
A relationship where a quantity is inversely proportional to the square of another.The inverse square law describes how a physical quantity — such as the intensity of light, gravity, or electrostatic force — diminishes with distance from its source. Specifically, the quantity is inversely proportional to the square of the distance. This means that if you double the distance from a point source, the intensity drops to one-quarter; triple it, and it drops to one-ninth. The law arises naturally for phenomena that spread out uniformly in three-dimensional space from a point source.
The inverse square law for gravity was formulated by Isaac Newton in his 1687 'Principia', and for electrostatic force by Charles-Augustin de Coulomb in the 1780s. The law for light intensity was recognized earlier, with Johannes Kepler and others noting the geometric dilution.
Imagine a point source emitting energy or force equally in all directions. At a distance r, that energy is spread over the surface of a sphere with area 4πr². Since the total energy is conserved, the intensity per unit area must be the total divided by the surface area, which is proportional to 1/r². This geometric dilution is the essence of the law.
It is fundamental to designing lighting systems, calculating radiation doses in medical physics, determining satellite communication link budgets, and understanding gravitational and electrostatic interactions in astrophysics and atomic physics.
The inverse square law is why the sky is dark at night: if the universe were infinite and static, every line of sight would end on a star, and the sky would be as bright as the sun's surface.






