Sir
Isaac Newton
Born: 4 Jan 1643 in Woolsthorpe, Lincolnshire,
England
Died: 31 March 1727 in London, England
Isaac Newton's life can be divided
into three quite distinct periods. The first is his boyhood
days from 1643 up to his appointment to a chair in 1669. The
second period from 1669 to 1687 was the highly productive
period in which he was Lucasian professor at Cambridge. The
third period (nearly as long as the other two combined) saw
Newton as a highly paid government official in London with
little further interest in mathematical research.
Isaac Newton was born in the manor
house of Woolsthorpe, near Grantham in Lincolnshire. Although
by the calendar in use at the time of his birth he was born
on Christmas Day 1642, we give the date of 4 January 1643
in this biography which is the "corrected" Gregorian
calendar date bringing it into line with our present calendar.
(The Gregorian calendar was not adopted in England until 1752.)
Isaac Newton came from a family of farmers but never knew
his father, also named Isaac Newton, who died in October 1642,
three months before his son was born. Although Isaac's father
owned property and animals which made him quite a wealthy
man, he was completely uneducated and could not sign his own
name.
Isaac's
mother Hannah Ayscough remarried Barnabas Smith the minister
of the church at North Witham, a nearby village, when Isaac
was two years old. The young child was then left in the care
of his grandmother Margery Ayscough at Woolsthorpe. Basically
treated as an orphan, Isaac did not have a happy childhood.
His grandfather James Ayscough was never mentioned by Isaac
in later life and the fact that James left nothing to Isaac
in his will, made when the boy was ten years old, suggests
that there was no love lost between the two. There is no doubt
that Isaac felt very bitter towards his mother and his step-father
Barnabas Smith. When examining his sins at age nineteen, Isaac
listed:-
Threatening my father and mother Smith
to burn them and the house over them.
Upon the death of his stepfather in
1653, Newton lived in an extended family consisting of his
mother, his grandmother, one half-brother, and two half-sisters.
From shortly after this time Isaac began attending the Free
Grammar School in Grantham. Although this was only five miles
from his home, Isaac lodged with the Clark family at Grantham.
However he seems to have shown little promise in academic
work. His school reports described him as 'idle' and 'inattentive'.
His mother, by now a lady of reasonable wealth and property,
thought that her eldest son was the right person to manage
her affairs and her estate. Isaac was taken away from school
but soon showed that he had no talent, or interest, in managing
an estate.
An uncle, William Ayscough, decided
that Isaac should prepare for entering university and, having
persuaded his mother that this was the right thing to do,
Isaac was allowed to return to the Free Grammar School in
Grantham in 1660 to complete his school education. This time
he lodged with Stokes, who was the headmaster of the school,
and it would appear that, despite suggestions that he had
previously shown no academic promise, Isaac must have convinced
some of those around him that he had academic promise. Some
evidence points to Stokes also persuading Isaac's mother to
let him enter university, so it is likely that Isaac had shown
more promise in his first spell at the school than the school
reports suggest. Another piece of evidence comes from Isaac's
list of sins referred to above. He lists one of his sins as:-
... setting my heart on money, learning,
and pleasure more than Thee ...
which tells us that Isaac must have
had a passion for learning.
We know nothing about what Isaac learnt
in preparation for university, but Stokes was an able man
and almost certainly gave Isaac private coaching and a good
grounding. There is no evidence that he learnt any mathematics,
but we cannot rule out Stokes introducing him to Euclid's
Elements which he was well capable of teaching (although there
is evidence mentioned below that Newton did not read Euclid
before 1663). Anecdotes abound about a mechanical ability
which Isaac displayed at the school and stories are told of
his skill in making models of machines, in particular of clocks
and windmills. However, when biographers seek information
about famous people there is always a tendency for people
to report what they think is expected of them, and these anecdotes
may simply be made up later by those who felt that the most
famous scientist in the world ought to have had these skills
at school.
Newton entered his uncle's old College,
Trinity College Cambridge, on 5 June 1661. He was older than
most of his fellow students but, despite the fact that his
mother was financially well off, he entered as a sizar. A
sizar at Cambridge was a student who received an allowance
toward college expenses in exchange for acting as a servant
to other students. There is certainly some ambiguity in his
position as a sizar, for he seems to have associated with
"better class" students rather than other sizars.
Westfall (see [23] or [24]) has suggested that Newton may
have had Humphrey Babington, a distant relative who was a
Fellow of Trinity, as his patron. This reasonable explanation
would fit well with what is known and mean that his mother
did not subject him unnecessarily to hardship as some of his
biographers claim.
