In 1687 Sir Isaac Newton first published his *Philosophiae Naturalis Principia
Mathematica* (Mathematical Principles of Natural Philosophy) which was a
radical treatment of mechanics, establishing the concepts which were to dominate
physics for the next two hundred years. Among the book's most important new
concepts was Newton's Universal Law of Gravitation. Newton managed to take
Kepler's Laws governing the motion of the planets and Galileo's ideas about
kinematics and projectile
motion
and synthesize them into a law which governed both motion on earth and motion in
the heavens. This was an achievement of enormous importance for physics;
Newton's discoveries meant that the universe was a rational place in which the
same principles of nature applied to all objects.

The Universal Law of Gravitation has several important features. First, it
is an inverse square law, meaning that the strength of the force between two
massive objects decreases in proportion to the square of the distance between
them as they move farther apart. Second, the direction in which the force acts
is always along the line (or vector) connecting the two gravitating objects.
Moreover, because there is no "negative mass," gravity is always an attractive
force. It is also noteworthy that gravity is a relatively weak force. Modern
physicists consider there to be four fundamental forces in nature (the Strong
and Weak Nuclear forces, the Electromagnetic force and gravity), of which
gravity is the weakest. This means that gravity is only significant when very
large masses are being considered.

In this chapter we will also consider how the gravitational
constant) *G* is determined and
how Newton's Theorem
can simplify the calculation).