Sir Isaac Newton Essay Research Paper Isaac

Sir Isaac Newton Essay, Research Paper Isaac Newton Special thanks to the Microsoft Corporation for their contribution to our site. The following information came from Microsoft Encarta.

Sir Isaac Newton Essay, Research Paper

Isaac Newton

Special thanks to the Microsoft Corporation for their contribution to our site. The following

information came from Microsoft Encarta.

I INTRODUCTION

Newton, Sir Isaac (1642-1727), mathematician and physicist, one of the foremost scientific intellects of all

time. Born at Woolsthorpe, near Grantham in Lincolnshire, where he attended school, he entered

Cambridge University in 1661; he was elected a Fellow of Trinity College in 1667, and Lucasian Professor

of Mathematics in 1669. He remained at the university, lecturing in most years, until 1696. Of these

Cambridge years, in which Newton was at the height of his creative power, he singled out 1665-1666

(spent largely in Lincolnshire because of plague in Cambridge) as “the prime of my age for invention”.

During two to three years of intense mental effort he prepared Philosophiae Naturalis Principia

Mathematica (Mathematical Principles of Natural Philosophy) commonly known as the Principia,

although this was not published until 1687.

As a firm opponent of the attempt by King James II to make the universities into Catholic institutions,

Newton was elected Member of Parliament for the University of Cambridge to the Convention Parliament

of 1689, and sat again in 1701-1702. Meanwhile, in 1696 he had moved to London as Warden of the

Royal Mint. He became Master of the Mint in 1699, an office he retained to his death. He was elected a

Fellow of the Royal Society of London in 1671, and in 1703 he became President, being annually

re-elected for the rest of his life. His major work, Opticks, appeared the next year; he was knighted in

Cambridge in 1705.

As Newtonian science became increasingly accepted on the Continent, and especially after a general peace

was restored in 1714, following the War of the Spanish Succession, Newton became the most highly

esteemed natural philosopher in Europe. His last decades were passed in revising his major works,

polishing his studies of ancient history, and defending himself against critics, as well as carrying out his

official duties. Newton was modest, diffident, and a man of simple tastes. He was angered by criticism or

opposition, and harboured resentment; he was harsh towards enemies but generous to friends. In

government, and at the Royal Society, he proved an able administrator. He never married and lived

modestly, but was buried with great pomp in Westminster Abbey.

Newton has been regarded for almost 300 years as the founding examplar of modern physical science, his

achievements in experimental investigation being as innovative as those in mathematical research. With

equal, if not greater, energy and originality he also plunged into chemistry, the early history of Western

civilization, and theology; among his special studies was an investigation of the form and dimensions, as

described in the Bible, of Solomon’s Temple in Jerusalem.

II OPTICS

In 1664, while still a student, Newton read recent work on optics and light by the English physicists Robert

Boyle and Robert Hooke; he also studied both the mathematics and the physics of the French philosopher

and scientist Ren Descartes. He investigated the refraction of light by a glass prism; developing over a few

years a series of increasingly elaborate, refined, and exact experiments, Newton discovered measurable,

mathematical patterns in the phenomenon of colour. He found white light to be a mixture of infinitely varied

coloured rays (manifest in the rainbow and the spectrum), each ray definable by the angle through which it

is refracted on entering or leaving a given transparent medium. He correlated this notion with his study of

the interference colours of thin films (for example, of oil on water, or soap bubbles), using a simple

technique of extreme acuity to measure the thickness of such films. He held that light consisted of streams of

minute particles. From his experiments he could infer the magnitudes of the transparent “corpuscles” forming

the surfaces of bodies, which, according to their dimensions, so interacted with white light as to reflect,

selectively, the different observed colours of those surfaces.