Newton's aim at Cambridge was a law
degree. Instruction at Cambridge was dominated by the philosophy
of Aristotle but some freedom of study was allowed in the
third year of the course. Newton studied the philosophy of
Descartes, Gassendi, Hobbes, and in particular Boyle. The
mechanics of the Copernican astronomy of Galileo attracted
him and he also studied Kepler's Optics. He recorded his thoughts
in a book which he entitled Quaestiones Quaedam Philosophicae
(Certain Philosophical Questions). It is a fascinating account
of how Newton's ideas were already forming around 1664. He
headed the text with a Latin statement meaning "Plato
is my friend, Aristotle is my friend, but my best friend is
truth" showing himself a free thinker from an early stage.
How Newton was introduced to the most
advanced mathematical texts of his day is slightly less clear.
According to de Moivre, Newton's interest in mathematics began
in the autumn of 1663 when he bought an astrology book at
a fair in Cambridge and found that he could not understand
the mathematics in it. Attempting to read a trigonometry book,
he found that he lacked knowledge of geometry and so decided
to read Barrow's edition of Euclid's Elements. The first few
results were so easy that he almost gave up but he:-
... changed his mind when he read that
parallelograms upon the same base and between the same parallels
are equal.
Returning to the beginning, Newton
read the whole book with a new respect. He then turned to
Oughtred's Clavis Mathematica and Descartes' La Géométrie.
The new algebra and analytical geometry of Viète was
read by Newton from Frans van Schooten's edition of Viète's
collected works published in 1646. Other major works of mathematics
which he studied around this time was the newly published
major work by van Schooten Geometria a Renato Des Cartes which
appeared in two volumes in 1659-1661. The book contained important
appendices by three of van Schooten disciples, Jan de Witt,
Johan Hudde, and Hendrick van Heuraet. Newton also studied
Wallis's Algebra and it appears that his first original mathematical
work came from his study of this text. He read Wallis's method
for finding a square of equal area to a parabola and a hyperbola
which used indivisibles. Newton made notes on Wallis's treatment
of series but also devised his own proofs of the theorems
writing:-
Thus Wallis doth it, but it may be
done thus ...
It would be easy to think that Newton's
talent began to emerge on the arrival of Barrow to the Lucasian
chair at Cambridge in 1663 when he became a Fellow at Trinity
College. Certainly the date matches the beginnings of Newton's
deep mathematical studies. However, it would appear that the
1663 date is merely a coincidence and that it was only some
years later that Barrow recognised the mathematical genius
among his students.
Despite some evidence that his progress
had not been particularly good, Newton was elected a scholar
on 28 April 1664 and received his bachelor's degree in April
1665. It would appear that his scientific genius had still
not emerged, but it did so suddenly when the plague closed
the University in the summer of 1665 and he had to return
to Lincolnshire. There, in a period of less than two years,
while Newton was still under 25 years old, he began revolutionary
advances in mathematics, optics, physics, and astronomy.
While Newton remained at home he laid
the foundations for differential and integral calculus, several
years before its independent discovery by Leibniz. The 'method
of fluxions', as he termed it, was based on his crucial insight
that the integration of a function is merely the inverse procedure
to differentiating it. Taking differentiation as the basic
operation, Newton produced simple analytical methods that
unified many separate techniques previously developed to solve
apparently unrelated problems such as finding areas, tangents,
the lengths of curves and the maxima and minima of functions.
Newton's De Methodis Serierum et Fluxionum was written in
1671 but Newton failed to get it published and it did not
appear in print until John Colson produced an English translation
in 1736.
When the University of Cambridge reopened
after the plague in 1667, Newton put himself forward as a
candidate for a fellowship. In October he was elected to a
minor fellowship at Trinity College but, after being awarded
his Master's Degree, he was elected to a major fellowship
in July 1668 which allowed him to dine at the Fellows' Table.
In July 1669 Barrow tried to ensure that Newton's mathematical
achievements became known to the world. He sent Newton's text
De Analysi to Collins in London writing:-
[Newton] brought me the other day some
papers, wherein he set down methods of calculating the dimensions
of magnitudes like that of Mr Mercator concerning the hyperbola,
but very general; as also of resolving equations; which I
suppose will please you; and I shall send you them by the
next.
