274 | 0.38 s | **Large-angle correction:** T = 2π√(L/g) × [1 + θ²/16 + (11/3072)θ⁴ + ...] Where θ is amplitude in radians. | Amplitude | Correction | |---|---| | 5° | +0.005% | | 10° | +0.019% | | 15° | +0.043% | | 30° | +0.17% | | 45° | +0.40% | | 60° | +0.73% | | 90° | +1.80% | Small-angle formula good to ~1% for amplitudes under 15°. **Energy in a pendulum:** At maximum swing (height h above lowest point): PE_max = mgh = mgL(1 − cos θ) At lowest point: KE_max = ½mv² = mgL(1 − cos θ) For small θ: h ≈ Lθ²/2, so PE ≈ ½mgLθ². **Physical pendulum:** For a rigid body (not just point mass on string): T = 2π × √(I/(mgd)) Where: - I = moment of inertia about pivot - m = total mass - d = distance from pivot to center of mass Reduces to simple pendulum when I = mL² (point mass at distance L). **Compound (rigid) pendulum examples:** | Object | Period formula | |---|---| | Uniform rod from end | T = 2π√(2L/(3g)) | | Uniform disk from edge | T = 2π√(3R/(2g)) | | Hoop from edge | T = 2π√(2R/g) | **Foucault pendulum:** Demonstrates Earth's rotation. Plane of oscillation appears to rotate over time at rate: ω_F = (2π/24hr) × sin(latitude) At the poles: full 360° rotation per 24 hours. At 45° latitude: 360° per 33.9 hours. At equator: no apparent rotation. Original Foucault pendulum (Paris, 1851): 67 m long, 28 kg bob, demonstrated Earth's rotation conclusively. **Pendulum clocks:** Best mechanical clocks reached accuracy of ~1 sec/day. Limiting factors: temperature (changes L), friction, atmospheric drag. Shortt clock (1921): ~0.001 sec/day at best — first to detect Earth's rotation irregularities. Atomic clocks superseded mechanical: cesium fountain ~10⁻¹⁶ accuracy. **Damping and decay:** Real pendulums lose energy: - Air drag. - Pivot friction. - Pendulum string flex. Amplitude decays exponentially: θ(t) = θ₀ × e^(−γt) × cos(ωt) Where γ = damping coefficient. Quality factor Q = ω/(2γ) measures decay rate. High-Q pendulums (Foucault: Q ~ 10⁴) swing for hours; cheap toys (Q ~ 10²) swing for minutes.

How to use this calculator

  1. Enter pendulum length from pivot to center of mass in meters.
  2. Enter gravitational acceleration (default 9.81 m/s² for Earth).
  3. Calculator returns period, frequency, and angular frequency.
  4. For accurate clock design, use small amplitudes (under 10°).
  5. For larger amplitudes, expect period to be slightly longer than calculated.
  6. For exact 1 s period (seconds pendulum): L ≈ 0.248 m on Earth.

Worked examples

Grandfather clock

**Scenario:** A grandfather clock needs a 2-second period (each tick = 1 second). What length pendulum? **Calculation:** L = g × T² / (4π²) = 9.81 × 4 / 39.48 ≈ 0.994 m. **Result:** Pendulum length ~99.4 cm. Standard grandfather clocks have ~1 m pendulums. Length adjustable with a screw on the bob — clockmakers tune by raising/lowering the bob a fraction of a millimeter at a time.

Foucault pendulum

**Scenario:** Foucault's original 67-meter Pantheon pendulum. Period? **Calculation:** T = 2π × √(67/9.81) = 2π × √(6.83) = 2π × 2.61 ≈ 16.4 s. **Result:** ~16.4 seconds per cycle. Long period gives time to observe slow plane rotation (~270°/day at Paris's 49° latitude). The long, slow swing makes the rotation effect visible to the human eye over an hour or two.

Pendulum on the Moon

**Scenario:** Take a 1 m pendulum to the Moon (g = 1.62 m/s²). New period? **Calculation:** T = 2π × √(1/1.62) = 2π × √(0.617) = 2π × 0.786 ≈ 4.93 s. **Result:** ~4.93 seconds vs 2.01 s on Earth — 2.5× slower. Earth clocks brought to the Moon would run slow if not redesigned. NASA atomic clocks on Moon missions stayed accurate using cesium oscillators, not pendulums.

