Part of the Engineering & Mechanics suite · 123 calculators

Inverse Square Law Calculator

How intensity falls with distance from a point source — light, sound, radiation, a radio signal or gravity — and the distance at which it reaches a level you choose.

Anything spreading evenly from a point covers a sphere whose area grows with the square of the radius, so the intensity per unit area falls with the square: double the distance, a quarter of the intensity.

Results update as you type
Results
Intensity at the second distance
4
Change
Change in decibels
Distance where the target intensity is reached
Reviewed September 2026. Physics is the same everywhere: SI units in, with imperial equivalents in the results.
No account required · Google Analytics off unless allowedCalculator arithmetic runs in your browserResults update as you type
All calculations run 100% in your browser. The calculator code does not submit your figures to GlobalCalc to obtain a result.
About inverse square law

How the inverse square law calculator works

Anything spreading evenly from a point covers a sphere whose area grows with the square of the radius, so the intensity per unit area falls with the square: double the distance, a quarter of the intensity. The same law governs illumination, radiation dose, sound pressure squared, and gravitational and electric force. The decibel row is 20 log₁₀ of the distance ratio.

Formula: I₂ = I₁ × (d₁ ÷ d₂)²; d = d₁ × √(I₁ ÷ I_target)

Worked examples

InputsIntensity at the second distanceNote
100 at 1 m → 5 m44 — a 25th
Halving the distance200200 — four times
Sunlight at Mars (1.52 AU)589.0755589 W/m²

Frequently asked questions

Why the square?

Because the surface of a sphere is 4πr². Whatever spreads evenly from a point is shared over that area, so each square meter gets a share that shrinks with r².

Does it apply to sound?

To sound intensity (power per area), yes — and sound pressure falls with plain distance, which is why the decibel drop is 6 dB per doubling either way. Indoors, reflections stop the fall-off within a few meters.

Does it apply to a beam or a long lamp?

Not exactly. A collimated laser hardly spreads, a long fluorescent tube falls off with distance rather than its square until you are far away, and a spotlight follows the law only within its beam.

How is this used in radiation safety?

Distance is the cheapest shield: stepping from 1 m to 3 m from a source cuts the dose rate to a ninth. Time, distance and shielding are the three rules.

Where these figures come from

Last checked: September 2026. Constants are the CODATA 2018 values; formulas are the standard textbook forms.