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Tuesday, October 2, 2012

John Bardeen

 

James Watson

 

Sheldon Glashow

 

Dmitri Mendeleev

 

Emil Fischer

 

Monday, October 1, 2012

Murray Gell-Mann

 

Murray Gell-Mann was born on 15th September 1929, in New York City. He obtained his B.Sc. at Yale University in 1948, and his Ph.D. in 1951 at the Massachusetts Institute of Technology. In 1952 he became a member of the Institute for Advanced Study, during 1952-1953 he was instructor at the University of Chicago, from 1953 to 1954 he was Assistant Professor, in 1954 he was appointed Associate Professor for research on dispersion relations. In this period he developed the strangeness theory and the eightfold way theory. In 1956 he was appointed Professor, his research then turned more to the theory of weak interactions.

In 1959 Professor Gell-Mann was awarded the Dannie Heineman Prize of the American Physical Society. He is a Fellow of this society and a member of the National Academy of Sciences.

Murray Gell-Mann was in 1955 married to J. Margaret Dow; they have a daughter, Elizabeth, and a son, Nicholas.
From Nobel Lectures, Physics 1963-1970, Elsevier Publishing Company, Amsterdam, 1972
This autobiography/biography was written at the time of the award and first published in the book series Les Prix Nobel. It was later edited and republished in Nobel Lectures. To cite this document, always state the source as shown above.
Copyright © The Nobel Foundation 1969

Addendum, May 2007

Murray Gell-Mann is one of today's most prominent scientists. He is currently Distinguished Fellow at the Santa Fe Institute as well as the Robert Andrews Millikan Professor Emeritus at the California Institute of Technology, where he joined the faculty in 1955. In 1969 he received the Nobel Prize in Physics for his work on the theory of elementary particles. He is the author of The Quark and the Jaguar, published in 1994, in which his ideas on simplicity and complexity are presented to a general readership.
Among his contributions to Physics was the "eightfold way" scheme that brought order out of the chaos created by the discovery of some 100 kinds of particles in collisions involving atomic nuclei. Gell-Mann subsequently found that all of those particles, including the neutron and proton, are composed of fundamental building blocks that he named "quarks," with very unusual properties. That idea has since been fully confirmed by experiment. The quarks are permanently confined by forces coming from the exchange of "gluons." He and others later constructed the quantum field theory of quarks and gluons, called "quantum chromodynamics," which seems to account for all the nuclear particles and their strong interactions.
Professor Gell-Mann was a director of the J.D. and C.T. MacArthur Foundation from 1979–2002 and is a board member of the Wildlife Conservation Society. From 1974 to 1988, he was a Citizen Regent of the Smithsonian Institution. He belongs to the National Academy of Sciences, the American Academy of Arts and Sciences, the American Philosophical Society, and the Council on Foreign Relations; he is also a Foreign Member of the Royal Society of London. He was on the U.S. President's Science Advisory Committee from 1969 to 1972 and the President's Committee of Advisors on Science and Technology from 1994 to 2001.
In 1988 Professor Gell-Mann was listed on the United Nations Environmental Program's Roll of Honor for Environmental Achievement (The Global 500). He also shared the 1989 Ettore Majorana "Science for Peace" prize. Earlier, he was given the Ernest O. Lawrence Memorial Award of the Atomic Energy Commission, the Franklin Medal of the Franklin Institute, the Research Corporation Award, and the John J. Carty Medal of the National Academy of Sciences. In 2005 Gell-Mann was awarded the Albert Einstein Medal. He has received honorary degrees from many universities, including Yale, Columbia, the University of Chicago, Cambridge, and Oxford. In 1994 the University of Florida awarded him an honorary degree in Environmental Studies.
Gell-Mann's interests extend to historical linguistics, archeology, natural history, the psychology of creative thinking, and other subjects connected with biological and cultural evolution and with learning. Much of his recent research at the Santa Fe Institute has focused on the theory of complex adaptive systems, which brings many of those topics together. Currently Professor Gell-Mann is spearheading the Evolution of Human Languages Program at the Santa Fe Institute. Another focus of his work relates to simplicity, complexity, regularity, and randomness. He is also concerned with how knowledge and understanding are to be extracted from the welter of "information" that can now be transmitted and stored as a result of the digital revolution. Professor Gell-Mann lives in Santa Fe, New Mexico and he teaches from time to time at the University of New Mexico in Albuquerque.



Robert Koch

 

August Kekule

 

Albrecht von Haller

 

Carl Gauss (Karl Friedrich Gauss)

 

Christiaan Huygens

 

Marcello Malpighi



William Harvey



Arthur Eddington


Justus Liebig

Leonard Euler

Enrico Fermi

Francis Crick

Max Born

Joseph J. Thomson

Edwin Hubble

Pierre Simon de Laplace

Charles Lyell

William Herschel

Marie Curie

Max Planck

Ludwig Boltzmann

Comte de Buffon

Tycho Brahe


Andreas Vesalius


paul dirac


Ernest Rutherford

Erwin Schrodinger

Rudolf Virchow

Linus Pauling


Werner Heisenberg


Franz Boas


Claude Bernard


James Clerk Maxwell



He is a very happy man, and has improved much since the weather got moderate; he has great work with doors, locks, keys etc., and 'Show me how it doos' is never out of his mouth. He also investigates the hidden course of streams and bell-wires, the way the water gets from the pond through the wall and a pend or small bridge and down a drain ...
When James was eight years old his mother died. His parents plan that they would educate him at home until he was 13 years old, and that he would then be able to go the Edinburgh University, fell through. A 16 year old boy was hired to act as tutor but the arrangement was not a successful one and it was decided that James should attend the Edinburgh Academy.

