m/s²
A simple pendulum is one of the most fundamental concepts in classical mechanics, consisting of a mass (called the bob) suspended from a fixed point by a massless, inextensible string or rod. When displaced from its equilibrium position and released, the pendulum oscillates back and forth under the influence of gravity, demonstrating periodic motion that has fascinated physicists and mathematicians for centuries.
The time period (T) of a simple pendulum—the time it takes to complete one full oscillation—is determined by a remarkably elegant equation, where L is the length of the pendulum in meters and g is the acceleration due to gravity (approximately 9.81 m/s² on Earth).
T = 2π√(L/g)This formula reveals a profound insight: the period depends only on the length and gravity, not on the mass of the bob or the amplitude of swing (for small angles).
The simple pendulum exhibits several remarkable characteristics. First, it demonstrates isochronism—the property that small oscillations take the same time regardless of amplitude. This property, discovered by Galileo, led to the development of pendulum clocks. Second, the motion is approximately simple harmonic for angles less than 15 degrees, meaning the restoring force is proportional to displacement. Third, the frequency (f = 1/T) represents how many complete cycles occur per second, measured in Hertz (Hz).
💡 Key Insight
The angular frequency (ω = 2π/T) describes the rate of change of the pendulum's angular position. Measured in radians per second, it provides a convenient way to express oscillatory motion. For a simple pendulum, ω = √(g/L), showing how both gravity and length influence oscillation.
Understanding pendulum physics has practical applications across multiple fields. Seismology uses pendulum principles to design seismometers that detect earthquake waves. Engineering applies pendulum dynamics to analyze suspension bridges, building sway, and mechanical systems. Historical timekeeping devices like grandfather clocks relied on carefully calibrated pendulums for accurate time measurement. Even modern physics experiments use pendulums to measure gravitational acceleration with high precision.
⚠️ Gravitational Variation
The gravitational acceleration g varies slightly across Earth's surface due to altitude, latitude, and local geology. At sea level near the equator, g ≈ 9.78 m/s², while at the poles it's approximately 9.83 m/s². This variation means a pendulum clock calibrated in one location will run at a different rate elsewhere—a crucial consideration for precision timekeeping before modern electronic clocks.
This calculator provides three powerful calculation modes. In Find Period mode, input the pendulum length and gravity to determine how long one complete swing takes. Find Length mode reverses the calculation—given a desired period and gravity, it computes the required pendulum length. Find Gravity mode is particularly useful in experimental physics, calculating the local gravitational acceleration from measured period and length.
✨ Unit Flexibility
The tool supports multiple unit systems for convenience. Length can be entered in meters (m), centimeters (cm), feet (ft), or inches (in), while time accepts seconds (s) or milliseconds (ms). For gravity calculations, you can manually enter a value or select from preset options for different celestial bodies, including Earth, Moon, Mars, Jupiter, and other planets, making it easy to explore how pendulums would behave in different gravitational environments.
The calculator includes an animated visualization that brings the physics to life. Watch as the pendulum bob swings back and forth with timing synchronized to your calculated period, providing immediate visual feedback. This animation helps develop intuition about how changing parameters affects motion—longer pendulums swing more slowly, while stronger gravity accelerates the oscillation.
While the simple pendulum formula is remarkably accurate for small angles, real pendulums experience additional effects:
🌪️ Air Resistance
Gradually dampens oscillations, causing the amplitude to decrease over time.
⚖️ String Mass
Assumed zero in the simple model, but slightly affects the period for physical pendulums.
📐 Large Amplitudes
Over 15° introduce nonlinear effects that make the period amplitude-dependent.
For precision applications, these factors must be considered alongside the basic calculation.
The simple pendulum serves as an excellent teaching tool for fundamental physics concepts. It demonstrates conservation of energy (kinetic and potential energy interchange), periodic motion, the relationship between force and acceleration, and how mathematical models describe physical phenomena. Students can easily conduct experiments with real pendulums and compare results to theoretical predictions, reinforcing the connection between mathematics and observable reality.
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A simple pendulum consists of a mass (bob) suspended from a fixed point by a massless string or rod. When displaced from its equilibrium position and released, it oscillates back and forth under the influence of gravity. The motion is approximately simple harmonic for small angles.
The time period T of a simple pendulum is calculated using the formula T = 2π√(L/g), where L is the length of the pendulum in meters and g is the acceleration due to gravity (9.81 m/s² on Earth). The period depends only on length and gravity, not on the mass or amplitude (for small angles).
Gravity provides the restoring force that pulls the pendulum back toward its equilibrium position. A stronger gravitational field (higher g) creates a stronger restoring force, causing the pendulum to swing faster and reducing its period. On the Moon (g = 1.62 m/s²), the same pendulum would swing much slower than on Earth.
No, the mass of the pendulum bob does not affect the time period for a simple pendulum. This is because both the gravitational force and the inertia are proportional to mass, so they cancel out in the equation. Only length and gravity determine the period.
Frequency (f) is the inverse of period (T): f = 1/T. If a pendulum has a period of 2 seconds, it completes 0.5 oscillations per second (0.5 Hz). Angular frequency (ω) is related by ω = 2πf = 2π/T and represents the rate of change of angular position.
The formula T = 2π√(L/g) is highly accurate for small angular displacements (less than 15 degrees). For larger angles, the actual period becomes longer than predicted because the restoring force is no longer proportional to displacement. The approximation also assumes a massless, inextensible string and no air resistance.