The Simple Pendulum
The simple pendulum consists of a bob of mass m attached to a massless inextensible string of length L. This pendulum swings around a fixed point, executing periodic motion. When the bob is displaced from its vertical equilibrium position by a small angle θ, gravitational forces lead to a restoring torque that brings it back to equilibrium.
Forces Acting on the Pendulum
- At the mean position (θ = 0), gravitational force (mg) acts downward while tension (T) acts along the string. The component of gravitational force (mg sin θ) provides the tangential acceleration, while mg cos θ provides radial acceleration.
- The torque due to the tangential force can be described with the equation:
\[ \tau = -L(mg \sin \theta) \]
- Applying Newton's second law of rotational motion results in:
\[ I \alpha = -mgL \sin \theta \]
Giving rise to an angular motion approximation, the motion becomes simple harmonic for small angles:
\[ \alpha \approx -\frac{mg}{I} \theta = -\frac{g}{L} \theta \]
The Time Period of the Pendulum
The relationship between the pendulum length and the period is captured by the formula:
\[ T = 2\pi \sqrt{\frac{L}{g}} \]
Where T is the time period of the pendulum, L is the length, and g is the acceleration due to gravity.
In conclusion, a simple pendulum exhibits periodic motion closely related to simple harmonic motion (SHM) when the angle of displacement is small, enabling the derivation of its oscillation period based on length.