James, together with his family, arrived at 31 Heriot Row, the house of Isabella Wedderburn his father's sister, on 18 November 1841. He attended Edinburgh Academy where he had the nickname 'Dafty'. P G Tait, although almost the same age, was one class below James. Tait, who would become a close school friend and friend for life, described Maxwell's school days [40]:-
At school he was at first regarded as shy and rather dull. he made no friendships and spent his occasional holidays in reading old ballads, drawing curious diagrams and making rude mechanical models. This absorption in such pursuits, totally unintelligible to his schoolfellows, who were then totally ignorant of mathematics, procured him a not very complimentary nickname. About the middle of his school career however he surprised his companions by suddenly becoming one of the most brilliant among them, gaining prizes and sometimes the highest prizes for scholarship, mathematics, and English verse.
In early 1846 at the age of 14, Maxwell wrote a paper on ovals. In this work he generalised the definition of an ellipse by defining the locus of a point where the sum of m times the distance from one fixed point plus n times the distance from a second fixed point is constant. If m = n = 1 then the curve is an ellipse. Maxwell also defined curves where there were more than two foci. This became his first paper On the description of oval curves, and those having a plurality of foci which was read to the Royal Society of Edinburgh on 6 April 1846. These ideas were not entirely new as Descartes had defined such curves before but the work was remarkable for a 14 year old.
Maxwell was not dux of the Edinburgh Academy, this honour going to Lewis Campbell who later became the professor of Greek at the University of St Andrews. Lewis Campbell was a close friend of Maxwell's and he wrote the biography [4] and its second edition [5]. These biographies make fascinating reading filled with personal memories.
At the age of 16, in November 1847, Maxwell entered the second Mathematics class taught by Kelland, the natural philosophy (physics) class taught by Forbes and the logic class taught by William Hamilton. Tait, also at the University of Edinburgh, later wrote in the Proceedings of the Royal Society of Edinburgh (1879-80) [6]:-
The winter of 1847 found us together in the classes of Forbes and Kelland, where he highly distinguished himself. With the former he was a particular favourite, being admitted to the free use of the class apparatus for original experiments. ... During this period he wrote two valuable papers which are published in our Transactions, on The Theory of Rolling Curves and The Equilibrium of Elastic Solids.
The University of Edinburgh still has a record of books that Maxwell borrowed to take home while an undergraduate. These include
Cauchy, Calcul Différentiel
Fourier, Théorie de la Chaleur
Monge, Géometrie Descriptive
Newton, Optics
Poisson, Mechanics
Taylor, Scientific Memoirs
Willis, Principles of Mechanism
Maxwell went to Peterhouse Cambridge in October 1850 but moved to Trinity where he believed that it was easier to obtain a fellowship. Again we quote Tait's article in the Proceedings of the Royal Society of Edinburgh (1879-80):-
... he brought to Cambridge in the autumn of 1850, a mass of knowledge which was really immense for so young a man, but in a state of disorder appalling to his methodical private tutor. Though the tutor was William Hopkins, the pupil to a great extent took his own way, and it may safely be said that no high wrangler of recent years ever entered the Senate-house more imperfectly trained to produce 'paying' work than did Clerk Maxwell. But by sheer strength of intellect, though with the very minimum of knowledge how to use it to advantage under the conditions of the Examination, he obtained the position of Second Wrangler, and was bracketed equal with the Senior Wrangler, in the higher ordeal of the Smith's Prizes.
Thomson [40] describes Maxwell's undergraduate days:-
... Scholars dined together at one table. This brought Maxwell into daily contact with the most intellectual set in the College, among whom were many who attained distinction in later life. These in spite of his shyness and some eccentricities recognised his exceptional powers. ... The impression of power which Maxwell produced on all he met was remarkable; it was often much more due to his personality than to what he said, for many found it difficult to follow him in his quick changes from one subject to another, his lively imagination started so many hares that before he had run one down he was off on another.
Maxwell obtained his fellowship and graduated with a degree in mathematics from Trinity College in 1854. The First Wrangler in that year was Edward Routh, who as well as being an excellent mathematician was a genius at mastering the cramming methods required to succeed in the Cambridge Tripos of that time. Maxwell remained at Cambridge where he took pupils, then was awarded a Fellowship by Trinity to continue work.
One of Maxwell's most important achievements was his extension and mathematical formulation of Michael Faraday's theories of electricity and magnetic lines of force. His paper On Faraday's lines of force was read to the Cambridge Philosophical Society in two parts, 1855 and 1856. Maxwell showed that a few relatively simple mathematical equations could express the behaviour of electric and magnetic fields and their interrelation.
However, in early 1856, Maxwell's father became ill and Maxwell wanted to be able to spend more time with him. He therefore tried to obtain an appointment in Scotland, applying for the post of Professor of Natural Philosophy at Marischal College in Aberdeen when Forbes told him it was vacant. Maxwell travelled to Edinburgh for the Easter vacation of 1856 to be with his father and the two went together to Glenlair. On 3 April his father died and, shortly after, Maxwell returned to Cambridge as he had planned. Before the end of April he learnt that he had been appointed to the chair at Marischal College.
In November 1856 Maxwell took up the appointment in Aberdeen. When the subject announced by St John's College Cambridge for the Adams Prize of 1857 was The Motion of Saturn's Rings Maxwell was immediately interested. Maxwell and Tait had thought about the problem of Saturn's rings in 1847 while still pupils at the Edinburgh Academy. Maxwell decided to compete for the prize and his research at Aberdeen in his first two years was taken up with this topic. He showed that stability could be achieved only if the rings consisted of numerous small solid particles, an explanation now confirmed by the Voyager spacecraft. In a letter to Lewis Campbell, written on 28 August 1857, while he was at Glenlair, Maxwell wrote:-
