EQUATION

 

$F=\frac{G{m}_1{m}_2}{r^2}$ $F=\frac{k{q}_1{q}_2}{d^2}$ $Fd=\frac{k{q}_1{q}_2}{d^2}$ $h=mst$tm3$$ R=\sqrt{a^2+b^2+2abcos\theta }$$

Newton's Law of Gravitation

The force of attraction between two point masses, according to Newton's law of gravitation, is given by the following equation:

\( F = \frac{G \cdot m_1 \cdot m_2}{r^2} \)

Where:

• F = Gravitational force between the two masses
• G = Universal gravitational constant
• m₁ = Mass of the first object
• m₂ = Mass of the second object
• r = Distance between the centers of the two masses