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Newton's Law of Universal Gravitation is expressed by the equation ( F = G \frac{m_1 m_2}{r^2} ), where ( F ) is the gravitational force between two masses, ( m_1 ) and ( m_2 ), ( r ) is the distance between the centers of the two masses, and ( G ) is the gravitational constant. This law states that every point mass attracts every other point mass with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

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