I have effected several breaches in the solid ring, and now am splash into the fluid one, amid a clash of symbols truly astounding. When I reappear it will be in the dusky ring, which is something like the siege of Sebastopol conducted from a forest of guns 100 miles one way, and 30,000 miles the other, and the shot never to stop, but go spinning away round a circle, radius 170,000 miles...
Maxwell's essay won him the Adams Prize and Airy wrote:-
It is one of the most remarkable applications of mathematics to physics that I have ever seen.
Maxwell became engaged to marry Katherine Mary Dewar in February 1858 and they married in June 1859. Despite the fact that he was now married to the daughter of the Principal of Marischal College, in 1860, when Marischal College and King's College combined, Maxwell, as the junior of the department, had to seek another post. His scientific work, however, had been proceeding with great success. Stokes had written to him on 7 November 1857:-
I have just received your papers on the dynamical top, etc., and the account of experiments on the perception of colour. The latter, which I missed seeing at the time when it was published, I have just read with great interest. The results afford most remarkable and important evidence in favour of the theory of three primary colour-perceptions, a theory which you, and you alone, as far as I know, have established on an exact numerical basis.
When the Chair of Natural Philosophy at Edinburgh became vacant in 1859, Forbes having moved to St Andrews, it seemed that fate had smiled on Maxwell to bring him back to his home town. He asked Faraday to act as a referee for him, in a letter written on 30 November 1859. Many of Maxwell's friends were also applicants for this post including Tait and Routh. Maxwell lost out to Tait despite his outstanding scientific achievements. When the Edinburgh paper, the Courant, reported the result it noted that:-
Professor Maxwell is already acknowledged to be one of the most remarkable men known to the scientific world.
The reason he was not appointed must have been those given by the paper when they wrote:-
... there is another quality which is desirable in a Professor in a University like ours and that is the power of oral exposition proceeding on the supposition of imperfect knowledge or even total ignorance on the part of pupils.
The claim that he was not the best person to teach poorly qualified pupils may have been a fair one but it is certainly not the case that he was a poor lecturer. Stokes wrote in 1854 that he had:-
... once been present when [Maxwell] was giving an account of his geometrical researches to the Cambridge Philosophical Society, on which occasion I was struck with the singularly lucid manner of his exposition.
Again Fleming, who had attended Maxwell's lectures, expressed similar thoughts [20]:-
Maxwell in short had too much learning and too much originality to be at his best in elementary teaching. For those however who could follow him his teaching was a delight.
In 1860 Maxwell was appointed to the vacant chair of Natural Philosophy at King's College in London. The six years that Maxwell spent in this post were the years when he did his most important experimental work. The duties of the post were more demanding than those at Aberdeen. Campbell writes in [4]:-
There were nine months of lecturing in the year, and evening lectures to artisans, etc., were recognised as a part of the Professor's duties.
In London, around 1862, Maxwell calculated that the speed of propagation of an electromagnetic field is approximately that of the speed of light. He proposed that the phenomenon of light is therefore an electromagnetic phenomenon. Maxwell wrote the truly remarkable words:-
We can scarcely avoid the conclusion that light consists in the transverse undulations of the same medium which is the cause of electric and magnetic phenomena.
Maxwell also continued work he had begun at Aberdeen, considering the kinetic theory of gases. By treating gases statistically in 1866 he formulated, independently of Ludwig Boltzmann, the Maxwell-Boltzmann kinetic theory of gases. This theory showed that temperatures and heat involved only molecular movement.
This theory meant a change from a concept of certainty, heat viewed as flowing from hot to cold, to one of statistics, molecules at high temperature have only a high probability of moving toward those at low temperature. Maxwell's approach did not reject the earlier studies of thermodynamics but used a better theory of the basis to explain the observations and experiments.
Maxwell left King's College, London in the spring of 1865 and returned to his Scottish estate Glenlair. He made periodic trips to Cambridge and, rather reluctantly, accepted an offer from Cambridge to be the first Cavendish Professor of Physics in 1871. He designed the Cavendish laboratory and helped set it up. The Laboratory was formally opened on 16 June 1874.
The four partial differential equations, now known as Maxwell's equations, first appeared in fully developed form in Electricity and Magnetism (1873). Most of this work was done by Maxwell at Glenlair during the period between holding his London post and his taking up the Cavendish chair. They are one of the great achievements of 19th-century mathematics.
One of the tasks which occupied much of Maxwell's time between 1874 and 1879 was his work editing Henry Cavendish's papers. Cavendish, see [14]:-
... published only two papers [and] left twenty packages of manuscript on mathematical and experimental electricity. ... Maxwell entered upon this work with the utmost enthusiasm: he saturated his mind with the scientific literature of Cavendish's period; he repeated many of his experiments, and copied out the manuscript with his own hand. ... The volume entitled The Electrical Researches of the Honourable Henry Cavendish was published in 1879, and is unequalled as a chapter in the history of electricity.
Fleming attended Maxwell's last lecture course at Cambridge. He writes [20]:-
During the last term in May 1879 Maxwell's health evidently began to fail, but he continued to give his lectures up to the end of the term. ... To have enjoyed even a brief personal acquaintance with Professor Maxwell and the privilege of his oral instruction was in itself a liberal education, nay more, it was an inspiration, because everything he said or did carried the unmistakable mark of a genius which compelled not only the highest admiration but the greatest reverence as well.
Maxwell returned with his wife, who was also ill, to Glenlair for the summer. His health continued to deteriorate and he suffered much pain although remained remarkably cheerful. On 8 October 1879 he returned with his wife to Cambridge but, by this time he could scarcely walk. One of the greatest scientists the world has known passed away on 5 November. His doctor, Dr Paget, said:-
No man ever met death more consciously or more calmly.

