Linked from

The 38 pages that link to Inverse-square law, each with the reason it gives.

• Tidal forceRelated: Newtonian gravity’s distance dependence creates stronger pull on the nearer side of a body.

• Virial theoremRelated: Newtonian gravity’s distance dependence fixes the familiar factor relating kinetic and potential energy.

• Solar irradianceRelated: It explains how solar irradiance changes as the distance from the Sun changes.

• Escape velocityRelated: The weakening of gravity with distance makes the escape-energy integral finite.

• Gravitational accelerationRelated: Gravity’s inverse-square dependence makes acceleration weaken with distance.

• Standard candleRelated: It converts a candle’s luminosity and observed brightness into distance.

• Absolute magnitudeRelated: Its distance dependence explains why brightness must be corrected before comparing intrinsic luminosities.

• Gravitational fieldRelated: Newtonian gravity’s field around a point mass follows this distance dependence.

• Gravitational constantRelated: Newton’s gravitational force follows this distance dependence, leaving G as its constant factor.

• Gravitational forceRelated: Newtonian gravitational strength falls with the square of separation.

• IlluminanceRelated: For a point source, illuminance falls with distance squared when orientation is fixed.

• Radiant intensityRelated: It converts source intensity into irradiance at a distance.

• Distance modulusRelated: It produces the logarithmic distance dependence encoded by distance modulus.

• Biot–Savart lawRelated: A current element’s field contribution falls with the square of its distance from the observation point.

• IrradianceRelated: It predicts how irradiance from a compact source falls as a surface moves away.

• Cavendish experimentRelated: The experiment’s force measurements depended on the predicted distance scaling of gravity.

• RadiometryRelated: For a point source, it links radiant intensity to irradiance with distance.

• Solar radiation pressureRelated: Sunlight intensity, and therefore pressure, falls with the square of solar distance.

• Luminous intensityRelated: It governs illuminance from a source when its luminous intensity is known.

• Dental radiographyRelated: Increasing distance from the X-ray source reduces exposure at the patient and operator.

• Solar constantRelated: It explains how solar irradiance changes with distance from the Sun.

• Bolometric luminosityRelated: Observed bolometric flux becomes intrinsic luminosity when distance is known.

• Flash photographyRelated: Moving a flash closer can sharply increase illumination and change brightness differences across a scene.

• Fifth forceRelated: Short-range tests look for departures from gravity's inverse-square behavior.

• Gauss's law for gravityRelated: Newtonian gravity's inverse-square dependence underlies the closed-surface flux relation.

• Heinrich Wilhelm Matthias OlbersRelated: Olbers’s paradox assumes distant stars dim according to this law, producing the apparent divergence.

• Newton's theorem of revolving orbitsRelated: Newton's orbital theory grew from connecting inverse-square attraction with Keplerian paths.

• Three-dimensional system (spatial)Related: In three spatial dimensions, spreading over spherical surfaces produces inverse-square behavior.