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Sir Isaac Newton

Sir Isaac Newton was an influential English scientist born in 1642. He formulated the laws of motion and universal gravitation, laying the foundations for classical mechanics. Newton published his work Principia Mathematica in 1687, which described universal gravitation and the three laws of motion. This work dominated the scientific view until the 20th century development of Einstein's theory of relativity. Newton made seminal contributions to optics and mathematics, and held positions at the University of Cambridge and as president of the Royal Society. He was considered one of the most influential scientists in history.

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0% found this document useful (0 votes)
48 views7 pages

Sir Isaac Newton

Sir Isaac Newton was an influential English scientist born in 1642. He formulated the laws of motion and universal gravitation, laying the foundations for classical mechanics. Newton published his work Principia Mathematica in 1687, which described universal gravitation and the three laws of motion. This work dominated the scientific view until the 20th century development of Einstein's theory of relativity. Newton made seminal contributions to optics and mathematics, and held positions at the University of Cambridge and as president of the Royal Society. He was considered one of the most influential scientists in history.

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Isaac Newton

Sir Isaac Newton PRS (25 December 1642 – 20 March 1726/27[a]) was an English


mathematician, physicist, astronomer, theologian, and author (described in his own day as a
"natural philosopher") who is widely recognised as one of the most influential scientists of all
time and as a key figure in the scientific revolution. His book Philosophiæ Naturalis Principia
Mathematica (Mathematical Principles of Natural Philosophy), first published in 1687, laid the
foundations of classical mechanics. Newton also made seminal contributions to optics, and
shares credit with Gottfried Wilhelm Leibniz for developing the infinitesimal calculus.
In Principia, Newton formulated the laws of motion and universal gravitation that formed the
dominant scientific viewpoint until it was superseded by the theory of relativity. Newton used
his mathematical description of gravity to prove 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. 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 later confirmed by the geodetic
measurements of Maupertuis, La Condamine, and others, convincing most European
scientists of the superiority of Newtonian mechanics over earlier systems.
Newton built the first practical reflecting telescope and developed a sophisticated theory of
colour based on the observation that a prism separates white light into the colours of
the visible spectrum. His work on light was collected in his highly influential book Opticks,
published in 1704. He also formulated an empirical law of cooling, made the first theoretical
calculation of the speed of sound, and introduced the notion of a Newtonian fluid. In addition
to his work on calculus, as a mathematician Newton contributed to the study of power series,
generalised the binomial theorem to non-integer exponents, developed a method for
approximating the roots of a function, and classified most of the cubic plane curves.
Newton was a fellow of Trinity College and the second Lucasian Professor of Mathematics at
the University of Cambridge. He was a devout but unorthodox Christian who privately
rejected the doctrine of the Trinity. Unusually for a member of the Cambridge faculty of the
day, he refused to take holy orders in the Church of England. Beyond his work on the
mathematical sciences, Newton dedicated much of his time to the study
of alchemy and biblical chronology, but most of his work in those areas remained
unpublished until long after his death. Politically and personally tied to the Whig party,
Newton served two brief terms as Member of Parliament for the University of Cambridge, in
1689–90 and 1701–02. He was knighted by Queen Anne in 1705 and spent the last three
decades of his life in London, serving as Warden (1696–1700) and Master (1700–1727) of
the Royal Mint, as well as president of the Royal Society (1703–1727).

Isaac Newton

PRS
Portrait of Newton at 46 by Godfrey Kneller, 1689

Born 4 January 1643 [O.S. 25 December 1642][a]

Woolsthorpe-by-Colsterworth, Lincolnshire, E

ngland

Died 31 March 1727 (aged 84) [O.S. 20 March

1726][a]

Kensington, Middlesex, Great Britain

Resting place Westminster Abbey

Nationality English

Education Trinity College, Cambridge (M.A., 1668)[3]

Newtonian mechanics
Known for
Universal gravitation

Calculus

Newton's laws of motion

Optics

Binomial series

Principia
Newton's method

Awards FRS (1672)[4]

Knight Bachelor (1705)

Scientific career

Fields Physics

Natural philosophy

Alchemy

Theology

Mathematics

Astronomy

Economics

Institutions University of Cambridge

Royal Society

Royal Mint

Academic Isaac Barrow[5]

advisors
Benjamin Pulleyn[6][7]

Notable Roger Cotes

students
William Whiston

Signature

Coat of arms
Sir Isaac Newton PRS (25 December 1642 – 20 March 1726/27[a]) was an English
mathematician, physicist, astronomer, theologian, and author (described in his own day as a
"natural philosopher") who is widely recognised as one of the most influential scientists of all
time and as a key figure in the scientific revolution. His book Philosophiæ Naturalis Principia
Mathematica (Mathematical Principles of Natural Philosophy), first published in 1687, laid the
foundations of classical mechanics. Newton also made seminal contributions to optics, and
shares credit with Gottfried Wilhelm Leibniz for developing the infinitesimal calculus.
In Principia, Newton formulated the laws of motion and universal gravitation that formed the
dominant scientific viewpoint until it was superseded by the theory of relativity. Newton used
his mathematical description of gravity to prove 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. 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 later confirmed by the geodetic
measurements of Maupertuis, La Condamine, and others, convincing most European
scientists of the superiority of Newtonian mechanics over earlier systems.
Newton built the first practical reflecting telescope and developed a sophisticated theory of
colour based on the observation that a prism separates white light into the colours of
the visible spectrum. His work on light was collected in his highly influential book Opticks,
published in 1704. He also formulated an empirical law of cooling, made the first theoretical
calculation of the speed of sound, and introduced the notion of a Newtonian fluid. In addition
to his work on calculus, as a mathematician Newton contributed to the study of power series,
generalised the binomial theorem to non-integer exponents, developed a method for
approximating the roots of a function, and classified most of the cubic plane curves.
Newton was a fellow of Trinity College and the second Lucasian Professor of Mathematics at
the University of Cambridge. He was a devout but unorthodox Christian who privately
rejected the doctrine of the Trinity. Unusually for a member of the Cambridge faculty of the
day, he refused to take holy orders in the Church of England. Beyond his work on the
mathematical sciences, Newton dedicated much of his time to the study
of alchemy and biblical chronology, but most of his work in those areas remained
unpublished until long after his death. Politically and personally tied to the Whig party,
Newton served two brief terms as Member of Parliament for the University of Cambridge, in
1689–90 and 1701–02. He was knighted by Queen Anne in 1705 and spent the last three
decades of his life in London, serving as Warden (1696–1700) and Master (1700–1727) of
the Royal Mint, as well as president of the Royal Society (1703–1727).

Contents

 1Life
o 1.1Early life
o 1.2Middle years
 1.2.1Mathematics
 1.2.2Optics
 1.2.3Mechanics and gravitation
 1.2.4Classification of cubics
o 1.3Later life
o 1.4Death
o 1.5Personal relations
 2After death
o 2.1Fame
o 2.2Commemorations
 3Religious views
o 3.1Effect on religious thought
o 3.2Occult
o 3.3Alchemy
 4Enlightenment philosophers
 5Apple incident
 6Works
o 6.1Published in his lifetime
o 6.2Published posthumously
o 6.3Primary sources
 7See also
 8References
o 8.1Sources
 9Further reading
o 9.1Alchemy and non-scientific life
o 9.2Religion
o 9.3Science
 10External links
o 10.1Writings by Newton

Life
Early life
Main article: Early life of Isaac Newton
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