Michael Faraday




Michael Faraday, the third of four children of James Faraday (1761–1810) and his wife, Margaret Hastwell Faraday (1764–1838), was born in Newington Butts on 22nd September 1791. James Faraday and all his children belonged to the small Christian sect called in Scotland the Glasites after their founder, John Glas, and in England the Sandemanians, after Robert Sandeman, who had brought these religious views to the country. Faraday worked as a blacksmith with James Boyd, a Sandemanian ironmonger of Welbeck Street, London.
Faraday later recalled: "my education was of the most ordinary description, consisting of little more than the rudiments of reading, writing, and arithmetic at a common day-school. My hours out of school were passed at home and in the streets". In 1804 he became an errand boy, delivering among other things newspapers, for the bookseller George Riebau of 2 Blandford Street. In October 1805, at the age of fourteen, he was indentured for seven years to Riebau as an apprentice bookbinder. It was during this apprenticeship that he developed an interest in chemistry. Faraday wrote: "whilst an apprentice, I loved to read the scientific books which were under my hands." He later thanked Riebau for helping him in his education: "you kindly interested yourself in the progress I made in the knowledge of facts relating to the different theories in existence, readily permitting me to examine those books in your possession that were in any way related to the subjects occupying my attention." This included reading books by Jane Marcet (Conversations on Chemistry) and Isaac Watts (Improvement of the Mind).
In the spring of 1812, the year his apprenticeship ended, William Dance, a customer of Riebau's, gave Faraday tickets to attend four lectures to be delivered by the professor of chemistry at the Royal Institution, Humphry Davy. He later recalled: "Sir H. Davy proceeded to make a few observations on the connections of science with other parts of polished and social life. Here it would be impossible for me to follow him. I should merely injure and destroy the beautiful and sublime observations that fell from his lips. He spoke in the most energetic and luminous manner of the Advancement of the Arts and Sciences. Of the connection that had always existed between them and other parts of a Nation's economy. During the whole of these observations his delivery was easy, his diction elegant, his tone good and his sentiments sublime." After becoming interested in science, Faraday applied to Davy for a job. In 1813 Faraday became his temporary assistant and spent the next 18 months touring Europe while during Davy's investigations into his theory of volcanic action.
His biographer, Frank James, wrote: "Davy had obtained a special passport from Napoleon stipulating that he could be accompanied only by his wife and two others. With Jane Davy requiring a maid, Davy (claiming that his valet had suddenly withdrawn) asked Faraday to undertake the tasks of a valet, making a promise, never fulfilled, to find a valet once they were on the continent. Faraday reluctantly agreed but this was the source of considerable friction between him and Jane Davy, who regarded him as a servant. For eighteen months they toured France, Switzerland, Italy, and southern Germany visiting many chemical laboratories. They met, among others, André-Marie Ampère in Paris, Charles-Gaspard and Arthur-Auguste De La Rive in Geneva, and the aged Alessandro Volta in Italy. Davy demonstrated the elemental nature of iodine to the French and in Florence showed that diamond was composed of carbon using the burning-glass of the duke of Tuscany. They witnessed the end of Napoleon's empire but following Napoleon's escape from Elba for the hundred days Davy decided to cut short the tour and returned to England in the middle of April 1815."
Faraday was also inspired by the work of Joseph Priestley: "Dr. Priestley had that freedom of mind, and that independence of dogma and of preconceived notions, by which men are so often bowed down and carried forward from fallacy to fallacy, their eyes not being opened to see what that fallacy is. I am very anxious at this time to exhort you all, - as I trust you all are pursuers of science, - to attend to these things; for Dr Priestley made his great discoveries mainly in consequence of his having a mind which could be easily moved from what it had held to the reception of new thoughts and notions; and I will venture to say that all his discoveries followed from the facility with which he could leave a preconceived idea."
On 21 May 1821 Faraday was appointed acting superintendent of the house of the Royal Institution. The following month he married Sarah Barnard (1800–1879), daughter of the
Sandemanian silversmith Edward Barnard (1767–1855). From the evidence that has survived the Faradays's marriage appears to have been happy and she was very supportive of his work. Although they had no children, at least two nieces lived with them for extended periods, Margery Ann Reid (1815–1888) and Jane Barnard (1832–1911).
Humphry Davy gave Faraday a valuable scientific education and also introduced him to important scientists in Europe. One scientist, Henry Paul Harvey, commented: "Sir H. Davy's greatest discovery was Michael Faraday." After Davy retired in 1827, Faraday replaced him as professor of chemistry at the Royal Institution. Faraday began to publish details of his research including condensation of gases, optical deceptions and the isolation of benzene from gas oils.
Faraday's greatest contribution to science was in the field of electricity. In 1821 he began experimenting with electromagnetism and by demonstrating the conversion of electrical energy into motive force, invented the electric motor. In 1831 Faraday discovered the induction of electric currents and made the first dynamo. In 1837 he demonstrated that electrostatic force consists of a field of curved lines of force, and conceived a specific inductive capacity. This led to Faraday being able to develop his theories on light and gravitational systems.
Harper's Magazine published an article stating: "At no period of Michael Faraday's unmatched career was he interested in utility. He was absorbed in disentangling the riddles of the universe, at first chemical riddles, in later periods, physical riddles. As far as he cared, the question of utility was never raised. Any suspicion of utility would have restricted his restless curiosity. In the end, utility resulted, but it was never a criterion to which his ceaseless experimentation could be subjected." William Ewart Gladstone, the Chancellor of the Exchequer, once asked Michael Faraday about the practical worth of electricity. He said he did not know but "there is every probability that you will soon be able to tax it!"
Faraday told a friend: "I have never had any student or pupil under me to aid me with assistance; but have always prepared and made my experiments with my own hands, working and thinking at the same time. I do not think I could work in company, or think aloud, or explain my thoughts at the time. Sometimes I and my assistant have been in the Laboratory for hours & days together, he preparing some lecture apparatus or cleaning up, & scarcely a word has passed between us; - all this being a consequence of the solitary & isolated system of investigation; in contradistinction to that pursued by a Professor with his aids & pupils as in your Universities."
Faraday was very keen to educate the public on science. In one lecture he argued: "If the term education may be understood in so large a sense as to include all that belongs to the improvement of the mind, either by the acquisition of the knowledge of others or by increase of it through its own exertions, we learn by them what is the kind of education science offers to man. It teaches us to be neglectful of nothing - not to despise the small beginnings, for they precede of necessity all great things in the knowledge of science, either pure or applied."
Friedrich Von Raumer was one of those impressed by the lecturers of Faraday: "He (Michael Faraday) speaks with ease and freedom, but not with a gossipy, unequal tone, alternately inaudible and bawling, as some very learned professors do; he delivers himself with clearness, precision and ability. Moreover, he speaks his language in a manner which confirmed me in a secret suspicion that I had, that a number of Englishmen speak it very badly."
Jane Pollack wrote in the St. Paul's Magazine that Faraday was an outstanding speaker: "It was an irresistible eloquence which compelled attention and invited upon sympathy. There was a gleaming in his eyes which no painter could copy, and which no poet could describe. Their radiance seemed to send a strange light into the very heart of his congregation, and when he spoke, it was felt that the stir of his voice and the fervour of his words could belong only to the owner of those kindling eyes. His thought was rapid and made its way in new phrases. His enthusiasm seemed to carry him to the point of ecstasy when he expatiated on the beauties of Nature, and when he lifted the veil from her deep mysteries. His body then took motion from his mind; his hair streamed out from his head; his hands were full of nervous action; his light, lithe body seemed to quiver with its eager life. His audience took fire with him, and every face was flushed."
The physicist, John Tyndall, recalled: "Underneath his sweetness and gentleness was the heat of a volcano. He was a man of excitable and fiery nature; but through high self-discipline he had converted the fire into a central glow and motive power of life, instead of permitting it to waste itself in useless passion. Faraday was not slow to anger, but he completely ruled his own spirit, and thus, though he took no cities, he captivated all hearts."
Faraday became a close friend of Angela Burdett-Coutts. According to Edna Healey, the author of Lady Unknown: The Life of Angela Burdett-Coutts (1978): "In Michael Faraday she found a brilliant, searching mind combined with a simple child-like faith that matched her own. The greatest experimental genius of his time, the man who discovered the laws of electrolysis, of light and magnetism, he was at ease in her company. The blacksmith's son who hated the social scene, made exceptions for her... As their friendship grew, he would call on her after the Friday lectures at the Royal Institution, eventually persuading her to apply for membership of the Royal Society."
On 19th January, 1847, Faraday wrote to Miss Burdett-Coutts: "For twenty years I have devoted all my exertions and powers to the advancement of science in this Institution; and for the last ten years or more I have given up all professional business and a large income with it for the same purpose... Although I earnestly desire to see lady members received amongst us, as in former times, do not let anything I have said induce you to do what may be not quite agreeable to your own inclinations." In February 1847 she became a full member of the Royal Society.
Michael Faraday rejected the Presidency of the Royal Society. He told John Tyndall: "Tyndall... I must remain plain Michael Faraday to the last; and let me now tell you, that if accepted the honour which the Royal Society desires to confer upon me, I would not answer for the integrity of my intellect for a single year. On being offered the Presidency of the Royal Society."
The government recognized his contribution to science by granting him a pension and giving him a house in Hampton Court. However, Faraday was unwilling to use his scientific knowledge to help military action and in 1853 refused to help develop poison gases to be used in the Crimean War. Faraday was the author of several books including Experimental Researches in Electricity and Chemical History of the Candle.
In 1853 spiritualism and table-turning became fashionable. Faraday examined the phenomenon and came to the conclusion that table-turning was caused by a quasi-involuntary muscular action, and had nothing to do with supernatural agency. In a letter to The Times stating his results, Faraday concluded by saying that the educational system must be deficient since otherwise well-educated people would not believe in the phenomenon in the way they did.
His biographer, Frank James, has pointed out: "In 1856 Faraday started his last major research project. Following George Gabriel Stokes's work on fluorescence in the early 1850s, which showed that a ray of light could change its wavelength after passing through a solution of sulphate of quinine, Faraday tried to realize this change directly. To achieve this he passed light through beaten gold and later colloidal solutions of gold. The wavelength of light was larger than the size of the gold particles, and yet they still affected the light. He sought to explain this phenomenon but, as with his work on gravity, came to no firm conclusions. Faraday's last piece of experimental work in 1862 was to see if magnetism had any effect on line spectra."
Michael Faraday died at his home, The Green, Hampton Court, where he died on 25th August 1867. He was buried five days later in the Sandemanian plot in Highgate cemetery.
^ Main Article ^

