Symmetry, as wide or narrow as you may define its meaning, is one idea by which man through the ages has tried to comprehend and create order, beauty, and perfection.
~Hermann Weyl
The 337th day of the year, 337 is a Pythagorean prime number, and when its digits are reversed, that is also prime. (A Pythagorean prime is a prime number of the form 4n + 1. Pythagorean primes are exactly the primes that are the sum of two squares (and from this derives the name in reference to the famous Pythagorean theorem.)
The mean of the first 337 square numbers is itself a square. This is the smallest number for which this is true.
The famous Fibonacci area paradox shows a 13x13 square converted to an 8x21 rectangle. The areas of the two figures, 13x13 + 8x21 = 337 (this illusion works with any Fibonacci number F(n) squared and a rectangle that is F(n-1) by F(n+1) ) Students must be aware that 13 x 13 = 169 is NOT equal to 8 x 21 = 168, so where is the flaw. Here is a post for a little history of these geometric vanishes.
EVENTS
1610 Galileo dedicates his Sidereus nuncius to Grand Duke Cosmos II. *VFR I am not sure what event Professor Rickey is referring here. According to Albert Van Helden in his introduction to his translation, "The Dedicatory letter of Sidereus nuncius is dated 12 March 1610, and on the next day Galileo sent an advance, unbound copy, accompanied by a letter, to the Tuscan court."
Thony Christie sent this translation from page 33 of the same book, "Written in Padua on the fourth day before the Ides of March 1610. Your Highnesses's most loyal servant, Galileo Galilei."
1638, Edmund Halley became a graduate of the University of Oxford without taking the degree examinations, the degree being conferred on the command of King Charles II. He was also elected a member of the Royal Society on 30 November 1678 becoming, at the age of 22, one of its youngest ever Fellows.
Halley entered Queen's College Oxford in 1673, when he was seventeen years old, already an expert astronomer with a fine collection of instruments purchased for him by his father. He began working with Flamsteed in 1675, the Astronomer Royal, assisting him with observations both at Oxford and at Greenwich. Flamsteed, in a paper of 1675 published in the Philosophical Transactions of the Royal Society, remarked:-
Edmond Halley, a talented young man of Oxford, was present at these observations and assisted carefully with many of them.
Halley made important observations at Oxford, including an occultation of Mars by the Moon on 11 June 1676, which he published in the Philosophical Transactions of the Royal Society. It is a little unclear what happened to Halley's undergraduate career, but what is certain is that he gave up his studies in 1676 and sailed to St Helena in the southern hemisphere in November of that year. The most likely explanation is that with the opening of the Royal Observatory at Greenwich in 1675, Flamsteed undertook the task of mapping the northern hemisphere stars and Halley decided to complement this programme with undertaking a similar task for the southern hemisphere.
Halley at abt age 30, In his left hand he holds a sheet of paper upon which is drawn a diagram of an elliptical orbit.
1833 Oberlin College, the first truly coeducational institution of higher education in the U.S., opens with 29 men, 15 women. *VFR
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| *WIK Partial View Oberlin by H. Alonzo Pease, 1838 |
1836 Adolphe Quetelet presents the average number of meteors per hour.
The 1833 Leonid storm had galvanized interest in meteors, and the time was ripe. Adolphe Quetelet, a Belgian statistician and founder and director of the Brussels Observatory, had mentioned mid-August meteors very tentatively six months earlier. His attention had been called to meteors by François Arago of France, who dominated European science at the time with his skill in discerning important scientific problems and suggesting experiments to solve them. What, asked Arago in the wake of the 1833 display, constituted a shower of meteors, and what was the rate of the ordinary, every night drizzle?
The problem was ideal for Quetelet, whose passion was statistics. In a speech to the Royal Academy of Sciences and Arts of Brussels on December 3, 1836, Quetelet gave his answer: averaged over the night and year, a single observer should expect to see eight sporadic (nonshower) meteors per hour. That figure is still good today. After his speech Quetelet made a brief mention of unusual August meteors, and in his 1836 annual report of the Brussels Observatory he presented the idea timidly and almost in passing: "I thought I also noticed a greater frequency of these meteors in the month of August (from the 8th to the 15th)."
