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Newton's Law of Universal Gravitation

๐Ÿ“Š intermediate
$$F = G\frac{m_1 m_2}{r^2}$$
Attractive force between two masses is proportional to product of masses and inversely proportional to square of distance.
Variables & Units
$F$
Gravitational force
Unit: $\text{N}$
$G$
Gravitational constant
Unit: $\text{Nยทm}^2/\text{kg}^2$
$m_1, m_2$
Masses
Unit: $\text{kg}$
$r$
Distance between centers
Unit: $\text{m}$
Key Information
๐Ÿ“ Derived From
Kepler's laws and empirical observation
๐Ÿ’ก Example
Earth ($5.97\times10^{24}\,\text{kg}$) and Moon ($7.35\times10^{22}\,\text{kg}$) separated by $3.84\times10^8\,\text{m}$: $$F = 6.67\times10^{-11}\frac{(5.97\times10^{24})(7.35\times10^{22})}{(3.84\times10^8)^2} \approx 1.98\times10^{20}\,\text{N}$$
๐Ÿ”ง Applications
Orbital mechanics, satellite trajectories, tidal predictions
โš ๏ธ Constraints
Valid for point masses or spherical distributions

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