(1) In 1813 Michael Faraday wrote about the lectures by Humphry Davy.

Sir H. Davy proceeded to make a few observations on the connections of science with other parts of polished and social life. Here it would be impossible for me to follow him. I should merely injure and destroy the beautiful and sublime observations that fell from his lips. He spoke in the most energetic and luminous manner of the Advancement of the Arts and Sciences. Of the connection that had always existed between them and other parts of a Nation's economy. During the whole of these observations his delivery was easy, his diction elegant, his tone good and his sentiments sublime.

(2) Humphry Davy, letter to the Royal Institution in 1813.

I have the honour to inform you that I have found a person who is desirous to occupy the situation in the Institution lately filled by William Payne. His name is Michael Faraday. He is a youth of twenty-two years of age. As far as I have been able to ascertain, he appears well fitted for the situation. His habits seem good, his disposition is active and cheerful, his manner intelligent. He is willing to engage himself on the same terms as those given to Mr. Payne at the time of quitting the Institution.

(3) Michael Faraday wrote a letter to Benjamin Abbott while paying a visit to Rome (11th June, 1813)

A lecturer should appear easy and collected, undaunted and unconcerned his thoughts about him and his mind clear and free for the contemplation and description of his subject. His action should not be hasty and violent but slow easy and natural consisting principally in changes of the posture of the body in order to avoid the air of stiffness or sameness that would otherwise be unavoidable.

(4) Michael Faraday wrote a letter to Benjamin Abbott while paying a visit to Rome (1st May, 1814)

The things (in Rome) would affect anyone, and that mind must be dull indeed that is not urged to think & think again on these astonishing remains of the Romans when they appear in sight at every corner. The two things here most striking are the Coliseum and St. Peter's, and one is not more worthy of the ancients than the other is of the moderns. The Coliseum is a mighty ruin & indeed so is Rome & so are the Romans, & it is almost impossible to conceive how the hardy warlike race which conquered the globe has degenerated into modern, effeminate, idle Italians. St. Peter's appears to have been erected on the plan of some fairy tale, for every luxury, every ornament and every embellishment & species of embellishment have been employed in its erection. Its size is mighty, it is mountainous, its architecture elegant, its materials costly.

(5) Michael Faraday, Address delivered at the Commemoration of the Centenary of the Birth of Dr Priestley (1833)

Dr. Priestley had that freedom of mind, and that independence of dogma and of preconceived notions, by which men are so often bowed down and carried forward from fallacy to fallacy, their eyes not being opened to see what that fallacy is. I am very anxious at this time to exhort you all, - as I trust you all are pursuers of science, - to attend to these things; for DR Priestley made his great discoveries mainly in consequence of his having a mind which could be easily moved from what it had held to the reception of new thoughts and notions; and I will venture to say that all his discoveries followed from the facility with which he could leave a preconceived idea.

(6) Friedrich Von Raumer, England in 1835 (1836)

He (Michael Faraday) speaks with ease and freedom, but not with a gossipy, unequal tone, alternately inaudible and bawling, as some very learned professors do; he delivers himself with clearness, precision and ability. Moreover, he speaks his language in a manner which confirmed me in a secret suspicion that I had, that a number of Englishmen speak it very badly.