When to use this calculator

**Use the pendulum formula for:**

- **Clock design**: grandfather clocks, regulators, ship chronometers. - **Metronomes**: musicians' timing devices. - **Demonstrations**: physics class, science museums. - **Gravity measurement**: portable pendulum gravimeters. - **Seismic monitoring**: long-period seismometers. - **Engineering oscillators**: tuned mass dampers in skyscrapers. - **Foucault pendulums**: demonstrating Earth's rotation.

**Limitations:**

- **Small angle approximation**: errors grow for amplitudes above ~10-15°. - **Simple pendulum assumption**: requires point mass, massless string. - **Damping ignored**: real pendulums lose amplitude over time. - **Non-uniform g**: very long pendulums show g variation along length.

**Choosing a pendulum design:**

For clocks: - Length: ~1 m for 2 s period (convenient). - Bob: heavy (high momentum, less damping effect). - Suspension: knife-edge or spring (low friction). - Drive: small impulse per swing from escapement. - Compensation: bimetallic strip or invar for temperature stability.

**Foucault pendulum requirements:**

- Long: 10-70 m typical, for clear visualization. - Heavy bob: 20-200 kg, minimizes air-drag effects. - Continuous drive: electromagnetic boost to maintain amplitude. - Special suspension (gimbaled or wire): doesn't impose preferred swing plane.

**Tuned mass dampers (TMDs):**

Building-top pendulums tune to building's natural sway frequency. When wind/earthquake excites building, TMD swings out of phase, dissipating energy.

Famous examples: - Taipei 101: 660-tonne sphere, 5 m diameter, 4 stories tall. - CN Tower: 9 m TMD at top. - Citicorp Tower NYC: 400-tonne TMD.

**Gravimetric measurements:**

Pendulum period gives g: g = 4π²L / T²

Precision pendulum gravimeter: parts-per-million accuracy. Used in: - Geological surveys (oil exploration). - Geodesy (Earth's shape). - Detection of subsurface density anomalies.

Modern instruments use atom interferometry or superconducting gravimeters — even more sensitive.

**Pendulum clock history:**

- 1583: Galileo observes isochronism. - 1656: Huygens invents first pendulum clock. - 1675: Anchor escapement improves accuracy. - 1721: Graham compensation pendulum. - 1851: Foucault demonstrates Earth rotation. - 1921: Shortt clock — best mechanical timekeeper. - 1949: Atomic clocks supersede pendulums.

**Common applications:**

- **Music**: metronomes (typically 40-208 bpm). - **Sports timing**: stopwatches historically used clockwork. - **Toys**: Newton's cradle, pendulum desk ornaments. - **Demonstrations**: bowling ball pendulum showing energy conservation. - **Trapeze and swings**: same math, larger amplitudes.

**Software:**

- **MATLAB / Python**: numerical solutions including damping. - **Wolfram Mathematica**: symbolic analysis. - **Spreadsheets**: simple calculations sufficient for most uses.

**Pitfalls:**

- **Confusing length to center of mass vs string length**: matters for compound pendulums. - **Ignoring large-angle corrections**: 30° swing has 0.17% longer period. - **Forgetting damping**: real periods may have slight beat from drag. - **Using wrong g**: Earth g varies ±0.5% with latitude. - **Temperature effects**: brass pendulum lengthens 0.002%/°C; bronze 0.0018%/°C. - **Treating pendulum mass as affecting period**: it doesn't (for simple pendulum). - **Using formula for double pendulum**: complex nonlinear dynamics, often chaotic.

Common mistakes to avoid

  • Forgetting the small-angle approximation breaks down above ~15°.
  • Using string length instead of length to center of mass for real bobs.
  • Thinking mass affects period (it doesn't for simple pendulum).
  • Applying formula on rapidly rotating systems (Coriolis force matters).
  • Forgetting temperature affects length (and thus period) of clock pendulums.
  • Confusing period with frequency (reciprocals).
  • Using simple pendulum formula for physical (rigid body) pendulums.
  • Ignoring damping in real-world applications.

Frequently Asked Questions

Sources & further reading

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