Today, The Winsors & The Grandma have gone to the library to meet Isaac Newton and to borrow Philosophia Naturalis Principia Mathematica written by him.
They want to know more things about this genius and about his studies that changed our science and our lives.
Before meeting Newton, fhe family has studied some English grammar with Present Simple vs. Present Continuous; they have finished their second reading, and they have talked about international and English measures.
Finally, they have talked about the history of La Torre del Rellotge (The Clock Tower) and its relationship with the metre, l'Avinguda Meridiana (the Greenwich meridian) and l'Avinguda del Paral·lel (the 41° 22′ 34″ terrestrial parallel).
Sir Isaac Newton (25 December 1642/4 January 1643-20 March 1726/27) 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formulated the laws of motion and universal gravitation that formed the dominant scientific viewpoint until it was superseded by the theory of relativity.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
was born, according to the Julian calendar, in use in England at the
time, on Christmas Day, 25 December 1642 (NS 4 January 1643) an hour or two after midnight, at Woolsthorpe Manor in Woolsthorpe-by-Colsterworth, a hamlet in the county of Lincolnshire.
From the age of about twelve until he was seventeen, Newton
was educated at The King's School, Grantham, which taught Latin and
Greek and probably imparted a significant foundation of mathematics.
In
June 1661, he was admitted to Trinity College, Cambridge, on the
recommendation of his uncle Rev William Ayscough, who had studied there.
At that time, the college's teachings were based on those of Aristotle, whom Newton supplemented with modern philosophers such as Descartes, and astronomers such as Galileo and Thomas Street, through whom he learned of Kepler's work. He set down in his notebook a series of Quaestiones
about mechanical philosophy as he found it. In 1665, he discovered the
generalised binomial theorem and began to develop a mathematical theory
that later became calculus.
Although he had been undistinguished as a Cambridge student, Newton's private studies at his home in Woolsthorpe over the subsequent two years saw the development of his theories on calculus, optics, and the law of gravitation.
His
studies had impressed the Lucasian professor Isaac Barrow, who was more
anxious to develop his own religious and administrative potential, he
became master of Trinity two years later; in 1669 Newton succeeded him, only one year after receiving his MA. He was elected a Fellow of the Royal Society (FRS) in 1672.
Newton's work has been said to distinctly advance every branch of mathematics then studied.
His work on the subject usually referred to as fluxions or calculus,
seen in a manuscript of October 1666, is now published among Newton's mathematical papers.
Newton is generally credited with the generalised binomial theorem, valid for any exponent. He discovered Newton's identities, Newton's method,
classified cubic plane curves, polynomials of degree three in two
variables, made substantial contributions to the theory of finite
differences, and was the first to use fractional indices and to employ
coordinate geometry to derive solutions to Diophantine equations. He
approximated partial sums of the harmonic series by logarithms, a precursor to Euler's summation formula, and was the first to use power series with confidence and to revert power series. Newton's work on infinite series was inspired by Simon Stevin's decimals.
In 1666, Newton observed that the spectrum of colours
exiting a prism in the position of minimum deviation is oblong, even
when the light ray entering the prism is circular, which is to say, the
prism refracts different colours by different angles. This led him to
conclude that colour is a property intrinsic to light -a point which had
been debated in prior years.
From 1670 to 1672, Newton lectured on optics. During this period he investigated the refraction of light,
demonstrating that the multicoloured spectrum produced by a prism could
be recomposed into white light by a lens and a second prism. Modern
scholarship has revealed that Newton's analysis and resynthesis of white light owes a debt to corpuscular alchemy.
He
showed that coloured light does not change its properties by separating
out a coloured beam and shining it on various objects and that
regardless of whether reflected, scattered, or transmitted, the light
remains the same colour. Thus, he observed that colour is the result of
objects interacting with already-coloured light rather than objects
generating the colour themselves. This is known as Newton's theory of colour.
In his Hypothesis of Light of 1675, Newton posited the existence of the ether to transmit forces between particles. The contact with the Cambridge Platonist philosopher Henry More revived his interest in alchemy.
In 1679, Newton returned to his work on celestial mechanics by considering gravitation and its effect on the orbits of planets with reference to Kepler's laws of planetary motion.
In 1704, Newton published Opticks, in which he expounded his corpuscular theory of light.
The Principia was published on 5 July 1687 with encouragement and financial help from Edmond Halley. In this work, Newton stated the three universal laws of motion.
Together, these laws describe the relationship between any object, the
forces acting upon it and the resulting motion, laying the foundation
for classical mechanics.
They contributed to many advances during the Industrial Revolution which
soon followed and were not improved upon for more than 200 years. Many
of these advancements continue to be the underpinnings of
non-relativistic technologies in the modern world. He used the Latin
word gravitas (weight) for the effect that would become known as gravity, and defined the law of universal gravitation.
In the same work, Newton presented a calculus-like method of geometrical analysis using first and last ratios, gave the first analytical determination (based on Boyle's law)
of the speed of sound in air, inferred the oblateness of Earth's
spheroidal figure, accounted for the precession of the equinoxes as a
result of the Moon's gravitational attraction on the Earth's oblateness,
initiated the gravitational study of the irregularities in the motion of the Moon, provided a theory for the determination of the orbits of comets, and much more.
Newton made clear his heliocentric view of the Solar System -developed in a somewhat modern way because already in the mid-1680s he recognised the deviation of the Sun from the centre of gravity of the Solar System. For Newton, it was not precisely the centre of the Sun or any other body that could be considered at rest, but rather the common centre of gravity of the Earth, the Sun and all the Planets is to be esteem'd the Centre of the World, and this centre of gravity either is at rest or moves uniformly forward in a right line. Newton adopted the at rest alternative in view of common consent that the centre, wherever it was, was at rest.
Newton's postulate of an invisible force able to act over vast distances led to him being criticised for introducing occult agencies into science. Later, in the second edition of the Principia (1713), Newton firmly rejected such criticisms in a concluding General Scholium, writing that it was enough that the phenomena implied a gravitational attraction,
as they did; but they did not so far indicate its cause, and it was
both unnecessary and improper to frame hypotheses of things that were
not implied by the phenomena.
Newton died in his sleep in London on 20 March 1727 (OS 20 March 1726; NS 31 March 1727). His body was buried in Westminster Abbey.
Voltaire may have been present at his funeral. A bachelor, he had
divested much of his estate to relatives during his last years, and died
intestate. His papers went to John Conduitt and Catherine Barton.
After his death, Newton's
hair was examined and found to contain mercury, probably resulting from
his alchemical pursuits. Mercury poisoning could explain Newton's eccentricity in late life.
If I have seen further it is by standing
on the shoulders of giants.
Isaac Newton
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