(7) Charles Schoenbein, letter to Michael Faraday (4th April, 1840)

Please do not to overwork yourself and to manage a little your mental and physical forces, for your health and life are most precious to your friends in particular and to the scientific world at large. We cannot yet spare you and you must continue to be our leader for many years to come. You ought to listen a little to the entreaties of your friends and to grant to your mind and body some little rest. I am sure Mrs. Faraday will be of my opinion and confident she will not cease reminding you of it.

(8) Michael Faraday, letter to Charles Schoenbein (13th November, 1845)

At present I have scarcely a moment to spare for any thing but work. I happen to have discovered a direct relation between magnetism & light also electricity & light - and the field it opens is so large & I think rich that I naturally wish to look at it first. I actually have no time to tell you what the thing is - for I now see no one & do no thing but just work. My head became giddy & I have therefore come to this place (Brighton) but still I bring my work with me. When I can catch time I will tell you more.

(9) Michael Faraday, Observations On Mental Education, a lecture before the Royal Institution (6th May 1854)

I will simply express my strong belief, that that point of self-education which consists in teaching the mind to resist its desires and inclinations, until they are proved to be right, is the most important of all, not only in things of natural philosophy, but in every department of dally life.

(10) Michael Faraday, letter to C. Ransteed (16th December, 1857)

I have never had any student or pupil under me to aid me with assistance; but have always prepared and made my experiments with my own hands, working and thinking at the same time. I do not think I could work in company, or think aloud, or explain my thoughts at the time. Sometimes I and my assistant have been in the Laboratory for hours & days together, he preparing some lecture apparatus or cleaning up, & scarcely a word has passed between us; - all this being a consequence of the solitary & isolated system of investigation; in contradistinction to that pursued by a Professor with his aids & pupils as in your Universities.

(11) Michael Faraday, Science as a Branch of Education, lecture to the Royal Institution (11th June, 1858)

If the term education may be understood in so large a sense as to include all that belongs to the improvement of the mind, either by the acquisition of the knowledge of others or by increase of it through its own exertions, we learn by them what is the kind of education science offers to man. It teaches us to be neglectful of nothing - not to despise the small beginnings, for they precede of necessity all great things in the knowledge of science, either pure or applied.

(12) John Tyndall, Faraday as a Discoverer (1868)

Tyndall... I must remain plain Michael Faraday to the last; and let me now tell you, that if accepted the honour which the Royal Society desires to confer upon me, I would not answer for the integrity of my intellect for a single year. On being offered the Presidency of the Royal Society.

(13) Harper's Magazine, The Usefulness of Useless Knowledge (1939)

At no period of Michael Faraday's unmatched career was he interested in utility. He was absorbed in disentangling the riddles of the universe, at first chemical riddles, in later periods, physical riddles. As far as he cared, the question of utility was never raised. Any suspicion of utility would have restricted his restless curiosity. In the end, utility resulted, but it was never a criterion to which his ceaseless experimentation could be subjected.

(14) John Tyndall, Faraday as a Discoverer (1868)

Underneath his sweetness and gentleness was the heat of a volcano. He was a man of excitable and fiery nature; but through high self-discipline he had converted the fire into a central glow and motive power of life, instead of permitting it to waste itself in useless passion. Faraday was not slow to anger, but he completely ruled his own spirit, and thus, though he took no cities, he captivated all hearts.

(15) Jane Pollack, St. Paul's Magazine (1870)

It was an irresistible eloquence which compelled attention and invited upon sympathy. There was a gleaming in his eyes which no painter could copy, and which no poet could describe. Their radiance seemed to send a strange light into the very heart of his congregation, and when he spoke, it was felt that the stir of his voice and the fervour of his words could belong only to the owner of those kindling eyes. His thought was rapid and made its way in new phrases. His enthusiasm seemed to carry him to the point of ecstasy when he expatiated on the beauties of Nature, and when he lifted the veil from her deep mysteries. His body then took motion from his mind; his hair streamed out from his head; his hands were full of nervous action; his light, lithe body seemed to quiver with its eager life. His audience took fire with him, and every face was flushed.

nicolaus copernicus



Synopsis

Nicolaus Copernicus was born on February 19, 1473 in Torun, Poland. Circa 1508, Copernicus developed his own celestial model of a heliocentric planetary system. Around 1514, he shared his findings in the Commentariolus. His second book on the topic, De revolutionibus orbium coelestium, was banned by the Roman Catholic Church not long after his May 24, 1543 death in Frauenburg, Poland.

Early Education

Famed astronomer Nicolaus Copernicus (Mikolaj Kopernik, in German) came into the world on February 19, 1473. The fourth and youngest child born to Nicolaus Copernicus Sr. and Barbara Watzenrode, an affluent copper merchant family in Torun, Poland, Copernicus was technically born of German heritage—by the time he was born, Torun had ceded to Poland, rendering him a citizen under the Polish crown. German was Copernicus's first language, but some scholars believe that he spoke some Polish as well.
When Copernicus was 10 years old, his father passed away. His maternal uncle, Bishop of Varmia Lucas Watzenrode, generously assumed the paternal role, taking it upon himself to ensure that Copernicus received the best possible education.
In 1491, Copernicus entered the University of Cracow, where he studied painting and mathematics. Though he did not take astronomy classes at that time, he developed a growing interest in the cosmos, and started collecting books on the topic.
Upon graduating from Cracow in 1494, Copernicus returned to Torun, where he took a canon's position—arranged by his uncle—at Frombork's cathedral. Though the opportunity was only typically available to priests, Copernicus was able to hold onto the job for the rest of his life. It was a fortunate stroke for Copernicus: The canon's position afforded him the opportunity to fund the continuation of his studies for as long as he liked. Still, the job demanded much of his schedule; he was only able to pursue his academic interests intermittently, during his free time.
In 1496, Copernicus took leave and traveled to Italy, where he enrolled in a religious law program as the University of Bologna. There, he met astronomer Domenico Maria Novara—a fateful encounter, as the two began exchanging astronomical ideas and observations. Historian Edward Rosen described the relationship as follows: "In establishing close contact with Novara, Copernicus met, perhaps for the first time in his life, a mind that dared to challenge the authority of [Ptolemy] the most eminent ancient writer in his chosen fields of study." The friends were so enthralled in their intellectual exchange, they decided to become roommates.
In 1500, after completing his law studies in Bologna, Copernicus went on to study practical medicine at the University of Padua. He did not, however, stay long enough to earn a degree, since the two-year leave of absence from his canon position was nearing expiration. In 1503, Copernicus attended the University of Ferrara, where he prepared to take the canon law exam. After passing the test
on his first attempt, he hurried back home to Poland, where he resumed his position as canon and rejoined his uncle at a nearby Episcopal residence. Copernicus remained at the Lidzbark-Warminski residence for the next seven years, working and tending to his elderly, ailing uncle, and exploring astronomy whenever he could find the time.
In 1510,
Copernicus moved to a residence in the Frombork Cathedral Chapter in hopes of clearing additional time to study astronomy. He would live there as a canon for the duration of his life.

