What is the Newton's law of universal gravitation? What is the formula? Learn with Kimavi in just one minute!

Newton's law of universal gravitation states that any two objects in the universe attract each other with a force of attraction that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

This law was first proposed by Sir Isaac Newton in 1687.

The strength of the gravitational force between two objects is controlled by a constant called the gravitational constant (k).

The gravitational force between two objects is a vector quantity and is always attractive.

The formula for Newton's law of universal gravitation is: F = G _ (m1 _ m2) / r^2, where F is the force of attraction, m1 and m2 are the masses of the two objects, G is the gravitational constant, and r is the distance between the two objects.

This law explains the behavior of objects in the solar system, as well as other astronomical phenomena.

It is also used to calculate the masses of stars and galaxies, and to study the structure and evolution of the universe.

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