By the following year, Quetelet had accidentally found records in his observatory of exceptional meteor displays on August 10th of 1834 and 1835 to accompany the increase he had seen in 1836. He called for scientists at the March 4, 1837, session of the Royal Academy of Brussel to watch the sky on August 10, 1837. *Sky and Telescope
He is also the inventor of the Body Mass Index.
1880 The Railroad Gazette credits Ellis Holbrook with being the first to give an accurate description of the so-called track transition curve, a method of making the transition from a straight track to a circular curve without the sudden lateral "jerk" caused by the change in curvature.
Unknown to them, the curve had been described {in part} by James Bernoulli in 1694 and known then as the Cantilever problem., to find the curvature a beam must have in order to be straightened by a given weight. Bernoulli gave the solution a = s^2 r where a is a constant r is the radius of curvature, thus the curvature was proportional to the arc length.
Euler, in the same year, 1744, extended the curve to the shape now called the Euler Spiral.
Euler, in the same year, 1744, extended the curve to the shape now called the Euler Spiral.
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| *Wik |
The curve emerged again in 1874 as the solution to a problem in diffraction, now known as the spiral of [Alfred] Cornu.
By 1886 the spiral attracted the attention of Italian Ernesto Cesaro, who thought the curve looked like the shape of thread wrapped on a spindle, and called the curve the clothoid, after Clotho, one of the three fates who was a spinner. HT to Julian Havel
By 1886 the spiral attracted the attention of Italian Ernesto Cesaro, who thought the curve looked like the shape of thread wrapped on a spindle, and called the curve the clothoid, after Clotho, one of the three fates who was a spinner. HT to Julian Havel
Got a note about the demo at this site, *HT @mral@mastodon.sdf.org
1910 Modern neon lighting is first demonstrated by Georges Claude at the Paris Motor Show. *PainterFlynn
1910 Modern neon lighting is first demonstrated by Georges Claude at the Paris Motor Show. *PainterFlynn
Paris is known as the “City of Light,” in part because it was the first to adopt gas street lighting. It also hosted the first neon lights, thanks to a French chemist and engineer who became known as the “Edison of Paris”: Georges Claude.
Experiments over almost two centuries pointed the way towards the gas discharge tube. Back in 1675, French astronomer Jean Picard noticed that his mercury barometer was emitting a faint glow. Eventually, physicists understood that electrons from mercury atoms were captured by the glass barometer tube, and then released when the level of the mercury dropped; these electrons excited mercury atoms in the vapor above the liquid. Much later, in 1855, a German physicist and glassblower named Heinrich Geissler invented the “geissler tube,” a long glass tube filled with gas that glowed when high voltage was applied across the tube.
The discovery of neon was part of the ongoing investigation of air. In 1775 Henry Cavendish observed a bit of gas residue after he tried to remove all the oxygen and nitrogen from a sample of air by fractional distillation. Then in the 1890s, the Scottish chemist William Ramsay identified neon, krypton, and xenon with M.W. Travers, and argon with Lord Rayleigh.
These gases also glowed with bright colors when high voltage was applied. Ramsay noted neon’s distinctive hue in his Nobel Prize lecture: it was “a brilliant flame-covered light, consisting of many red, orange, and yellow lines.” (Travers described it as a “blaze of crimson light.”) By the turn of the century, there were several varieties of electric discharge lighting available in Europe and the U.S.
Enter Georges Claude, who worked as an electrical inspector while dabbling in scientific invention. He figured out how to scale up the fractional distillation, and was soon capable of producing as much as 10,000 cubic meters of liquefied air each day. He co-founded his own company, L’Air Liquide, in 1902, selling his product to the steel industry in particular, and it quickly grew into an international corporation.
Claude had originally hoped to follow in Ramsay’s footsteps and make his own noble gaseous discoveries, but soon realized that “there was nothing more to be done.” Instead, he set about putting leftover neon produced as a byproduct from his liquefaction enterprise to good use. He disliked the overly bright electric lighting used at the time, and looked to all those previously invented gas discharge tubes for inspiration, as well as Edison’s hugely successful incandescent bulbs.
