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Gravitational force is a natural phenomenon that describes the attractive force between two objects with mass. It is responsible for keeping planets in orbit around the sun and objects on Earth from floating away into space.
The gravitational force between two objects can be calculated using the equation F = G (m1m2)/r^2, where G is the gravitational constant, m1 and m2 are the masses of the two objects, and r is the distance between them.
The unit of measurement for gravitational force is Newtons (N). This unit is named after Sir Isaac Newton, who first described the theory of gravity.
An example of gravitational force is the force that keeps the moon in orbit around the Earth. The Earth's gravitational pull on the moon keeps it in a constant circular path around the Earth.
According to the equation F = G (m1m2)/r^2, the force of gravity decreases as the distance between two objects increases. This means that the farther apart two objects are, the weaker their gravitational force will be.