Heliocentric Solar System

Throughout the seven years he spent in Lidzbark-Warminski, Copernicus read several books on the subject of astronomy. Among the sources that Copernicus consulted was Regiomontus's Epitome of the Almagest, which presented an alternative to astrologist Claudius Ptolemy's model of the universe, and significantly influenced his research.
By 1508, Copernicus had begun developing his own celestial model, a heliocentric planetary system. Ptolemy had previously invented a geometric planetary model, which was inconsistent with Aristotle's idea that celestial bodies moved in a circular motion at different speeds around a fixed point, the earth. In an attempt to reconcile such inconsistencies, Copernicus's heliocentric solar system named the sun, rather than the earth, as the center of the solar system. Subsequently, Copernicus believed that the size of each planet's orbit depended on its distance from the sun.
Though his theory was viewed as revolutionary and met with some controversy, Copernicus was not the first astronomer to propose such a theory; centuries prior, in 270 B.C., ancient Greek astronomer Aristarchus of Samos had identified the sun as the solar system's central unit. Aristarchus's ideas were quickly dismissed, however, because Ptolemy's theories were far more eagerly accepted by the influential Roman Catholic Church, which adamantly supported the earth-based solar system theory. Still, Copernicus's heliocentric solar system proved to be more detailed and accurate than Aristarchus's, including a more efficient formula for calculating planetary positions throughout the year.
After moving to the Frombork Cathedral Chapter in the early 1500s, Copernicus further developed his heliocentric model, and went on to design and apply a complex mathematical system for proving his theory. In 1513, his dedication prompted him to build his own modest observatory so that he could view the planets in action at any given time.
Copernicus's observations did, at times, lead him to form inaccurate conclusions, including his assumption that planets' orbit occurred in perfect circles. As German astronomer Johannes Kepler would later prove in the 17th century, planetary orbits are actually elliptical in shape.

'Commentariolus' and Controversy

Around 1514, Copernicus completed a written work, Commentariolus (Latin for "Small Commentary"), a 40-page manuscript that he referred to as the "Sketch of Hypothesis Made by Nicolaus Copernicus on the Heavenly Motions." Commentariolus summarized Copernicus's heliocentric planetary system and strove to provide systematic proof—in the form of both astronomical observations and mathematical formulas—of the model.
The sketch set forth seven axioms, each describing an aspect of the heliocentric solar system: 1) Planets don't revolve around one fixed point; 2) the earth is at the center of the moon's orbit; 3) The sun is at the center of the universe, and all celestial bodies rotate around it; 4) The distance between the earth and sun is only a tiny fraction of stars' distance from the earth and sun; 5) Stars do not move, and if they appear to, it is only because the earth itself is moving; 6) Earth moves in a sphere around the sun,
causing the sun's yearly movement; and 7) Earth's orbit around the sun causes the planets to orbit in the opposite direction.
Commentariolus also went on to describe in detail Copernicus's assertion that a mere 34 circles could sufficiently illustrate planetary motion. Copernicus sent his manuscript to several friends and contemporaries, and while the manuscript received little to no response among his colleagues, a buzz began to build around Copernicus and his unconventional theories within two years of Commentariolus's release. Adding an air of mystery to Copernicus's growing reputation—and notoriety, for some—was his rejection to an invitation by the Lateran Council, which invited astronomers to provide advice in reforming the calendar.
Copernicus's written works, Commentariolus and, later, De revolutionibus orbium coelestium (Latin for "On the Revolutions of the Heavenly Spheres"), raised a fair share of controversy. Copernicus's critics claimed that he failed to solve the mystery of the parallax—the seeming displacement in the position of a celestial body, when viewed along varying lines of sight—and that his work lacked a sufficient explanation for why the earth orbits the sun.
In addition to drawing criticism from scholars, Copernicus's theories incensed the Roman Catholic Church; his model was considered heretical because it was contrary to the Church’s teachings. When De revolutionibus orbium coelestium was published in 1543, just before Copernicus's death, religious leader Martin Luther voiced his opposition to the heliocentric solar system model. His underling, Lutheran minister Andreas Osiander, quickly followed suit, saying of Copernicus, "This fool wants to turn the whole art of astronomy upside down."
Osiander even went so far as to write a disclaimer stating that the heliocentric system was a theory, not a fact, and add it to the book's preface, leading readers to assume that Copernicus himself had written it. By this time, Copernicus was ailing and unfit for the task of defending his work.
Ironically, Copernicus had dedicated De revolutionibus orbium coelestium to Pope Paul III. If his tribute to the pope was an attempt to cull the Catholic Church's softer reception, it was to no avail. The Church ultimately banned De revolutionibus posthumously, and the book remained on the list of forbidden reading material for nearly three centuries thereafter.

Death and Legacy

In May of 1543, mathematician and scholar Georg Joachim Rheticus presented Copernicus with a copy of a newly published De revolutionibus orbium coelestium. Suffering the aftermath of a recent stroke, Copernicus is said
to have been clutching the book when he died in his bed on May 24, 1543 in Frauenburg, Poland.
In the 17th century, when the ban on De revolutionibus orbium coelestium was lifted, Kepler revealed to the public that the preface had indeed been written by Osiander, not Copernicus. As Kepler worked on expanding upon and correcting the errors of Copernicus's heliocentric theory, Copernicus became a symbol of the brave scientist standing alone, defending his theories against the common beliefs of his time.

Johannes Kepler




Antoine Laurent Lavoisier

Galileo Galilei


Synopsis

Galileo Galilei (born on February 15, 1564) was an Italian scientist who supported Copernicanism, the idea that Earth orbits the sun. Galileo defended his views in Dialogue Concerning the Two Chief World Systems. For doing so, he was tried by the Roman Inquisition, was found "suspect of heresy" and spent the rest of his life under house arrest. His findings changed our world view for all time.

