Newton observed an apple falling from a tree, which led him to discover his law of universal gravitation. The law states that every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. Specifically, the gravitational force between two objects equals G*(m1*m2)/r^2, where G is the gravitational constant, m1 and m2 are the object masses, and r is the distance between their centers. This explained gravity and allowed prediction of orbital motion.