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Simple Pendulum Period Calculator

Calculate the period T and frequency f of a simple pendulum instantly. Enter length (L) and gravity (g) — the formula T = 2π√(L/g) gives the exact answer. Includes a reference table for common lengths.

  • Data verified · June 2026
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The Simple Pendulum Period Calculator computes the oscillation period (T) and frequency (f) of an ideal simple pendulum using its length and local gravitational acceleration. The governing formula is T = 2π × √(L/g), where L is the pendulum length in meters and g is gravitational acceleration (9.81 m/s² at sea level on Earth). This tool applies to small-angle oscillations (θ < 15°), where the restoring force is approximately linear. Used in physics education, clock design, seismology, and gravitational field surveys, the period depends solely on length and gravity — not on mass or initial displacement (for small angles).

When to use this calculator

  • Designing a grandfather clock escapement: a 0.994 m pendulum (the 'seconds pendulum') gives exactly T = 2.000 s, one tick per second.
  • Physics lab experiment: measuring local gravitational acceleration g by timing 50 oscillations of a known-length pendulum and solving g = 4π²L/T².
  • Seismic station calibration: long-period pendulums (L = 10–100 m equivalent) are used as reference oscillators in gravimeters to detect g variations across geological formations.
  • Amusement park ride engineering: swing rides and pendulum-style attractions are modeled as simple pendulums to set safe oscillation periods and predict maximum angular velocity at the bottom of the arc.

Pendulum Period & Frequency by Length (g = 9.80665 m/s²)

Length L (m)Period T (s)Frequency f (Hz)Real-World Example
0.2481.0001.0001-second frequency standard
0.9942.0000.500Seconds pendulum (grandfather clock)
1.0002.0060.499Classic 1 m lab pendulum
2.0002.8370.352Slow decorative wall clock
4.0004.0130.249Large hall pendulum
9.8106.2830.159Period = exactly 2π seconds
25.00010.0370.100Long structural/architectural pendulum
100.00020.0740.050Geophysical / seismic reference scale

Fuente: NIST standard gravity g = 9.80665 m/s² (physics.nist.gov); fórmula T = 2π × √(L/g), válida para ángulos < 15°.

How it works

How It's Calculated

The period of a simple pendulum under the small-angle approximation is:

T = 2π × √(L / g)

Where:

  • T = Period (seconds) — time for one complete oscillation (out and back)

  • L = Effective pendulum length (meters) — from pivot to center of mass of the bob

  • g = Gravitational acceleration (m/s²) — 9.81 m/s² is standard; varies by location
  • Frequency and period are reciprocals:

    f = 1 / T = (1 / 2π) × √(g / L)

    Angular frequency (rad/s):

    ω = 2π / T = √(g / L)

    Validity condition: This formula holds when the maximum angle θ₀ < ~15°. For larger angles, the true period is:

    T_exact = 2π × √(L/g) × [1 + (1/16)θ₀² + (11/3072)θ₀⁴ + ...]

    At θ₀ = 15°, the error from using the small-angle formula is only ~0.5%.

    ---

    Period Reference Table

    All values use g = 9.80665 m/s² (standard gravity, NIST definition)

    ---

    Deriving Pendulum Length from a Target Period

    To find what length gives a desired period T:

    L = g × T² / (4π²)

    Example — seconds pendulum (T = 2.000 s):

    L = 9.81 × 4.000 / 39.478 = 0.9940 m

    ---

    Typical Cases

    Case 1 — The Classic 1-Meter Lab Pendulum


  • Inputs: L = 1.000 m, g = 9.81 m/s²

  • Calculation: T = 2π × √(1.000 / 9.81) = 2π × 0.3193 = 2.007 s

  • Frequency: f = 1 / 2.007 = 0.498 Hz

  • Interpretation: Just under one half-swing per second. A standard introductory physics result.
  • Case 2 — The Seconds Pendulum (Clockmaking)


  • Inputs: L = 0.9940 m, g = 9.81 m/s²

  • Calculation: T = 2π × √(0.9940 / 9.81) = 2π × 0.31834 = 2.000 s

  • Frequency: f = 0.500 Hz

  • Interpretation: Each half-swing ("tick" or "tock") = exactly 1 second. This is the design basis of traditional grandfather clocks. Its exact length varies slightly with latitude: ~0.9932 m at the equator (g = 9.780 m/s²) vs. ~0.9960 m at the poles (g = 9.832 m/s²).
  • Case 3 — Measuring g in the Field


  • Goal: Determine local g at a field station

  • Setup: L = 1.500 m pendulum, 50 oscillations timed at 122.6 s → T = 2.452 s

  • Solve for g: g = 4π² × L / T² = 39.478 × 1.500 / 6.012 = 9.847 m/s²

  • Interpretation: Local g is slightly above standard — consistent with a high-latitude or high-altitude location with dense subsurface rock.
  • Case 4 — Pendulum on the Moon


  • Inputs: L = 1.000 m, g_Moon = 1.625 m/s²

  • Calculation: T = 2π × √(1.000 / 1.625) = 2π × 0.7845 = 4.927 s

  • Comparison: On Earth the same pendulum ticks at 2.007 s — on the Moon it's 2.46× slower, matching the lower lunar gravity.
  • ---

    Common Errors to Avoid

    1. Using diameter instead of effective length: L must be measured from the pivot point to the center of mass of the bob, not to its bottom edge. For a 3 cm steel ball, this error introduces ~1.5 cm offset, adding ~7 ms to T at L = 1 m.

    2. Applying the formula at large angles: At θ₀ = 30°, the true period is ~1.7% longer than the small-angle prediction. At θ₀ = 90°, the error exceeds 18%. Always keep swings below 15° for formula accuracy within 0.5%.