He particularly liked the design of so-called “Moore lamps,” invented by one of Edison’s former workers, Daniel McFarlan Moore. These were tall glass tubes with electrodes at either end, filled with nitrogen or CO2 at low pressure; they glowed white when high voltage was applied. But they were expensive and tended to leak, so Moore lamps never quite caught on. Claude replaced the CO2 with neon, and added a carbon filter so that impurities from the hot electrodes would not cause the electrodes to sputter and light to dim. Eventually he built 20-foot neon tubes capable of glowing for 1200 hours.
Claude quickly filed a patent, and displayed his neon tubes in December 1910, at the Paris Motor Show. People were dazzled, but the tubes weren’t ideal for general lighting.
But they were perfect for signage, and in 1912, Claude sold his first neon sign to a barbershop on the Boulevard Monmartre. Soon there was a large rooftop neon sign for Cinzano (an Italian vermouth) and entrance lighting for the Paris Opera. Claude founded his second company, Claude Neon, and made a fortune selling franchises for his neon lighting. He received a U.S. patent for neon lighting in 1915.
1958 Germany issued a stamp to commemorate the 500th anniversary of the Cusanus Hospice at Kues, founded by Cardinal Nicolaus (1401-1464), Nicolaus Cusanus (Nickolaus Krebs). *VFR
Arguably the most important German thinker of fifteenth century, Nicholas of Cusa (1401–1464) was also an ecclesiastical reformer, administrator and cardinal. His life-long effort was to reform and unite the universal and Roman Church, whether as canon law expert at the Council of Basel and after, as legate to Constantinople and later to German dioceses and houses of religion, as bishop in his own diocese of Brixen, and as advisor in the papal curia. His active life as a Church administrator and bishop found written expression in several hundred Latin sermons and more theoretical background in his writings on ecclesiology, ecumenism, mathematics, philosophy and theology. Cusanus had an open and curious mind. He was learned and steeped in the Neoplatonic tradition, well aware of both humanist and scholastic learning, yet mostly self-taught in philosophy and theology. Nicholas anticipated many later ideas in mathematics, cosmology, astronomy and experimental science while constructing his own original version of systematic Neoplatonism. A whole range of earlier medieval writers, such as Thierry of Chartre, Ramon Llull and Albert the Great, influenced Nicholas, but his important intellectual roots are in Proclus and Dionysius the Areopagite. In spite of his significance few later thinkers, apart from Giordano Bruno, understood or were influenced by him until the late nineteenth century *Stanford Ency. of Philosophy
Mathematics plays a key role for Cusanus in orienting the human mind towards God. Mathematical figures provide a means for the mind to consider how figures may be deformed and transformed, and thus prepares the mind to reach the "coincidence of opposites" in the "Absolutely maximal Being".
From the Catholic Encyclopedia (1913 edition):
Like Nicole Oresme, Nicholas also wrote about the possibility of the plurality of worlds.
1968 CDC Announces 7600 Supercomputer: Control Data Corporation announces its 7600 model, considered by some to be the first true supercomputer. The CDC 7600 calculated at a speed of nearly 40 megaflops. Seymour Cray designed this computer, as well as its predecessor, the 6600 that was popular with scientific researchers, and a successor, the 8600, which the company never marketed. *CHM
1992 a test engineer for Sema Group uses a personal computer to send the world's first text message via the Vodafone network to the phone of a colleague. *PainterFlynn
The first SMS message was sent over the Vodafone GSM network in the United Kingdom on 3 December 1992, from Neil Papworth of Sema Group (now Mavenir Systems) using a personal computer to Richard Jarvis of Vodafone using an Orbitel 901 handset. The text of the message was "Merry Christmas."
