Formulas & tables/Physics/Gravitation/Newton's law of universal gravitation

Newton's law of universal gravitation

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

Result unit: N (newton)

What it describes

Two bodies attract each other with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.

Symbols

FF
gravitational force
[N]
GG
gravitational constant (≈6.67⋅10−11\approx 6.67\cdot10^{-11})
[N·m²/kg²]
m1,m2m_1, m_2
masses of the bodies
[kg]
rr
distance between the bodies
[m]

Where it comes from

Every pair of bodies attracts each other. The force falls off quickly with distance (as the square) — doubling the separation weakens it fourfold. Bodies much smaller than the distance between them are treated as point masses.

When to use it

Interactions of masses (planets, satellites, falling bodies). This law gives rise to g=GM/R2g=GM/R^2 and the cosmic velocities.

Example

Find the attractive force between two 1000 kg masses 2 m apart.
Substitutionm1=m2=1000m_1=m_2=1000 kg, r=2r=2 m, G=6.67⋅10−11G=6.67\cdot10^{-11}.
ResultF=6.67⋅10−11⋅1064≈1.7⋅10−5F=6.67\cdot10^{-11}\cdot\dfrac{10^6}{4}\approx1.7\cdot10^{-5} N.

Related formulas

Found this formula useful? Share it.

It's free — send it to a friend who's revising.

Teaching? Embed this formula on your site.

Free widget — paste it on your school site, blog or notes. It links to the full version.

Teaching a class or tutoring? Guide students in NexTutor →