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Simple Pendulum

A simple pendulum consists of a point mass suspended from a fixed point by a massless string. For small angles, the motion is simple harmonic with period T = 2π√(L/g), independent of mass and amplitude.

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Period is independent of mass—heavier and lighter bobs swing at the same rate. Doubling length increases period by √2 ≈ 1.41×. A seconds pendulum (T=2s) has length ≈ 0.994 m on Earth. Foucault pendulums demonstrate Earth's rotation; the swing plane appears to rotate.

Key quantities
T = 2π√(L/g)
Period
Key relation
f = 1/T
Frequency
Key relation
L (m)
Length
Key relation
v_max = ωLθ₀
Max Velocity
Key relation

Ready to run the numbers?

Why: Pendulum physics underpins timekeeping (clocks, metronomes), gravimetry, and demonstrations of Earth's rotation (Foucault pendulum). Understanding period-length relationships is essential for mechanical oscillators.

How: The period depends only on length and gravity: T = 2π√(L/g). Mass and amplitude (for small angles) do not affect the period. Energy alternates between kinetic and potential.

Period is independent of mass—heavier and lighter bobs swing at the same rate.Doubling length increases period by √2 ≈ 1.41×.

Run the calculator when you are ready.

Solve the Pendulum EquationEnter length, period, or frequency to calculate pendulum properties

🕰️ Grandfather Clock

1m pendulum for 2-second period

🎢 Playground Swing

3m chain swing

🎵 Metronome

Period = 0.5s (120 BPM)

🌍 Foucault Pendulum

67m museum pendulum

🌙 Pendulum on Moon

1m pendulum, g = 1.62 m/s²

🔬 Physics Lab

50cm lab pendulum

🏗️ Wrecking Ball

20m cable, 500kg ball

💎 Earring Swing

3cm dangling earring

🎡 Pendulum Ride

15m amusement ride

⏱️ Seconds Pendulum

T = 2s exactly (L ≈ 0.994m)

Enter Your Values

For educational and informational purposes only. Verify with a qualified professional.

🔬 Physics Facts

⏱️

Galileo discovered pendulum isochronism in 1583 by observing a chandelier in Pisa Cathedral.

— History of Physics

🕰️

Christiaan Huygens built the first pendulum clock in 1656, revolutionizing timekeeping.

— Horology

🌍

Foucault's 1851 pendulum in Paris demonstrated Earth's rotation without external reference.

— Classical Mechanics

📐

For angles <15°, the small-angle approximation sin(θ)≈θ holds with <1% error.

— Harmonic Motion

What is a Simple Pendulum?

A simple pendulum consists of a point mass suspended from a fixed point by a massless, inextensible string. When displaced from equilibrium and released, it oscillates in a vertical plane under gravity. For small angles, the motion is simple harmonic with a period that depends only on length and gravity—not on mass or amplitude.

⏱️

Period Independence

The period depends only on length (L) and gravity (g), not on mass or amplitude (for small angles).

T = 2π√(L/g)

📐

Small Angle Approximation

For angles less than ~15°, sin(θ) ≈ θ, making the motion truly simple harmonic.

At 15°: sin(15°) = 0.259, θ = 0.262 rad

Error: ~1%

Energy Conservation

Total mechanical energy is conserved (ignoring friction). PE and KE continuously interchange.

E = PE + KE = constant

How to Calculate Pendulum Properties

🧮 Period & Frequency

Period

T = 2π√(L/g)

Frequency

f = 1/T = (1/2π)√(g/L)

Angular Frequency

ω = 2πf = √(g/L)

📊 Position & Velocity

Angular Position

θ(t) = θ₀ cos(ωt)

Angular Velocity

ω(t) = -θ₀ω sin(ωt)

Max Linear Velocity

v_max = ωLθ₀

Applications of Simple Pendulums

🕰️ Timekeeping

Grandfather clocks, metronomes, and early scientific instruments used pendulum regularity for precise timing.

🌍 Measuring Gravity

Gravimeters use pendulum period to detect gravity variations for geological surveys and mineral exploration.

🔬 Physics Education

Classic experiment for demonstrating harmonic motion, energy conservation, and period-length relationships.

🌐 Earth Rotation

Foucault pendulums demonstrate Earth's rotation as the swing plane appears to rotate over hours.

🏗️ Construction

Plumb bobs and construction pendulums establish vertical reference lines for accurate building.

