Simple Pendulum Interactive Calculator

Designing a timing system or measuring local gravity with a pendulum means you need accurate period, frequency, and length relationships before you cut a single rod or write a single line of control code. Use this Simple Pendulum Interactive Calculator to calculate period, frequency, pendulum length, gravitational acceleration, maximum angular displacement, and maximum velocity using pendulum length, gravity, and initial angle as inputs. This matters across physics education, seismometer design, precision timekeeping, and geophysical surveying — anywhere pendulum dynamics drive system performance. This page includes the governing equations, a worked example, full derivation theory, and a FAQ.

What is a simple pendulum?

A simple pendulum is a weight on a string or rod that swings back and forth under gravity. Its period — the time for one complete swing — depends only on the length of the string and the local gravitational acceleration, not on the weight of the bob.

Simple Explanation

Think of a playground swing: a longer chain means a slower, longer swing. A shorter chain means faster. That relationship between length and swing time is the core of simple pendulum physics. Gravity pulls the bob back toward center each time it swings out — the stronger the pull, the faster it swings.

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How to Use This Calculator

1. Select your calculation mode from the dropdown — choose what you want to solve for: period, frequency, length, gravity, max angle, or max velocity.
2. Enter the known values into the visible input fields — pendulum length (m), gravitational acceleration (m/s²), period (s), frequency (Hz), initial angle (degrees), or max velocity (m/s) depending on the selected mode.
3. Check your units — length in meters, angles in degrees, gravity in m/s².
4. Click Calculate to see your result.

Simple Pendulum Diagram

Simple Pendulum Calculator

Governing Equations

Use the formula below to calculate the period of a simple pendulum.

Use the formula below to calculate frequency and angular frequency.

Use the formula below to calculate maximum velocity and energy per unit mass.

Simple Example

Length (L) = 1.0 m, Gravity (g) = 9.81 m/s²
T = 2π√(1.0 / 9.81) = 2.006 s
Frequency (f) = 1 / 2.006 = 0.4985 Hz
Angular frequency (ω) = √(9.81 / 1.0) = 3.132 rad/s

Theory & Practical Applications

Derivation from Restoring Torque

The simple pendulum consists of a point mass suspended by a massless, inextensible string or rigid rod of length L. When displaced from equilibrium by angle θ, gravity produces a restoring torque τ = -mgL sin θ about the pivot point. For small angles where sin θ ≈ θ (in radians), this becomes τ = -mgLθ. Applying Newton's second law for rotation (τ = Iα), where the moment of inertia I = mL² for a point mass, yields mL²(d²θ/dt²) = -mgLθ. Simplifying gives d²θ/dt² = -(g/L)θ, which is the differential equation for simple harmonic motion with angular frequency ω = √(g/L). The period follows as T = 2π/ω = 2π√(L/g).

This result reveals a counterintuitive property: the period depends only on length and gravitational field strength, remaining independent of mass and amplitude (within the small angle approximation). A 1 kg mass and a 100 kg mass attached to identical 2.48 m strings both complete one oscillation in exactly 3.16 seconds under Earth gravity. This mass independence made pendulums ideal for precision timekeeping before electronic oscillators, as variations in bob mass from temperature-induced density changes or accumulated dust had no effect on period.

Small Angle Approximation and Its Limits

The formula T = 2π√(L/g) assumes sin θ ≈ θ, valid when θ is expressed in radians and remains small. For θ₀ = 5° (0.0873 rad), sin θ₀ = 0.0872, yielding 0.1% error. At θ₀ = 15° (0.262 rad), sin θ₀ = 0.259, producing 1.2% error. By θ₀ = 30°, the error reaches 4.8%. Precision applications require the exact period formula involving complete elliptic integral of the first kind: T = 4√(L/g) K(k), where k = sin(θ₀/2) and K(k) is the elliptic integral. For θ₀ = 30°, this exact calculation gives T = 1.017 × 2π√(L/g), a 1.7% increase over the small-angle approximation.

Seismometer designers exploit this nonlinearity deliberately. Modern broadband seismometers use inverted pendulums or horizontal pendulums with periods of 30-360 seconds, requiring lengths of 223-32,400 meters if configured as simple vertical pendulums. By operating at larger angles or using mechanical advantage systems, compact designs achieve long effective periods. The STS-2 seismometer achieves a 120-second period in a 0.6 m housing by using a leaf-spring suspension that creates an extremely small effective "gravitational" restoring force.