    3. Assuming g = 9.81 m/s² everywhere: Standard gravity (9.80665 m/s²) is a defined NIST constant, but real g ranges from 9.764 m/s² (equatorial mountain tops) to 9.834 m/s² (polar sea level). Using the wrong g introduces proportional T error via √g.

    4. Ignoring air resistance and pivot friction: In a real pendulum, damping gradually reduces amplitude. The formula gives the undamped natural period; real clocks use an escapement mechanism to compensate for this energy loss and maintain constant amplitude.

    5. Confusing period with half-period: A "tick" on a grandfather clock is a half-period (one directional swing). T = 2.00 s means 1 second per tick, not 2 seconds. Misreading this doubles or halves all timing calculations.

    Worked Example: 1-meter lab pendulum

    Inputs: L = 1.000 m, g = 9.81 m/s²
    T = 2π × √(L/g) = 2π × √(1.000 / 9.81)
    T = 2π × √(0.10194) = 2π × 0.31928
    T = 2.007 s
    f = 1 / T = 1 / 2.007 = 0.498 Hz
    Period T = 2.007 s, Frequency f = 0.498 Hz

    Frequently asked questions

    What is the period of a simple pendulum formula?
    The period formula is T = 2π × √(L/g), where L is the pendulum length in meters and g is local gravitational acceleration (9.81 m/s² on Earth). This applies for small-angle oscillations (θ < 15°). The formula shows that period increases with the square root of length and decreases with stronger gravity. Mass of the bob has no effect.
    What is the period of a 1-meter simple pendulum?
    Using T = 2π × √(L/g) with L = 1 m and g = 9.81 m/s²: T = 2π × √(0.10194) = 2π × 0.31928 ≈ 2.006 s. Its frequency is f = 1/2.006 ≈ 0.498 Hz. This is one of the most common examples in introductory physics labs.
    What length pendulum gives exactly a 2-second period (seconds pendulum)?
    The 'seconds pendulum' has T = 2.000 s and requires L = g × T² / (4π²) = 9.81 × 4 / 39.478 ≈ 0.994 m at standard gravity. Each half-swing (one 'tick') is exactly 1 second — the basis of traditional grandfather clock design. The required length varies slightly by latitude: ~0.9932 m at the equator vs. ~0.9960 m at the poles.
    Does the mass of the pendulum bob affect the period?
    No. Under the simple pendulum model, mass cancels out of the equation of motion entirely. The net restoring force is proportional to mass (F = mg sinθ), and so is the inertia (F = ma), so mass divides out. Galileo confirmed this experimentally around 1602; Newton's second law explains why.
    What value of g should I use for my calculation?
    NIST defines standard gravity as exactly g = 9.80665 m/s². For most calculations, 9.81 m/s² is sufficient (error < 0.004%). For precise work — geodesy, metrology, gravimeter calibration — use your local g value. It ranges from ~9.764 m/s² near the equator at altitude to ~9.834 m/s² at sea level near the poles. NOAA's National Geodetic Survey provides local g measurements.
    At what angle does the small-angle approximation break down?
    The formula T = 2π√(L/g) uses sinθ ≈ θ (radians), which holds within 1% error for θ < ~14° (~0.245 rad). Error by angle: at 15° → 0.5%; at 30° → 1.7%; at 45° → 4%; at 90° → >18%. For larger angles, use the series correction: T_corrected = T₀ × [1 + θ²/16 + 11θ⁴/3072 + ...].
    How can I measure local gravity g with a pendulum?
    Rearrange the formula to get g = 4π² × L / T². Measure L precisely (pivot to bob center of mass). Time 20–50 complete oscillations to minimize reaction-time error, then divide total time by the number of cycles to get T. Example: L = 1.000 m, 50 swings in 100.3 s → T = 2.006 s → g = 4π² × 1.000 / 4.024 = 9.810 m/s², matching NIST standard.
    How does the pendulum period change on the Moon vs. Earth?
    The Moon's surface gravity is g_Moon = 1.625 m/s² (~1/6 of Earth's). For a 1 m pendulum: T_Moon = 2π × √(1/1.625) ≈ 4.93 s — about 2.46× longer than on Earth (2.007 s). This gravitational dependence is why pendulum clocks must be recalibrated when moved between latitudes or altitudes.
    Why does doubling the pendulum length not double the period?
    Because the formula T = 2π√(L/g) has L under a square root. Doubling L multiplies T by √2 ≈ 1.414. To double the period, you must quadruple the length. For example: L = 1 m → T ≈ 2.007 s; L = 4 m → T ≈ 4.013 s (doubled period requires 4× the length).

    Methodology & trust

    Editorial

    ciencia calculator reviewed by the Hacé Cuentas editorial team, checked against NIST — Standard Acceleration of Gravity (g = 9.80665 m/s²), following our editorial policy and methodology.

    Updates

    Last reviewed: June 2026. Parameters are verified periodically against the cited sources.

    Privacy

    Calculations run 100% in your browser. We do not store or transmit your data.

    Limitations

    Indicative results. For critical decisions, consult a professional.

    📌 How to cite this calculator
    APA format

    Rodríguez, M. (2026). Simple Pendulum Period Calculator. Hacé Cuentas. https://hacecuentas.com/en/simple-pendulum-period

    BibTeX
    @misc{hacecuentas_simple_pendulum_period_2026,
      author       = {Rodríguez, Martín},
      title        = {{Simple Pendulum Period Calculator}},
      year         = {2026},
      howpublished = {\url{https://hacecuentas.com/en/simple-pendulum-period}},
      note         = {Hacé Cuentas}
    }

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