🎢 Amusement Rides

Pendulum rides use the physics of oscillation for thrilling but predictable motion.

Complete Formula Reference

Period

T = 2π√(L/g)

Length from Period

L = gT²/(4π²)

Max Velocity

v_max = √(2gL(1-cosθ₀))

Max Height

h = L(1 - cosθ₀)

String Tension (max)

T_max = mg(3 - 2cosθ₀)

Total Energy

E = mgL(1 - cosθ₀)

Large Angle Corrections

For larger angles, the simple formula T = 2π√(L/g) underestimates the period. A more accurate formula includes correction terms:

T = 2π√(L/g) × [1 + (1/16)θ₀² + (11/3072)θ₀⁴ + ...]
Initial AnglePeriod Error (simple formula)
0.05%
15°0.5%
30°1.7%
45°4.0%
60°7.3%
90°18%

Frequently Asked Questions

Why doesn't mass affect the period?

The gravitational force (mg) and the inertial resistance (ma) both depend on mass. They cancel out in the equation of motion, leaving period independent of mass—just like free fall!

How does a grandfather clock keep accurate time?

The pendulum is adjusted to exactly 1 meter (for T = 2s). An escapement mechanism gives the pendulum small impulses to overcome friction, maintaining constant amplitude without affecting period.

Would a pendulum work on the Moon?

Yes, but with a longer period! Moon's gravity is ~1/6 of Earth's, so T_moon = T_earth × √6 ≈ 2.45 times longer. A seconds pendulum (T=2s on Earth) would have T≈4.9s on the Moon.

Why does a Foucault pendulum appear to rotate?

It doesn't actually rotate—the Earth rotates beneath it! The swing plane stays fixed relative to the stars while Earth turns. At the poles, it completes one apparent rotation in 24 hours.

Reference: Pendulum Lengths for Common Periods

Period (s)Length (m)Length (cm)Application
0.50.0626.2Fast metronome (120 BPM)
1.00.24824.8Quick pendulum
2.00.99499.4Seconds pendulum (clock)
3.02.236223.6Large clock
5.06.21621Slow swing
10.024.852485Large Foucault pendulum

Tips and Common Mistakes

✅ Best Practices

  • • Keep initial angle small (<15°) for accuracy
  • • Measure length to center of mass of bob
  • • Time multiple swings and divide
  • • Ensure pivot has minimal friction

❌ Common Mistakes

  • • Using large angles without correction
  • • Measuring length to bottom of bob
  • • Ignoring string mass for accuracy
  • • Forgetting period is independent of mass

Practice Problems

Problem 1: Clock Pendulum

What length pendulum gives exactly T = 1 second?

L = gT²/(4π²) = 9.81 × 1²/(4π²) = 0.248 m = 24.8 cm

Problem 2: Maximum Speed

A 1m pendulum starts at 10°. What's its maximum speed?

v_max = √(2gL(1-cosθ₀)) = √(2 × 9.81 × 1 × (1-cos10°))
v_max = √(19.62 × 0.0152) = 0.546 m/s

Problem 3: Planetary Pendulum

A pendulum has T = 2s on Earth. What's its period on Mars (g = 3.72 m/s²)?

T ∝ 1/√g, so T_Mars = T_Earth × √(g_Earth/g_Mars)
T_Mars = 2 × √(9.81/3.72) = 2 × 1.624 = 3.25 seconds

Historical Significance

🔬 Galileo Galilei (1583)

At age 19, Galileo noticed that a swinging chandelier in the Pisa cathedral took the same time per swing regardless of amplitude. This observation led to the discovery of pendulum isochronism.

⏰ Christiaan Huygens (1656)

Built the first practical pendulum clock, which revolutionized timekeeping. His work on pendulum theory established the mathematics of oscillatory motion.

🌍 Léon Foucault (1851)

Demonstrated Earth's rotation using a 67m pendulum in the Panthéon, Paris. The swing plane appeared to rotate as Earth turned beneath it.

📐 Henry Kater (1817)

Invented the reversible pendulum for precise measurement of gravitational acceleration, which remained the standard method for over a century.

