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Physics calculators

Physics

Universal gravitation calculator

Compute the gravitational attraction between any two masses, with presets for Earth-Moon, Sun-Earth and Earth-satellite pairs.

Inputs

G = 6.674e-11 N m²/kg²

Common bodies (mass, radius)
  • Earth: M = 5.972e+24 kg, R = 6.371e+6 m
  • Moon: M = 7.342e+22 kg, R = 1.737e+6 m
  • Mars: M = 6.417e+23 kg, R = 3.390e+6 m
  • Sun: M = 1.989e+30 kg, R = 6.960e+8 m
  • Jupiter: M = 1.898e+27 kg, R = 6.991e+7 m
Result
Gravitational force F
4348N
Field due to m₂ at m₁
7.281e-22m/s²
Field due to m₁ at m₂
8.696m/s²

F = G m₁ m₂ / r², g = G M / r².

How this calculator works

The calculator multiplies the two masses, divides by the square of their separation, and multiplies by G = 6.674 × 10⁻¹¹ N m²/kg² to get the gravitational force. It then computes the gravitational field strength each mass would produce at the location of the other.

Common questions

What is Newton's law of universal gravitation?
F = G m₁ m₂ / r², where G = 6.674 × 10⁻¹¹ N m²/kg². Every pair of point masses attracts the other along the line joining them with this magnitude.
Is r measured from the surface or the centre?
From the centre of each body. For a satellite at altitude h above Earth, r = R_Earth + h, not just h.
What is gravitational field strength?
g = F/m = GM/r². The field strength at a point is the force per unit mass on a test mass placed there, measured in N/kg or m/s².
Why is r squared?
Gravitational field lines spread out over a sphere of area 4πr². The field strength is inversely proportional to that area, giving an inverse-square law in distance.