
Isaac Newton
1642 – 1727 · aged 85
English mathematician and physicist (1642–1727)
- Born
- 1642 · Woolsthorpe Manor
- Died
- 1727 · Kensington
Life timeline
Their life from birth to death. On the timeline, world events of the time are shown faintly.
- 1642BornBorn in Woolsthorpe Manor
- 1669 – 1702RoleLucasian Professor of Mathematics
- 1689 – 1690RoleMember of the 1689-90 Parliament
- 1696 – 1700RoleWarden of the Mint
- 1700 – 1727RoleMaster of the Mint
- 1701 – 1702RoleMember of the 1701-02 Parliament
- 1703 – 1727RolePresident of the Royal Society
- 1705AwardKnight Bachelor
- 1727DiedDied in Kensington
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Meanwhile in the world
Major world events during their lifetime (1642 – 1727).
- 1642 – 1651English Civil War
Biography
Sir Isaac Newton (4 January 1643 [O.S. 25 December 1642] – 31 March 1727 [O.S. 20 March 1726]) was an English polymath who was a mathematician, physicist, astronomer, alchemist, theologian, historian and inventor. He was a key figure in the Scientific Revolution and the Enlightenment that followed. His book Philosophiæ Naturalis Principia Mathematica (Mathematical Principles of Natural Philosophy), first published in 1687, achieved the first great unification in physics and established classical mechanics. Newton also made seminal contributions to optics, and shares credit with the German mathematician Gottfried Wilhelm Leibniz for formulating infinitesimal calculus, although he developed calculus years before Leibniz. Newton contributed to and refined the scientific method, and his work is considered the most influential in bringing forth modern science.
In the Principia, Newton formulated the laws of motion and universal gravitation that formed the dominant scientific viewpoint for centuries until it was superseded by the theory of relativity. While this is the case, his laws still serve as sufficient approximations for all physical phenomena involving low speeds (much less than the speed of light) and weak gravitational fields. He used his mathematical description of gravity to derive Kepler's laws of planetary motion, account for tides, the trajectories of comets, the precession of the equinoxes and other phenomena, eradicating doubt about the Solar System's heliocentricity. Newton solved the two-body problem and introduced the three-body problem. He demonstrated that the motion of objects on Earth and celestial bodies could be accounted for by the same principles. Newton's inference that the Earth is an oblate spheroid was subsequently confirmed by the geodetic measurements of Pierre Louis Maupertuis, Alexis Clairaut, Charles Marie de La Condamine, and others, convincing most European scientists of the superiority of Newtonian mechanics over earlier systems. He was also the first to calculate the age of Earth by experiment, and described a precursor to the modern wind tunnel. Further, he was the first to provide a quantitative estimate of the solar mass.
Text from the Wikipedia article Isaac Newton, CC BY-SA 4.0
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