The roots of these unconventional ideas were with Newton by about 1668; when first expressed (tersely

and partially) in public in 1672 and 1675, they provoked hostile criticism, mainly because colours were

thought to be modified forms of homogeneous white light. Doubts, and Newton’s rejoinders, were printed

in the learned journals. Notably, the scepticism of Christiaan Huygens and the failure of the French physicist

Edm Mariotte to duplicate Newton’s refraction experiments in 1681 set scientists on the Continent against

him for a generation. The publication of Opticks, largely written by 1692, was delayed by Newton until the

critics were dead. The book was still imperfect: the colours of diffraction defeated Newton. Nevertheless,

Opticks established itself, from about 1715, as a model of the interweaving of theory with quantitative

experimentation.

III MATHEMATICS

In mathematics too, early brilliance appeared in Newton’s student notes. He may have learnt geometry at

school, though he always spoke of himself as self-taught; certainly he advanced through studying the

writings of his compatriots William Oughtred and John Wallis, and of Descartes and the Dutch school.

Newton made contributions to all branches of mathematics then studied, but is especially famous for his

solutions to the contemporary problems in analytical geometry of drawing tangents to curves

(differentiation) and defining areas bounded by curves (integration). Not only did Newton discover that

these problems were inverse to each other, but he discovered general methods of resolving problems of

curvature, embraced in his “method of fluxions” and “inverse method of fluxions”, respectively equivalent to

Leibniz’s later differential and integral calculus. Newton used the term “fluxion” (from Latin meaning “flow”)

because he imagined a quantity “flowing” from one magnitude to another. Fluxions were expressed

algebraically, as Leibniz’s differentials were, but Newton made extensive use also (especially in the

Principia) of analogous geometrical arguments. Late in life, Newton expressed regret for the algebraic style

of recent mathematical progress, preferring the geometrical method of the Classical Greeks, which he

regarded as clearer and more rigorous.

Newton’s work on pure mathematics was virtually hidden from all but his correspondents until 1704, when

he published, with Opticks, a tract on the quadrature of curves (integration) and another on the

classification of the cubic curves. His Cambridge lectures, delivered from about 1673 to 1683, were

published in 1707.

A The Calculus Priority Dispute Newton had the essence of the methods of fluxions

by 1666. The first to become known, privately, to other mathematicians, in 1668, was his method of

integration by infinite series. In Paris in 1675 Gottfried Wilhelm Leibniz independently evolved the first ideas

of his differential calculus, outlined to Newton in 1677. Newton had already described some of his

mathematical discoveries to Leibniz, not including his method of fluxions. In 1684 Leibniz published his first

paper on calculus; a small group of mathematicians took up his ideas.

In the 1690s Newton’s friends proclaimed the priority of Newton’s methods of fluxions. Supporters of

Leibniz asserted that he had communicated the differential method to Newton, although Leibniz had claimed

no such thing. Newtonians then asserted, rightly, that Leibniz had seen papers of Newton’s during a London

visit in 1676; in reality, Leibniz had taken no notice of material on fluxions. A violent dispute sprang up, part

public, part private, extended by Leibniz to attacks on Newton’s theory of gravitation and his ideas about

God and creation; it was not ended even by Leibniz’s death in 1716. The dispute delayed the reception of

Newtonian science on the Continent, and dissuaded British mathematicians from sharing the researches of

Continental colleagues for a century.

IV MECHANICS AND GRAVITATION

According to the well-known story, it was on seeing an apple fall in his orchard at some time during 1665

or 1666 that Newton conceived that the same force governed the motion of the Moon and the apple. He

calculated the force needed to hold the Moon in its orbit, as compared with the force pulling an object to

the ground. He also calculated the centripetal force needed to hold a stone in a sling, and the relation

between the length of a pendulum and the time of its swing. These early explorations were not soon

exploited by Newton, though he studied astronomy and the problems of planetary motion.

Correspondence with Hooke (1679-1680) redirected Newton to the problem of the path of a body

subjected to a centrally directed force that varies as the inverse square of the distance; he determined it to

be an ellipse, so informing Edmond Halley in August 1684. Halley’s interest led Newton to demonstrate the

relationship afresh, to compose a brief tract on mechanics, and finally to write the Principia.

