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Newton's law of universal gravitation: F = G m₁m₂ / r²

A student says that of two pairs at the same separation, the heavier pair pulls harder. Is the student correct?

A heavier pair sat farther apart; a lighter pair sat closer together. Your two rules shrugged: they could not settle which force wins. Newton's law settles every such case, because it gives the force as a number.

You have seen that increasing either mass strengthens the force, and that distance weakens it by the inverse square: the 36 N force on the probe fell to 9 N at twice the distance. One equation ties the whole story together.

Newton's law of universal gravitation: F = G m₁m₂ / r²
F = G m₁m₂ / r²Newton's law of universal gravitation

The two masses multiply together on top. Increase either one, and F grows.

symbolnameunitm₁mass of the first objectkgm₂mass of the second objectkg
The two masses sit on top of the fraction: they multiply together.

The distance r is squared underneath. Double r, and F falls to one quarter: the inverse-square law you know.

r runs center to center: from the center of one object to the center of the other, in meters. r is never the surface-to-surface gap.

symbolnameunitm₁mass of the first objectkgm₂mass of the second objectkgrdistance between the two centersm
The distance r is squared underneath, and r runs center to center.

In F = G m₁m₂ / r², which distance is r?

G is a constant: the same multiplier in every gravity calculation, everywhere. G's unit is chosen so that F comes out in newtons. The value of G comes in the next lesson.

symbolnameunitFgravitational force between the two objectsNGuniversal gravitational constantN·m²/kg²m₁mass of the first objectkgm₂mass of the second objectkgrdistance between the two centersm
Each symbol, its meaning, and its unit.

One of two moored ships takes on cargo, doubling its mass, the other ship and the distance unchanged. Use F = G m₁m₂ / r² to say what happens to the force between them.

Write down the equation:

F = G m₁m₂ / r²

Read off what changed:

m₁ doubles; m₂, r and G are unchanged.

The top of the fraction doubles.

The force F doubles.

In F = G m₁m₂ / r², how do the two masses enter?

The two ships then drift to twice their old separation. What does the law say now?

Write down the equation:

F = G m₁m₂ / r²

Read off what changed:

r doubles, so r² grows by 2² = 4.

The bottom of the fraction grows four times larger.

The force F falls to one quarter of its value.

In F = G m₁m₂ / r², how does the distance enter?

Your turn

Which of the following is Newton's law of universal gravitation?

Which pairing of a symbol from F = G m₁m₂ / r² with its unit is correct?

A satellite orbits 3.0 × 10⁵ m above Earth's surface. Earth's radius is 6.4 × 10⁶ m. Enter the r for Newton's law, in meters.