SCIENTIFIC REVOLUTION 69
Sun, the perihelion of its orbit
would stay in the same place.
However all the planets in our solar
system affect each other, so the
perihelia precess (rotate) around
the Sun. Like all the other planets,
Mercury’s perihelion precesses,
but the precession cannot be
completely accounted for using
Newton’s equations. This was
recognized as a problem in 1859.
More than 50 years later, Einstein’s
Theory of General Relativity
described gravity as an effect of
the curvature of space-time, and
calculations based on this theory
do account for the observed
precession of Mercury’s orbit,
as well as other observations not
linked to Newton’s laws.
Newton’s laws today
Newton’s laws form the basis of
what is referred to as “classical
mechanics”—a set of equations
used to calculate the effects of
forces and motion. Although these
laws have been superseded by
equations based on Einstein’s
theories of relativity, the two sets
of laws agree as long as any motion
involved is small compared to
the speed of light. So for the
calculations involved in designing
airplanes or cars, or figuring out
how strong the components of
a skyscraper need to be, the
equations of classical mechanics
are both accurate enough and
much simpler to use. Newtonian
mechanics, while it may not strictly
be correct, is still widely used. ■
Nature and nature’s laws lay
hid in night; God said “Let
Newton be” and all was light.
Alexander Pope
Isaac Newton
Born on Christmas Day in
1642, Isaac Newton attended
school in Grantham, before
studying at Trinity College,
Cambridge, where he
graduated in 1665. During
his life, Newton was variously
Professor of Mathematics at
Cambridge, Master of the
Royal Mint, Member of
Parliament for Cambridge
University, and President of
the Royal Society. Besides
his dispute with Hooke,
Newton became involved
in a feud with German
mathematician Gottfried
Leibnitz over priority in the
development of calculus.
In addition to his
scientific work, Newton
spent much time in alchemical
investigations and Biblical
interpretation. A devout but
unorthodox Christian, he
successfully managed to
avoid being ordained as a
priest, which was normally
a requirement for some of
the offices he held.
Key works
1684 On the Motion of Bodies
in an Orbit
1687 Philosophiae Naturalis
Principia Mathematica
1704 Opticks
The precession (change in the
rotational axis) of the orbit of Mercury
was the first phenomenon that could
not be explained by Newton’s laws.