Collins corresponded with all the leading
mathematicians of the day so Barrow's action should have led
to quick recognition. Collins showed Brouncker, the President
of the Royal Society, Newton's results (with the author's
permission) but after this Newton requested that his manuscript
be returned. Collins could not give a detailed account but
de Sluze and Gregory learnt something of Newton's work through
Collins. Barrow resigned the Lucasian chair in 1669 to devote
himself to divinity, recommending that Newton (still only
27 years old) be appointed in his place. Shortly after this
Newton visited London and twice met with Collins but, as he
wrote to Gregory:-
... having no more acquaintance with
him I did not think it becoming to urge him to communicate
anything.
Newton's first work as Lucasian Professor
was on optics and this was the topic of his first lecture
course begun in January 1670. He had reached the conclusion
during the two plague years that white light is not a simple
entity. Every scientist since Aristotle had believed that
white light was a basic single entity, but the chromatic aberration
in a telescope lens convinced Newton otherwise. When he passed
a thin beam of sunlight through a glass prism Newton noted
the spectrum of colours that was formed.
He argued that white light is really
a mixture of many different types of rays which are refracted
at slightly different angles, and that each different type
of ray produces a different spectral colour. Newton was led
by this reasoning to the erroneous conclusion that telescopes
using refracting lenses would always suffer chromatic aberration.
He therefore proposed and constructed a reflecting telescope.
In 1672 Newton was elected a fellow
of the Royal Society after donating a reflecting telescope.
Also in 1672 Newton published his first scientific paper on
light and colour in the Philosophical Transactions of the
Royal Society. The paper was generally well received but Hooke
and Huygens objected to Newton's attempt to prove, by experiment
alone, that light consists of the motion of small particles
rather than waves. The reception that his publication received
did nothing to improve Newton's attitude to making his results
known to the world. He was always pulled in two directions,
there was something in his nature which wanted fame and recognition
yet another side of him feared criticism and the easiest way
to avoid being criticised was to publish nothing. Certainly
one could say that his reaction to criticism was irrational,
and certainly his aim to humiliate Hooke in public because
of his opinions was abnormal. However, perhaps because of
Newton's already high reputation, his corpuscular theory reigned
until the wave theory was revived in the 19th century.
Newton's
relations with Hooke deteriorated further when, in 1675, Hooke
claimed that Newton had stolen some of his optical results.
Although the two men made their peace with an exchange of
polite letters, Newton turned in on himself and away from
the Royal Society which he associated with Hooke as one of
its leaders. He delayed the publication of a full account
of his optical researches until after the death of Hooke in
1703. Newton's Opticks appeared in 1704. It dealt with the
theory of light and colour and with
investigations of the colours of thin sheets 'Newton's
rings' and diffraction
of light.
To explain some of his observations
he had to use a wave theory of light in conjunction with his
corpuscular theory.
Another argument, this time with the English Jesuits in Liège
over his theory of colour, led to a violent exchange of letters,
then in 1678 Newton appears to have suffered a nervous breakdown.
His mother died in the following year and he withdrew further
into his shell, mixing as little as possible with people for
a number of years.
Newton's greatest achievement was his
work in physics and celestial mechanics, which culminated
in the theory of universal gravitation. By 1666 Newton had
early versions of his three laws of motion. He had also discovered
the law giving the centrifugal force on a body moving uniformly
in a circular path. However he did not have a correct understanding
of the mechanics of circular motion.
Newton's novel idea of 1666 was to
imagine that the Earth's gravity influenced the Moon, counter-
balancing its centrifugal force. From his law of centrifugal
force and Kepler's third law of planetary motion, Newton deduced
the inverse-square law.
In 1679 Newton corresponded with Hooke
who had written to Newton claiming:-
... that the Attraction always is in
a duplicate proportion to the Distance from the Center Reciprocall
...
M Nauenberg writes an account of the
next events:-
After his 1679 correspondence with
Hooke, Newton, by his own account, found a proof that Kepler's
areal law was a consequence of centripetal forces, and he
also showed that if the orbital curve is an ellipse under
the action of central forces then the radial dependence of
the force is inverse square with the distance from the centre.
This discovery showed the physical
significance of Kepler's second law.
In 1684 Halley, tired of Hooke's boasting
[M Nauenberg]:-
... asked Newton what orbit a body
followed under an inverse square force, and Newton replied
immediately that it would be an ellipse. However in De Motu..
he only gave a proof of the converse theorem that if the orbit
is an ellipse the force is inverse square. The proof that
inverse square forces imply conic section orbits is sketched
in Cor. 1 to Prop. 13 in Book 1 of the second and third editions
of the Principia, but not in the first edition.
Halley persuaded Newton to write a
full treatment of his new physics and its application to astronomy.
Over a year later (1687) Newton published the Philosophiae
naturalis principia mathematica or Principia as it is always
known.
