The law of universal gravitation states that gravitational force between masses decreases with the distance between them, according to an inversesquare law. In addition, the theory notes that the greater an object's mass, the greater its gravitational force on another mass. Newton published his argument in Philosophiae Naturalis Principia Mathematica (1687). It is important to note that Newton was not "inventing" or "discovering" gravity; he was merely defining it mathematically. Newton would use universal gravitation, along with his laws of motion, to substantiate Kepler's laws of planetary motion. Newtonian gravitation can be derived from general relativity in the limit where the bodies are moving slowly with respect to the speed of light and the gravitational field is weak and unchanging with time. This would be a good example of the correspondence principle where the newer and more accurate or comprehensive theory breaks down to the previous theory in the domain where the previous theory is valid.

Every object in the Universe attracts every other object with a force directed along the line of centers for the two objects that is proportional to the product of their masses and inversely proportional to the square of the separation between the two objects. (See also inversesquare law.)
 Two bodies attract each other with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
Strictly speaking, this law applies only to pointlike objects. If the objects have spatial extent , the true force has to be found by integrating the forces between the various points.
The law expressed as an equation:
where:
Last updated: 05132005 07:56:04