Book I of the Principia states the foundations of the science of mechanics, developing upon them the

mathematics of orbital motion round centres of force. Newton identified gravitation as the fundamental force

controlling the motions of the celestial bodies. He never found its cause. To contemporaries who found the

idea of attractions across empty space unintelligible, he conceded that they might prove to be caused by the

impacts of unseen particles.

Book II inaugurates the theory of fluids: Newton solves problems of fluids in movement and of motion

through fluids. From the density of air he calculated the speed of sound waves.

Book III shows the law of gravitation at work in the universe: Newton demonstrates it from the revolutions

of the six known planets, including the Earth, and their satellites. However, he could never quite perfect the

difficult theory of the Moon’s motion. Comets were shown to obey the same law; in later editions, Newton

added conjectures on the possibility of their return. He calculated the relative masses of heavenly bodies

from their gravitational forces, and the oblateness of Earth and Jupiter, already observed. He explained tidal

ebb and flow and the precession of the equinoxes from the forces exerted by the Sun and Moon. All this

was done by exact computation.

Newton’s work in mechanics was accepted at once in Britain, and universally after half a century. Since

then it has been ranked among humanity’s greatest achievements in abstract thought. It was extended and

perfected by others, notably Pierre Simon de Laplace, without changing its basis and it survived into the late

19th century before it began to show signs of failing. See Quantum Theory; Relativity.

V ALCHEMY AND CHEMISTRY

Newton left a mass of manuscripts on the subjects of alchemy and chemistry, then closely related topics.

Most of these were extracts from books, bibliographies, dictionaries, and so on, but a few are original. He

began intensive experimentation in 1669, continuing till he left Cambridge, seeking to unravel the meaning

that he hoped was hidden in alchemical obscurity and mysticism. He sought understanding of the nature and

structure of all matter, formed from the “solid, massy, hard, impenetrable, movable particles” that he

believed God had created. Most importantly in the “Queries” appended to “Opticks” and in the essay “On

the Nature of Acids” (1710), Newton published an incomplete theory of chemical force, concealing his

exploration of the alchemists, which became known a century after his death.

VI HISTORICAL AND CHRONOLOGICAL STUDIES

Newton owned more books on humanistic learning than on mathematics and science; all his life he studied

them deeply. His unpublished “classical scholia” explanatory notes intended for use in a future edition of

the Principia reveal his knowledge of pre-Socratic philosophy; he read the Fathers of the Church even

more deeply. Newton sought to reconcile Greek mythology and record with the Bible, considered the

prime authority on the early history of mankind. In his work on chronology he undertook to make Jewish

and pagan dates compatible, and to fix them absolutely from an astronomical argument about the earliest

constellation figures devised by the Greeks. He put the fall of Troy at 904 BC, about 500 years later than

other scholars; this was not well received.

VII RELIGIOUS CONVICTIONS AND PERSONALITY Newton

also wrote on Judaeo-Christian prophecy, whose decipherment was essential, he thought, to the

understanding of God. His book on the subject, which was reprinted well into the Victorian Age,

represented lifelong study. Its message was that Christianity went astray in the 4th century AD, when the

first Council of Nicaea propounded erroneous doctrines of the nature of Christ. The full extent of Newton’s

unorthodoxy was recognized only in the present century: but although a critic of accepted Trinitarian

dogmas and the Council of Nicaea, he possessed a deep religious sense, venerated the Bible and accepted

its account of creation. In late editions of his scientific works he expressed a strong sense of God’s

providential role in nature.

VIII PUBLICATIONS

Newton published an edition of Geographia generalis by the German geographer Varenius in 1672. His

own letters on optics appeared in print from 1672 to 1676. Then he published nothing until the Principia

(published in Latin in 1687; revised in 1713 and 1726; and translated into English in 1729). This was

followed by Opticks in 1704; a revised edition in Latin appeared in 1706. Posthumously published writings

include The Chronology of Ancient Kingdoms Amended (1728), The System of the World (1728), the

first draft of Book III of the Principia, and Observations upon the Prophecies of Daniel and the

Apocalypse of St John (1733).