Energy Conservation and Maximum Velocity

When released from angle θ₀, the pendulum bob falls through vertical height h = L(1 - cos θ₀). Conservation of energy requires that gravitational potential energy mgh converts entirely to kinetic energy (1/2)mv² at the bottom of the swing, yielding v_max = √(2gh) = √(2gL(1 - cos θ₀)). For θ₀ = 15°, this gives v_max = 0.2288√(gL). A 1.2 m pendulum on Earth reaches v_max = 0.783 m/s. This velocity occurs twice per cycle (once in each direction), taking the bob through equilibrium at maximum kinetic energy and zero potential energy relative to the lowest point.

The total mechanical energy E = (1/2)mv² + mgh remains constant throughout oscillation, with energy continually exchanging between kinetic and potential forms. At maximum displacement, all energy is potential (E = mgL(1 - cos θ₀)). At the bottom, all energy is kinetic (E = (1/2)mv_max²). For practical pendulums, air resistance and bearing friction dissipate energy, causing amplitude decay. High-quality pendulum clocks use escapement mechanisms to inject precise energy pulses, maintaining constant amplitude. The amplitude decay rate follows dA/dt = -γA for small damping coefficient γ, producing exponential decay A(t) = A₀e^-γt.

Gravitational Field Measurement and Pendulum Gravimetry

Rearranging T = 2π√(L/g) to solve for g gives g = 4π²L/T², enabling precise gravitational acceleration measurements through period timing. This principle underlies pendulum gravimetry, historically crucial for geophysical surveying. A pendulum with L = 1.0000 m and measured T = 2.0071 s yields g = 9.7654 m/s². Measuring period to ±0.0001 s (achievable with photogate timing) produces gravitational acceleration uncertainty of ±0.001 m/s², sufficient to detect ore deposits, underground cavities, or elevation changes.

The Kater reversible pendulum, developed in 1817, achieves even higher precision by eliminating the need to know exact pivot-to-center-of-mass distance. This compound pendulum swings from two knife-edge pivots, with period adjusted by moving masses until both pivot points yield identical periods. At this condition, the distance between knife edges exactly equals the length of an equivalent simple pendulum, determinable by direct measurement. Kater's original instrument achieved 0.0001% accuracy in g, measuring 9.81139 m/s² in London—within modern accepted values considering that local g varies from 9.78 m/s² at the equator to 9.83 m/s² at the poles due to Earth's rotation and oblate shape.

Temperature Effects in Precision Timekeeping

Clock pendulums face a subtle challenge: thermal expansion changes length L, directly affecting period. Steel has thermal expansion coefficient α ≈ 11×10⁻⁶ K⁻¹, so a 1 m steel pendulum rod expands by 0.011 mm per °C. Since period scales as √L, a 1% length increase (10 mm) produces 0.5% period increase, causing a clock to lose 432 seconds per day. Temperature variations of ±10°C throughout a year would produce ±4.3 minutes daily error.

18th-century clockmakers developed temperature-compensated pendulums using bimetallic rods or mercury-filled jars. The gridiron pendulum alternates steel and brass rods; brass's higher expansion coefficient (19×10⁻⁶ K⁻¹) allows downward brass expansion to offset upward steel expansion, maintaining constant effective length. The mercury pendulum uses mercury's volumetric expansion in a cylindrical container to raise the center of mass as the rod lengthens, compensating period changes. Modern pendulum clocks use Invar (α ≈ 1.2×10⁻⁶ K⁻¹), reducing thermal errors by 90% and achieving daily rates within ±1 second over 20°C temperature ranges.

Worked Example: Designing a Precision Gravity Measurement Apparatus

Problem: Design a simple pendulum apparatus to measure local gravitational acceleration with ±0.01 m/s² uncertainty. The laboratory has a timing system accurate to ±0.5 milliseconds. Determine the required pendulum length, expected period, number of oscillations to time, and the maximum allowable initial angle to maintain acceptable accuracy.

