Newton, Isaac (1642–1727)
Newton organized our understanding of physical motion into three scientific laws, now known as Newton's laws of motion. Among other things, these laws explain the principle of rockets and how they are able to work in the vacuum of outer space. Newton's law of universal gravitation forms the basis of celestial mechanics and our understanding of the movement of satellites, both natural and artificial.
Newton was also the first to differentiate clearly between spherical aberration and chromatic aberration. Curiously, he held the view that all substances possessed the same dispersive power and that it was therefore impossible to eliminate or suppress chromatic aberration in any optical system consisting of lenses. While this conclusion no doubt delayed the invention of the achromatic lens, it had the compensatory effect of encouraging the development of the reflecting telescope, since mirrors were known to be inherently free of chromatic aberration. Newton himself was among the first to devise successful methods for casting mirrors and polishing them to the correct form. He produced his first reflector in 1668 – barely more than a toy, 16 cm (6 inches) long, with a mirror only 3.1 cm (just over an inch) in diameter.
Newton personally expressed almost no opinion on the question of whether life existed elsewhere in the universe, preferring to consider it a theological rather than a physical issue. In the second edition to the Principia he writes:
[I]f the fixed stars are the centres of other like systems, these, being formed by the like wise counsel, must be all subject to the dominion of the One.
Related entry• Newton's orbital cannon
Related categories• PHYSICISTS
• ASTRONOMERS AND ASTROPHYSICISTS
• GRAVITATIONAL PHYSICS
Home • About • Copyright © The Worlds of David Darling • Encyclopedia of Alternative Energy • Contact