Difference between revisions of "Isaac Newton"
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− | '''Isaac Newton''' ( | + | '''Isaac Newton''' (1643–1727) was a British [[mathematician]], physicist, and astronomer. He is widely regarded as one of the most influential scientists of all time, known for laying the groundwork for classical mechanics and for co-inventing [[calculus]]. |
− | == | + | == Early Life == |
− | + | Newton was born on January 4, 1643 (OS December 25, 1642) in Woolsthorpe, Lincolnshire, England. He was born prematurely and his father died before he was born. After early schooling in Grantham, he entered Trinity College, Cambridge in 1661. | |
− | + | During the Great Plague in 1665–1666, Newton returned home from Cambridge. While there, he made significant discoveries in mathematics, optics, and gravitation, a period often referred to as his ''annus mirabilis'' (year of wonders). | |
− | |||
− | == | + | == Work in Calculus == |
− | + | Newton developed a system of calculus—what he called the ''method of fluxions''—around 1665–1666. He used calculus techniques to analyze motion and change, though his notation differed significantly from modern standards. | |
− | + | German mathematician [[Gottfried Leibniz]] developed calculus independently and published his findings first. This led to a famous dispute over priority. Today, both men are credited with the independent development of calculus. | |
− | |||
− | |||
− | == | + | == Laws of Motion == |
− | + | Newton's most well-known contributions to [[physics]] are his three laws of motion, which he presented in the ''Principia Mathematica'' (1687): | |
− | |||
− | |||
+ | # An object remains at rest or in uniform motion unless acted on by a net external force. | ||
+ | # If an object has mass <math>m</math> and acceleration <math>a</math>, the net force acting on it is <math>F = ma</math>. | ||
+ | # For every action, there is an equal and opposite reaction. | ||
− | [[Category: | + | These laws form the foundation of classical mechanics. |
+ | |||
+ | == Universal Gravitation == | ||
+ | Newton also formulated the law of universal gravitation, which states that every pair of masses attracts each other with a force given by: | ||
+ | <cmath>F = G \frac{m_1 m_2}{r^2}</cmath> | ||
+ | where: | ||
+ | * <math>F</math> is the gravitational force, | ||
+ | * <math>m_1</math> and <math>m_2</math> are the masses, | ||
+ | * <math>r</math> is the distance between them, and | ||
+ | * <math>G</math> is the gravitational constant. | ||
+ | |||
+ | This law unified celestial and terrestrial mechanics and explained phenomena such as planetary orbits and tides. | ||
+ | |||
+ | == Work in Optics == | ||
+ | Newton studied the nature of light and color. He showed that white light is composed of different colors by passing it through a prism. He also built the first practical reflecting telescope, known today as the Newtonian telescope, to solve problems of chromatic aberration found in refracting telescopes. | ||
+ | |||
+ | == Later Life and Honors == | ||
+ | Newton served as Lucasian Professor of Mathematics at Cambridge from 1669 to 1702. He became President of the Royal Society in 1703 and was knighted by Queen Anne in 1705. He also worked at the Royal Mint, where he helped reform England's currency system. | ||
+ | |||
+ | He died in London in 1727 and was buried in Westminster Abbey. | ||
+ | |||
+ | == Legacy == | ||
+ | Newton's work remained the foundation of physics until the development of relativity and quantum mechanics in the 20th century. His influence spans fields from [[mathematics]] to astronomy and engineering. | ||
+ | |||
+ | == See Also == | ||
+ | * [[Calculus]] | ||
+ | * [[Physics]] | ||
+ | * [[Gottfried Leibniz]] | ||
+ | |||
+ | [[Category:Mathematicians]] |
Latest revision as of 20:01, 22 June 2025
Isaac Newton (1643–1727) was a British mathematician, physicist, and astronomer. He is widely regarded as one of the most influential scientists of all time, known for laying the groundwork for classical mechanics and for co-inventing calculus.
Contents
Early Life
Newton was born on January 4, 1643 (OS December 25, 1642) in Woolsthorpe, Lincolnshire, England. He was born prematurely and his father died before he was born. After early schooling in Grantham, he entered Trinity College, Cambridge in 1661.
During the Great Plague in 1665–1666, Newton returned home from Cambridge. While there, he made significant discoveries in mathematics, optics, and gravitation, a period often referred to as his annus mirabilis (year of wonders).
Work in Calculus
Newton developed a system of calculus—what he called the method of fluxions—around 1665–1666. He used calculus techniques to analyze motion and change, though his notation differed significantly from modern standards.
German mathematician Gottfried Leibniz developed calculus independently and published his findings first. This led to a famous dispute over priority. Today, both men are credited with the independent development of calculus.
Laws of Motion
Newton's most well-known contributions to physics are his three laws of motion, which he presented in the Principia Mathematica (1687):
- An object remains at rest or in uniform motion unless acted on by a net external force.
- If an object has mass
and acceleration
, the net force acting on it is
.
- For every action, there is an equal and opposite reaction.
These laws form the foundation of classical mechanics.
Universal Gravitation
Newton also formulated the law of universal gravitation, which states that every pair of masses attracts each other with a force given by:
where:
is the gravitational force,
and
are the masses,
is the distance between them, and
is the gravitational constant.
This law unified celestial and terrestrial mechanics and explained phenomena such as planetary orbits and tides.
Work in Optics
Newton studied the nature of light and color. He showed that white light is composed of different colors by passing it through a prism. He also built the first practical reflecting telescope, known today as the Newtonian telescope, to solve problems of chromatic aberration found in refracting telescopes.
Later Life and Honors
Newton served as Lucasian Professor of Mathematics at Cambridge from 1669 to 1702. He became President of the Royal Society in 1703 and was knighted by Queen Anne in 1705. He also worked at the Royal Mint, where he helped reform England's currency system.
He died in London in 1727 and was buried in Westminster Abbey.
Legacy
Newton's work remained the foundation of physics until the development of relativity and quantum mechanics in the 20th century. His influence spans fields from mathematics to astronomy and engineering.