Pendulum Periods on Different Celestial Bodies

Bodyg (m/s²)Period (1m pendulum)Relative to Earth
Sun (surface)2740.38 s0.19×
Mercury3.703.27 s1.63×
Venus8.872.11 s1.05×
Earth9.812.01 s1.00×
Moon1.624.93 s2.46×
Mars3.723.26 s1.62×
Jupiter24.791.26 s0.63×

Derivation of Pendulum Motion

Step 1: Restoring Force

The component of gravity tangent to the arc provides the restoring force:

F = -mg sin(θ)

Step 2: Newton's Second Law

For arc length s = Lθ and acceleration d²s/dt² = L d²θ/dt²:

mL(d²θ/dt²) = -mg sin(θ)

Step 3: Small Angle Approximation

For small θ, sin(θ) ≈ θ, giving simple harmonic motion:

d²θ/dt² = -(g/L)θ → ω² = g/L → T = 2π√(L/g)

Key Relationships Summary

Double length

1.41× period

T ∝ √L

Quadruple length

2× period

T ∝ √L

Double gravity

0.71× period

T ∝ 1/√g

Double mass

Same period!

T independent of m

Real Pendulums: Damping Effects

Real pendulums lose energy to air resistance and friction at the pivot. The amplitude decreases exponentially over time, though the period remains nearly constant for light damping.

Damped Motion

Amplitude decreases over time:

θ(t) = θ₀ e^(-γt) cos(ω't)
ω' = √(ω₀² - γ²)

Quality Factor

Measures energy loss per cycle:

Q = ω₀/(2γ)
Higher Q = less damping

Frequently Asked Questions

Why doesn't mass affect the period of a simple pendulum?

The gravitational force (mg) and the inertial resistance (ma) both depend on mass. They cancel out in the equation of motion, leaving period independent of mass—just like free fall! This is a fundamental property of simple harmonic motion under gravity.

How does a grandfather clock keep accurate time?

The pendulum is adjusted to exactly 1 meter (for T = 2s). An escapement mechanism gives the pendulum small impulses to overcome friction, maintaining constant amplitude without affecting period. The period depends only on length and gravity, making it very stable.

Would a pendulum work on the Moon?

Yes, but with a longer period! Moon's gravity is ~1/6 of Earth's, so T_moon = T_earth × √6 ≈ 2.45 times longer. A seconds pendulum (T=2s on Earth) would have T≈4.9s on the Moon. The pendulum would swing much slower but still oscillate.

Why does a Foucault pendulum appear to rotate?

It doesn't actually rotate—the Earth rotates beneath it! The swing plane stays fixed relative to the stars while Earth turns. At the poles, it completes one apparent rotation in 24 hours. This demonstrates Earth's rotation without external reference.

What is the small angle approximation and when does it fail?

For angles less than ~15°, sin(θ) ≈ θ, making the motion truly simple harmonic. At 15°, the error is only ~1%. For larger angles, the period increases. At 30°, error is ~1.7%; at 60°, it's ~7.3%. The simple formula T = 2π√(L/g) underestimates period for large angles.

How do you measure gravitational acceleration using a pendulum?

Measure the period T and length L precisely, then use g = 4π²L/T². This is the principle behind gravimeters used in geological surveys. The Kater reversible pendulum was the standard method for measuring g for over a century, achieving accuracies better than 0.01%.

What causes damping in real pendulums?

Real pendulums lose energy to air resistance (proportional to velocity squared) and friction at the pivot (proportional to velocity). The amplitude decreases exponentially: A(t) = A₀e^(-γt). The quality factor Q = ω₀/(2γ) measures how many oscillations before significant decay.

📚 Official Data Sources

NIST Physical Measurement Laboratory

US National Institute of Standards - Physical constants and measurements

Last Updated: 2026-02-01

MIT OpenCourseWare Physics

MIT physics courses including harmonic motion and pendulums

Last Updated: 2025-12-15

Physics Hypertextbook

Comprehensive physics reference including pendulum mechanics

Last Updated: 2025-11-20

HyperPhysics (Georgia State)

Georgia State University physics reference - pendulum oscillations

Last Updated: 2025-10-10

⚠️ Disclaimer: This calculator provides theoretical estimates based on the simple pendulum formula T = 2π√(L/g), which assumes small angles, massless string, point mass bob, and no damping. Actual pendulum behavior may vary due to air resistance, string mass, pivot friction, large-angle effects, and environmental factors. For angles greater than 15°, corrections are needed. Always verify critical measurements with professional instruments. This calculator is for educational and planning purposes only.

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