In optics, the power of a lens, represented as 'P', is a critical property that quantifies how much a lens can converge or diverge light. Specifically, power is defined as the inverse of the focal length (f) measured in meters:
\[ P = \frac{1}{f} \]
where the unit of power is diopters (D), with 1D equal to the power of a lens having a focal length of 1 meter. A positive power corresponds to a converging lens (convex), which brings parallel rays of light to a focus, while a negative power corresponds to a diverging lens (concave), which causes light to spread apart.
The section outlines various examples that demonstrate how to calculate the power based on given focal lengths and interpret the significance of the calculated powers in practical applications like corrective lenses. Understanding lens power is essential not only for optical designs but also serves many daily applications in vision correction.