Astronomy & Space
Intermediate

Newton's Law of Gravitation

The attractive force between any two masses.

Formula

F=Gm1m2r2F = G\frac{m_1 m_2}{r^2}

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Variables

GGravitational constant
m_1,m_2Masses
rSeparation

Example

Two 1000 kg masses 1 m apart ⇒ F ≈ 6.7×10⁻⁵ N

How it works

Newton’s law of gravitation says that every mass pulls on every other mass, and the pull gets stronger when either mass is larger. It also weakens quickly with distance because the separation is squared, so doubling the distance makes the force four times smaller. The constant G sets the overall scale of gravity in SI units and was measured experimentally; the inverse-square form matches the way a central force spreads out in three-dimensional space.

When to use it

Use this formula when you need the gravitational force between two objects that can be treated as point masses or as spherically symmetric bodies. It is common in astronomy and orbital mechanics, such as finding the attraction between planets and moons, satellites and Earth, or estimating weight-like forces at a distance.

Worked example, step by step

Find the gravitational force between Earth and a 2.0 kg object at Earth’s surface. Given: G = 6.67×10^-11 N m^2 kg^-2, m1 = 5.97×10^24 kg, m2 = 2.0 kg, r = 6.37×10^6 m Use F = Gm1m2/r^2 F = (6.67×10^-11)(5.97×10^24)(2.0) / (6.37×10^6)^2 F = (7.96×10^14) / (4.06×10^13) F ≈ 19.6 N So the gravitational force is about 20 N, which is the object’s weight near Earth’s surface.

Common mistakes to avoid

  • Forgetting to square the distance r in the denominator
  • Using kilometres or metres inconsistently instead of converting everything to SI units
  • Mixing up mass and weight, or using the wrong value for G

Did You Know?

Henry Cavendish "weighed the world" in 1798, measuring G with a delicate torsion balance in a sealed shed.

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Reviewed & maintained by the FormulaWon editorial teamLast reviewed September 2026