Profile

Galileo Galilei was born on February 15, 1564, in Pisa in the Duchy of Florence, Italy. He was the first of six children born to Vincenzo Galilei, a well-known musician and music theorist, and Giulia Ammannati. In 1574, the family moved to Florence, where Galileo started his formal education at the Camaldolese monastery in Vallombrosa.
In 1583, Galileo entered the University of Pisa to study medicine. Armed with high intelligence and talent, he soon became fascinated with many subjects, particularly mathematics and physics. While at Pisa, Galileo was exposed to the Aristotelian view of the world, then the leading scientific authority and the only one sanctioned by the Roman Catholic Church. At first, Galileo supported this view, like any other intellectual of his time, and was on track to be a university professor. However, due to financial difficulties, Galileo left the university in 1585 before earning his degree.
Galileo continued to study mathematics, supporting himself with minor teaching positions. During this time he began his two-decade study on objects in motion and published The Little Balance, describing the hydrostatic principles of weighing small quantities, which brought him some fame. This gained him a teaching post at the University of Pisa, in 1589. There Galileo conducted his fabled experiments with falling objects and produced his manuscript Du Motu (On Motion), a departure from Aristotelian views about motion and falling objects. Galileo developed an arrogance about his work, and his strident criticisms of
Aristotle left him isolated among his colleagues. In 1592, his contract with the University of Pisa was not renewed.
Galileo quickly found a new position at the University of Padua, teaching geometry, mechanics and astronomy. The appointment was fortunate, for his father had died in 1591, leaving Galileo entrusted with the care of his younger brother Michelagnolo. During his 18-year tenure at Padua, he gave entertaining lectures and attracted large crowds of followers, further increasing his fame and his sense of mission.
In 1600, Galileo met Marina Gamba, a Venetian woman, who bore him three children out of wedlock: daughters Virginia and Livia, and son Vincenzo. He never married Marina, possibly due to financial worries and possibly fearing his illegitimate children would threaten his social standing. He worried the two girls would never marry well, and when they were older, had them enter a convent. His son’s birth was eventually legitimized and he became a successful musician.
In 1604, Galileo published The Operations of the Geometrical and Military Compass, revealing his skills with experiments and practical technological applications. He also constructed a hydrostatic balance for measuring small objects. These developments brought him additional income and more recognition. That same year, Galileo refined his theories on motion and falling objects, and developed the universal law of acceleration,  


which all objects in the universe obeyed. Galileo began to express openly his support of the Copernican theory that the earth and planets revolved around the sun. This challenged the doctrine of Aristotle and the established order set by the Catholic Church.
In July 1609, Galileo learned about a simple telescope built by Dutch eyeglass makers, and he soon developed one of his own. In August, he demonstrated it to some Venetian merchants, who saw its value for spotting ships and gave Galileo salary to manufacture several of them. However, Galileo’s ambition pushed him to go further, and in the fall of 1609 he made the fateful decision to turn his telescope toward the heavens. In March 1610, he published a small booklet, The Starry Messenger, revealing his discoveries that the moon was not flat and smooth, but a sphere with mountains and craters. He found Venus had phases like the moon, proving it rotated around the sun. He also discovered Jupiter had revolving moons, which didn’t revolve around the earth.
Soon Galileo began mo
unting a body of evidence that supported Copernican theory and contradicted Aristotle and Church doctrine. In 1612, he published his Discourse on Bodies in Water, refuting the Aristotelian explanation of why objects float in water, saying that it wasn’t because of their flat shape, but instead the weight of the object in relation to the water it displaced. In 1613, he published his observations of sunspots, which further refuted Aristotelian doctrine that the sun was perfect. That same year, Galileo wrote a letter to a student to explain how Copernican theory did not contradict Biblical passages, stating that scripture was written from an earthly perspective and implied that science provided a different, more accurate perspective. The letter was made public and Church Inquisition consultants pronounced Copernican theory heretical. In 1616, Galileo was ordered not to “hold, teach, or defend in any manner” the Copernican theory regarding the motion of the earth. Galileo obeyed the order for seven years, partly to make life easier and partly because he was a devoted Catholic.
In 1623, a friend of Galileo, Cardinal Maffeo Barberini, was selected as Pope Urban VIII. He allowed Galileo to pursue his work on astronomy and even encouraged him to publish it, on condition it be objective and not advocate Copernican theory. In 1632, Galileo published the Dialogue Concerning the Two Chief World Systems, a discussion among three people: one who supports Copernicus' heliocentric theory of the universe, one who argues against it, and one who is impartial. Though
Galileo claimed Dialogues was neutral, it was clearly not. The advocate of Aristotelian belief comes across as the simpleton, getting caught in his own arguments.
Church reaction against the book was swift, and Galileo was summoned to Rome. The Inquisition proceedings lasted from September 1632 to July 1633. During most of this time, Galileo was treated with respect and never imprisoned. However, in a final attempt to break him, Galileo was threatened with torture,
and he finally admitted he had supported Copernican theory, but privately held that his statements were correct. He was convicted of heresy and spent his remaining years under house arrest. Though ordered not to have any visitors nor have any of his works printed outside of Italy, he ignored both. In 1634, a French translation of his study of forces and their effects on matter was published, and a year later, copies of the Dialogue were published in Holland. While under house arrest, Galileo wrote Two New Sciences, a summary of his life’s work on the science of motion and strength of materials. It was printed in Holland in 1638. By this time, he had become blind and in ill health. Galileo died on January 8, 1642, after suffering from a fever and heart palpitations.
But in time, the Church couldn’t deny the truth in science. In 1758, it lifted the ban on most works supporting Copernican theory, and by 1835 dropped its opposition to heliocentrism altogether. In the 20th century several popes acknowledged the great work of Galileo,and in 1992 Pope John Paul II expressed regret about how the Galileo affair was handled. Galileo’s contribution to our understanding of the universe was significant not only in his discoveries, but in the methods he developed and the use of mathematics to prove them. He played a major role in the scientific revolution and deserves the moniker of “The Father of Modern Science.”

Sigmund Freud