The Principia is recognised as the
greatest scientific book ever written. Newton analysed the
motion of bodies in resisting and non-resisting media under
the action of centripetal forces. The results were applied
to orbiting bodies, projectiles, pendulums, and free-fall
near the Earth. He further demonstrated that the planets were
attracted toward the Sun by a force varying as the inverse
square of the distance and generalised that all heavenly bodies
mutually attract one another.
Further generalisation led Newton to
the law of universal gravitation:-
... all matter attracts all other matter
with a force proportional to the product of their masses and
inversely proportional to the square of the distance between
them.
Newton explained a wide range of previously
unrelated phenomena: the eccentric orbits of comets, the tides
and their variations, the precession of the Earth's axis,
and motion of the Moon as perturbed by the gravity of the
Sun. This work made Newton an international leader in scientific
research. The Continental scientists certainly did not accept
the idea of action at a distance and continued to believe
in Descartes' vortex theory where forces work through contact.
However this did not stop the universal admiration for Newton's
technical expertise.
James II became king of Great Britain
on 6 February 1685. He had become a convert to the Roman Catholic
church in 1669 but when he came to the throne he had strong
support from Anglicans as well as Catholics. However rebellions
arose, which James put down but he began to distrust Protestants
and began to appoint Roman Catholic officers to the army.
He then went further, appointing only Catholics as judges
and officers of state. Whenever a position at Oxford or Cambridge
became vacant, the king appointed a Roman Catholic to fill
it. Newton was a staunch Protestant and strongly opposed to
what he saw as an attack on the University of Cambridge.
When the King tried to insist that
a Benedictine monk be given a degree without taking any examinations
or swearing the required oaths, Newton wrote to the Vice-Chancellor:-
Be courageous and steady to the Laws
and you cannot fail.
The Vice-Chancellor took Newton's advice
and was dismissed from his post. However Newton continued
to argue the case strongly preparing documents to be used
by the University in its defence. However William of Orange
had been invited by many leaders to bring an army to England
to defeat James. William landed in November 1688 and James,
finding that Protestants had left his army, fled to France.
The University of Cambridge elected Newton, now famous for
his strong defence of the university, as one of their two
members to the Convention Parliament on 15 January 1689. This
Parliament declared that James had abdicated and in February
1689 offered the crown to William and Mary. Newton was at
the height of his standing - seen as a leader of the university
and one of the most eminent mathematicians in the world. However,
his election to Parliament may have been the event which let
him see that there was a life in London which might appeal
to him more than the academic world in Cambridge.
After suffering a second nervous breakdown
in 1693, Newton retired from research. The reasons for this
breakdown have been discussed by his biographers and many
theories have been proposed: chemical poisoning as a result
of his alchemy experiments; frustration with his researches;
the ending of a personal friendship with Fatio de Duillier,
a Swiss-born mathematician resident in London; and problems
resulting from his religious beliefs. Newton himself blamed
lack of sleep but this was almost certainly a symptom of the
illness rather than the cause of it. There seems little reason
to suppose that the illness was anything other than depression,
a mental illness he must have suffered from throughout most
of his life, perhaps made worse by some of the events we have
just listed.
Newton decided to leave Cambridge to
take up a government position in London becoming Warden of
the Royal Mint in 1696 and Master in 1699. However, he did
not resign his positions at Cambridge until 1701. As Master
of the Mint, adding the income from his estates, we see that
Newton became a very rich man. For many people a position
such as Master of the Mint would have been treated as simply
a reward for their scientific achievements. Newton did not
treat it as such and he made a strong contribution to the
work of the Mint. He led it through the difficult period of
recoinage and he was particularly active in measures to prevent
counterfeiting of the coinage.
In 1703 he was elected president of
the Royal Society and was re-elected each year until his death.
He was knighted in 1705 by Queen Anne, the first scientist
to be so honoured for his work. However the last portion of
his life was not an easy one, dominated in many ways with
the controversy with Leibniz over which had invented the calculus.
Given the rage that Newton had shown
throughout his life when criticised, it is not surprising
that he flew into an irrational temper directed against Leibniz.
We have given details of this controversy in Leibniz's biography
and refer the reader to that article for details. Perhaps
all that is worth relating here is how Newton used his position
as President of the Royal Society. In this capacity he appointed
an "impartial" committee to decide whether he or
Leibniz was the inventor of the calculus. He wrote the official
report of the committee (although of course it did not appear
under his name) which was published by the Royal Society,
and he then wrote a review (again anonymously) which appeared
in the Philosophical Transactions of the Royal Society.
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