Gravitational Force Calculator

Calculate Newtonian attraction between two masses at a known distance.

Universal gravitation calculator
Enter both masses in kilograms and their center-to-center separation in meters.

About gravitational force

Newton's law of universal gravitation states that every pair of masses attracts each other. The force magnitude equals the gravitational constant multiplied by both masses and divided by the square of the distance between their centers. This calculator uses G equal to 6.6743 × 10^-11 newton square meters per kilogram squared, with masses entered in kilograms and distance in meters. The resulting force is expressed in newtons. Force grows directly with either mass. Doubling one mass doubles the attraction, and doubling both masses makes it four times larger. Distance has an inverse-square effect. Doubling the center-to-center separation reduces force to one quarter, while tripling it reduces force to one ninth. This rapid decrease explains why ordinary objects exert gravitational forces too small to notice even though gravity acts between all masses. For spherical bodies with symmetric density, the external gravitational effect can be modeled as though each body's mass were concentrated at its center. For compact objects whose dimensions are small compared with their separation, the point-mass approximation is also useful. It becomes less accurate for nearby irregular or extended bodies because different portions of each object have different separations. Detailed models then integrate force over the mass distribution. The Newtonian equation works extremely well for classroom problems, laboratory-scale estimates, spacecraft calculations in many ordinary regimes, and planetary comparisons. General relativity is required for the highest precision, very strong gravitational fields, or relativistic conditions. Other forces may dominate at small scales, and an object's apparent weight near a planet also depends on rotation, altitude, latitude, and local geology. Use center-to-center distance rather than the gap between object surfaces. Keep all entries in SI units unless you convert them first; grams must be divided by 1000 to obtain kilograms, and kilometers multiplied by 1000 to obtain meters. The displayed scientific notation preserves very small and very large results clearly. This educational result does not include other bodies, motion, tidal effects, or relativistic corrections, but it provides a direct and reproducible application of Newton's foundational model.

Gravitational force examples

These examples use point masses and SI units.

Masses and distanceAttractive forceObservation
1 kg and 1 kg, 1 m apart6.674300e-11 NThe force equals the gravitational constant.
10 kg and 20 kg, 2 m apart3.337150e-9 NThe mass product is divided by four.
1000 kg and 500 kg, 10 m apart3.337150e-7 NStill a very small everyday force.

How to calculate gravitational force

  1. Convert the first object's mass to kilograms and enter it.
  2. Convert the second object's mass to kilograms and enter it.
  3. Measure and enter the center-to-center distance in meters.
  4. Select Calculate gravitational force and read the result in newtons.

Frequently asked questions

What is the universal gravitational constant?

The calculator uses 6.6743 × 10^-11 newton square meters per kilogram squared. It is the measured proportionality constant in Newton's universal gravitation equation.

Which distance should I enter?

Enter the distance between the centers of mass, not merely the empty gap between surfaces. For spheres, this is the distance between their geometric centers.

Why is the force between everyday objects so small?

The gravitational constant is extremely small in SI units. Electromagnetic contact forces and Earth's attraction therefore overwhelm the mutual gravity of ordinary nearby objects.

Does gravity act equally on both objects?

Yes, each object experiences a force of the same magnitude in the opposite direction. Their accelerations differ because acceleration also depends on each object's mass.

When is Newton's equation insufficient?

General relativity is needed for extreme precision, strong fields, or speeds approaching light speed. Extended irregular bodies may also require integration over their mass distributions.