Part A: Optimal Pendulum Length

The fractional uncertainty in g follows from propagating uncertainties in L and T through g = 4π²L/T²:

Δg/g = ΔL/L + 2ΔT/T

For a 1.0 m length measured with a meterstick (ΔL ≈ 0.001 m), the length uncertainty contributes ΔL/L = 0.001. If we time n = 50 complete oscillations with total timing uncertainty Δt = 0.0005 s, the period uncertainty is ΔT = Δt/n = 0.00001 s. For L = 1.0 m and g ≈ 9.81 m/s², the period is approximately T = 2π√(1.0/9.81) = 2.006 s. This gives:

ΔT/T = 0.00001/2.006 = 0.000005 = 0.0005%

The fractional uncertainty in g becomes:

Δg/g = 0.001 + 2(0.000005) = 0.001010

With g ≈ 9.81 m/s², this produces Δg = 0.00991 m/s² ≈ 0.01 m/s², meeting the requirement. Using L = 1.0 m is therefore adequate.

Part B: Exact Period Calculation

Assuming g = 9.81 m/s² (to be measured), the predicted period is:

T = 2π√(L/g) = 2π√(1.0/9.81) = 2π(0.31933) = 2.0064 s

Timing n = 50 oscillations yields total time t = 50 × 2.0064 = 100.32 s. With timing precision ±0.5 ms, this gives period measurement T = 100.32/50 = 2.0064 ± 0.00001 s.

Part C: Maximum Allowable Angle

To maintain the desired 0.01 m/s² uncertainty in g, the small-angle approximation error must remain below this threshold. The period for finite amplitude follows:

T(θ₀) ≈ T₀[1 + (1/16)θ₀² + (11/3072)θ₀⁴ + ...]

where θ₀ is in radians and T₀ = 2π√(L/g). The fractional period error is:

ΔT/T₀ = (1/16)θ₀²

Since g scales as T⁻², the fractional error in g is:

Δg/g = 2ΔT/T₀ = (1/8)θ₀²

Requiring Δg/g = 0.01/9.81 = 0.00102 gives:

θ₀² = 8(0.00102) = 0.00816 rad²

θ₀ = 0.0903 rad = 5.18°

The pendulum must be released from angles less than 5.2° to avoid introducing errors exceeding the measurement uncertainty target. In practice, using θ₀ ≈ 3-4° provides additional margin.

Part D: Final Measurement Protocol

With L = 1.000 ± 0.001 m, release angle θ₀ = 4.0°, timing 50 complete oscillations, suppose the measured time is t = 100.38 ± 0.0005 s. This gives:

T = 100.38/50 = 2.0076 ± 0.00001 s

Solving for g:

g = 4π²L/T² = 4π²(1.000)/(2.0076)² = 39.478/4.0304 = 9.7954 m/s²

The uncertainty Δg follows from:

Δg = g√[(ΔL/L)² + (2ΔT/T)²] = 9.7954√[(0.001)² + (2 × 0.00001/2.0076)²]

Δg = 9.7954√[0.000001 + 0.0000001] = 9.7954(0.001049) = 0.0103 m/s²

Final result: g = 9.80 ± 0.01 m/s². This measurement accuracy would distinguish between sea level (g ≈ 9.81 m/s²) and 100 m elevation (g ≈ 9.78 m/s²) in mountainous terrain, useful for surveying applications or detecting subsurface mass anomalies in geophysical prospecting.

Applications Across Industries

Seismic monitoring relies on pendulum dynamics in horizontal and vertical seismometers. The LaCoste-Romberg gravimeter uses a zero-length spring pendulum (spring force proportional to length) to achieve periods exceeding 20 seconds, enabling detection of gravitational field variations as small as 10 μGal (10⁻⁷ g). These instruments map underground oil reservoirs, ore bodies, and magma chambers by measuring density-induced gravity anomalies.

Foucault pendulums in science museums demonstrate Earth's rotation. The pendulum's swing plane precesses at rate Ω sin φ, where Ω = 7.29×10⁻⁵ rad/s is Earth's angular velocity and φ is latitude. At 45° latitude, the precession period is 34.0 hours. A 67 m pendulum in the Panthéon (Paris) with period 16.5 seconds provides clear visual evidence of Earth's rotation through accumulation of 11.3° precession per hour.

Impact testing and ballistic pendulums measure projectile momentum and energy. A bullet embeds in a pendulum bob; measuring the resulting swing height h determines initial velocity through v = (M+m)/m × √(2gh), where M is bob mass and m is projectile mass. This technique provided pre-electronic velocity measurements accurate to 2-3%.

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