Newton’s Law of Gravitation
- State the law of universal gravitation and compute the force between two masses
- Relate a planet’s surface gravity to its mass and radius through g = GM/R²
- Predict how gravitational force changes with separation using the inverse-square law
Every mass attracts every other mass
Newton’s law of universal gravitation says any two point masses attract along the line joining them with a force proportional to each mass and inversely proportional to the square of their separation. The constant G = 6.67 × 10⁻¹¹ N·m²/kg² is tiny, which is why gravity is only noticeable when at least one mass is astronomical. A uniform sphere acts gravitationally as if all its mass were at its center, so r is measured center-to-center.
Surface gravity ties g to a planet
Set the gravitational force on a mass m at a planet’s surface equal to mg: G M m / R² = m g. The mass m cancels — the reason all objects fall with the same g — leaving g = GM/R². This is why g depends on the planet, not the falling object. Above the surface, replace R with the distance r from the center; because of the inverse square, g falls off as 1/r² as you climb.
A planet has the same mass as Earth but half its radius. How does the free-fall acceleration g at its surface compare with Earth’s?
- 1.Surface gravity is g = GM/R², so with M fixed, g scales as 1/R².
- 2.Halving the radius replaces R with R/2, giving a factor 1/(R/2)² = 1/(R²/4) = 4/R².
- 3.Therefore g_planet = GM/(R/2)² = 4 GM/R² = 4 g_Earth.
- 4.The smaller radius brings the surface much closer to the mass, so the inverse-square law makes gravity four times stronger.
The gravitational force between two masses is F. If the distance between their centers is doubled (masses unchanged), the new force is:
A planet has twice Earth’s mass and twice Earth’s radius. Its surface gravity compared with Earth’s is:
Keep the two formulas straight: F = Gm₁m₂/r² is the force between two masses, while g = GM/R² is the field (acceleration) one mass produces at distance R. Both are inverse-square — whenever a distance changes, square the ratio before scaling.
Answer the 2 checkpoints as you read.
Sign in to save your progress