Sir Isaac Newton (1642-1727)
An English mathematician, physicist, alchemist, and theologian.
The founder of contemporary physics and mathematical analysis,
as well as of the methodology of experimental sciences
(he formulated, among others, the four principles of scientific method).
He formulated the three celebrated laws of motion and derived the law
of universal gravitation, contributed to the development of optics and
spectral analysis (by splitting white light). He developed the
calculus (in parallel and independently of Leibniz) and laid the
foundations for the calculus of variations. His laws of motion
and the law of universal gravitation allowed him to explain
Kepler's laws of planetary motion, which
constituted an ultimate confirmation of the heliocentric system
of Copernicus. Newton was
involved in many disputes regarding the priority of scientific
discoveries. This was in part because he used to publish his discoveries
reluctantly and with considerable delay.
His fundamental works were, among others:
- 1669-1671:
- Designed and built the first reflecting telescope
(Newtonian telescope).
- 1687:
- His fundamental work "Philosophiae Naturalis
Principia Mathematica" ("Mathematical Principles of
Natural Philosophy"), has been published many years after the
discovery of most of the results described in it. The book included,
among others:
- The three
laws of motion, in more modern formulation:
- The First Law (the inertia principle): If no net force acts
on an object, then it will stay at rest, or in uniform motion
along a straight line.
- The Second Law (the principle of acceleration): F = m·a,
that is the change of motion (acceleration a) of an object is proportional
to the magnitude of the force (F) acting on it, and inversely proportional
to its mass (m).
- The Third Law (the principle of acion and reaction): To
each action corresponds and equal reaction in the opposite direction.
- The law of universal gravitation (which he derived
using Kepler's third law), expressed by:
- F = G·m1·m2 / r2,
where:
- G = 6.673·10-11 Nm2/kg2 -
the gravitational constant,
- F - the force of gravitational attraction,
- m1, m2 - the masses
of attracting bodies;
- r - the distance of centers of gravity of these bodies.
- An application of those laws to explanation of, among others,
the mechanism of tides, the details of the motion of the
Moon
(taking into account gravitational perturbations caused
by the Sun), the shape of the
Earth
(an ellipsoid flattened at the poles), precession of
Earth's
rotational axis, and the motion of planets and comets.
- 1704:
- Published the work "Opticks..."
("Optics..."), in which he summarized his discoveries
in the field of splitting white light with a prism (this led to
a subsequent creation of spectral analysis allowing, among others,
to determine the chemical composition of distant astronomical objects),
gave a detailed description of a corpuscular theory of light
and described optical phenomena in thin layers (among others,
the so-called "Newtonian rings").
More information on Newton can be found in his biography at the MacTutor: The Archive of the History of Mathematics site
in Scottland and Newtonia - a
large collection of information on Newton.
- Named after Newton were:
- a large crater (78 km diameter) on the near side of the
Moon
,
- one of the largest craters (287 km diameter) on
Mars
,
- asteroids 662 Newtonia and 8000 Isaac Newton.
Site maintained by "URANOS Group"
Comments, opinions:
kontakt@uranos.eu.org
Last update: 06.VIII.2001