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Galileo GalileiGalilei Galileo (1564-1642) an Italian physicist and astronomer, was greatly remembered for some very important contributions to astronomy and physics.  He was also known for his battle against the authorities for freedom of inquiry.  Early in his life, Galileo was taught by monks at Vallombrosa, and then entered the university of Pisa in 1581 to study medicine.  He soon turned to philosophy and mathematics and left the University without a degree in 1585. In 1589 he became professor of mathematics at Pisa.  He supposedly taught theories that contradicted Aristotle's theories, and in 1592 his contract was not renewed. The same year he was appointed the chair of mathematics at the University of Padua, which he remained at until 1610.  While at Padua, he invented a 'calculating compass' for solving mathematics problems.  In 1609 he heard that in Holland a spy glass had been invented, and he was inspired to create the first telescope, which was as powerful as a modern day field glass.  By December of the same year, he had built another telescop twenty times stronger than the first, which he was able to discovery craters on the moon with, stars in the milky way, and the four largest satellites of Jupiter. He had also observed the phases of Venus by this time.  After his great discoveries, he mainly stuck to writing books.  In 1613 he published a book about sunspots, 1624 a book called Dialogue on the Tides, which he discusses Ptolemaic and Copernican theories, in which he got himself reprimanded by the Inquisition of Rome. 

Jules Gabriel Verne was born in 1828, in Nates, France. Jules' parents were of a sefaring tradition, one factor which influenced his writings. As a boy, Jules Verne ran off to be a cabin boy on a merchant ship, but he was cought and returned to his parents. In 1847 Jules was sent to study law in Paris. While there, however, his passion for theatre grew. Later in 1850, Jules Verne's first play was published. His father was outraged when he heard that Jules was not going to continue law, so he disconinued the money he ws giving him to pay for his expenses in paris. This forced Verne to make money by selling his stories.

After spending many hours in Paris libraries studying geology, engeneering, and astronomy, Jules Verne published his first novel Five Weeks in a Balloon. Soon he started writing novels such as Journey to the Center of the Earth, From the Earth to the Moon, and 20,000 Leagues Under the Sea.

Because of the popularity of these and other novels, Jules Verne became a very rich man. In 1876, he bought a large yacht and sailed around Europe. The last novel befor Jules Verne's death was The Invasion of the Sea. Jules Verne died in the city of Amines in 1905.

Popular Books by Jules Verne

    1863 - Five Weeks in a Balloon
    1864 - A Journey to the Center of the Earth
    1866 - From the Earth to the Moon
    1870 - Twenty Thousand Leagues Under the Sea
    1873 - Around the World in Eighty Days
    1874 - Mysterious Island
    1904 - Master of the World

Newton's Life

In 1642, the year Galileo died, Isaac ewton was born in Woolsthorpe, Lincolnshire, England on Christmas Day. His father had died three months earlier, and baby Isaac, very premature, was also not expected to survive. It was said he could be fitted into a quart pot. When Isaac was three, his mother married a wealthy elderly clergyman from the next village, and went to live there, leaving Isaac behind with his grandmother. The clergyman died, and Isaac's mother came back, after eight years, bringing with her three small children. Two years later, Newton went away to the Grammar School in Grantham, where he lodged with the local apothecary, and was fascinated by the chemicals. The plan was that at age seventeen he would come home and look after the farm. He turned out to be a total failure as a farmer.

His mother's brother, a clergyman who had been an undergraduate at Cambridge, persuaded his mother that it would be better for Isaac to go to university, so in 1661 he went up to Trinity College, Cambridge. Isaac paid his way through college for the first three years by waiting tables and cleaning rooms for the fellows (faculty) and the wealthier students. In 1664, he was elected a scholar, guaranteeing four years of financial support. Unfortunately, at that time the plague was spreading across Europe, and reached Cambridge in the summer of 1665. The university closed, and Newton returned home, where he spent two years concentrating on problems in mathematics and physics. He wrote later that during this time he first understood the theory of gravitation, which we shall discuss below, and the theory of optics (he was the first to realize that white light is made up of the colors of the rainbow), and much mathematics, both integral and differential calculus and infinite series. However, he was always reluctant to publish anything, at least until it appeared someone else might get credit for what he had found earlier.

On returning to Cambridge in 1667, he began to work on alchemy, but then in 1668 Nicolas Mercator published a book containing some methods for dealing with infinite series. Newton immediately wrote a treatise, De Analysi, expounding his own wider ranging results. His friend and mentor Isaac Barrow communicated these discoveries to a London mathematician, but only after some weeks would Newton allow his name to be given. This brought his work to the attention of the mathematics community for the first time. Shortly afterwards, Barrow resigned his Lucasian Professorship (which had been established only in 1663, with Barrow the first incumbent) at Cambridge so that Newton could have the Chair.

Newton's first major public scientific achievement was the invention, design and construction of a reflecting telescope. He ground the mirror, built the tube, and even made his own tools for the job. This was a real advance in telescope technology, and ensured his election to membership in the Royal Society. The mirror gave a sharper image than was possible with a large lens because a lens focusses different colors at slightly different distances, an effect called chromatic aberration. This problem is minimized nowadays by using compound lenses, two lenses of different kinds of glass stuck together, that err in opposite directions, and thus tend to cancel each other's shortcomings, but mirrors are still used in large telescopes.

Later in the 1670's, Newton became very interested in theology. He studied Hebrew scholarship and ancient and modern theologians at great length, and became convinced that Christianity had departed from the original teachings of Christ. He felt unable to accept the current beliefs of the Church of England, which was unfortunate because he was required as a Fellow of Trinity College to take holy orders. Happily, the Church of England was more flexible than the Catholic Church in these matters, and King Charles II issued a royal decree excusing Newton from the necessity of taking holy orders! Actually, to prevent this being a wide precedent, the decree specified that, in perpetuity, the Lucasian professor need not take holy orders. (The current Lucasian professor is Stephen Hawking.)

In 1684, three members of the Royal Society, Sir Christopher Wren, Robert Hooke and Edmond Halley, argued as to whether the elliptical orbits of the planets could result from a gravitational force towards the sun proportional to the inverse square of the distance.

Halley went up to Cambridge, and put the problem to Newton, who said he had solved it four years earlier, but couldn't find the proof among his papers. Three months later, he sent an improved version of the proof to Halley, and devoted himself full time to developing these ideas, culminating in the publication of the Principia in 1686. This was the book that really did change man's view of the universe, as we shall shortly discuss, and its importance was fully appreciated very quickly. Newton became a public figure. He left Cambridge for London, where he was appointed Master of the Mint, a role he pursued energetically, as always, including prosecuting counterfeiters. He was knighted by Queen Anne. He argued with Hooke about who deserved credit for discovering the connection between elliptical orbits and the inverse square law until Hooke died in 1703, and he argued with a German mathematician and philosopher, Leibniz, about which of them invented calculus. Newton died in 1727, and was buried with much pomp and circumstance in Westminster Abbey--despite his well-known reservations about the

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