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The gravitational force (F) between two masses (m1 and m2) is given by: F = (G * m1 * m2) /r^2. Where r is the distance between the masses, and G is the gravitational constant, 6.67300 * 10^-11.

This means the larger the masses are, the more they pull toward each other. It also means that the closer they get, the stronger they pull.

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