BIRTHS
1616 John Wallis (3 Dec 1616; 8 Nov 1703) English mathematician. Wallis was skilled in cryptography and decoded Royalist messages for the Parliamentarians during the Civil War. Wallis was part of a group interested in natural and experimental science who started to meet in London. This group became the Royal Society (1663), with Wallis as a founder member and one of its first Fellows. He contributed substantially to the origins of calculus and was the most influential English mathematician before Newton. Wallis introduced our symbol for infinity (1656), and exponents using negative or fractional numbers (such as 1/x2 = x-2 or square root of x = x-1/2). In 1668, he was the first to suggest the law of conservation of momentum for colliding bodies, the first of all-important conservation laws.*TIS
1842 Ellen Henrietta Swallow Richards, ( December 3, 1842 – March 30, 1911) an American chemist, was born Dec. 3, 1842, in Dunstable, Mass. She attended Vassar College and received a degree in chemistry in 1870, and to further her studies, she applied for admission to MIT. MIT had never admitted a female student, and at a special session of the admission committee, she was granted entrance, with the explicit proviso that her admission was not to be seen as a precedent for admitting further females to the MIT ranks. Swallow (she had not yet married) got a second chemistry degree in 1873 and did the required work for a Masters, but that degree was never granted, since MIT had not yet awarded a Master’s degree to anyone, much less a woman. She taught for some years, unpaid, at a Women's Laboratory at MIT, meeting the needs of secondary school science teachers who had no laboratory experience. Finally, Richards (she was now married to Robert Richards, a Professor of Mining Science at MIT) received a paid appointment as an instructor in chemistry at MIT. She was thus the first woman instructor at MIT, having already been the first woman admitted, and the first to be granted a degree. She was also the first woman in the entire country to receive a degree in chemistry, which she did twice.
On December 10, 1870, after some discussion and a vote, the Faculty of the Institute of Technology recommended to the MIT Corporation the admission of Swallow as a special student in chemistry. Swallow thus became the first woman admitted to Massachusetts Institute of Technology, although the corporation made it clear that "her admission did not establish a precedent for the general admission of females," according to the records of the corporation's meeting on December 14, 1870. In 1873, Swallow received a Bachelor of Science degree from MIT for her thesis, "Notes on Some Sulpharsenites and Sulphantimonites from Colorado". She continued her studies at MIT and would have been awarded its first advanced degree, but MIT balked at granting this distinction to a woman and did not award its first advanced degree, a Master of Science in chemistry, until 1886.
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1903 Sydney Goldstein (3 Dec 1903 in Hull, England - 22 Jan 1989 in Belmont, Massachusetts, USA) Goldstein's work in fluid dynamics is of major importance. He is described as, "... one of those who most influenced progress in fluid dynamics during the 20th century." He studied numerical solutions to steady-flow laminar boundary-layer equations in 1930. In 1935 he published work on the turbulent resistance to rotation of a disk in a fluid. His work was important in aerodynamics, a subject in which Goldstein was extremely knowledgeable. *SAU
1924 John Warner Backus (December 3, 1924 – March 17, 2007) was an American computer scientist. He led the team that invented and implemented FORTRAN, the first widely used high-level programming language, and was the inventor of the Backus–Naur form (BNF), a widely used notation to define syntaxes of formal languages. He later did research into the function-level programming paradigm, presenting his findings in his influential 1977 Turing Award lecture "Can Programming Be Liberated from the von Neumann Style?"
The IEEE awarded Backus the W. W. McDowell Award in 1967 for the development of FORTRAN. He received the National Medal of Science in 1975 and the 1977 Turing Award "for profound, influential, and lasting contributions to the design of practical high-level programming systems, notably through his work on FORTRAN, and for publication of formal procedures for the specification of programming languages"
1938 Cleveland Abbe (3 Dec 1838; 28 Oct 1916) U.S. astronomer and first meteorologist, born in New York City, the "father of the U.S. Weather Bureau," which was later renamed the National Weather Service. Abbe inaugurated a private weather reporting and warning service at Cincinnati. His weather reports or bulletins began to be issued on Sept. 1, 1869. The Weather Service of the United States was authorized by Congress on 9 Feb 1870, and placed under the direction of the Signal Service. Abbe was the only person in the country who was already experienced in drawing weather maps from telegraphic reports and forecasting from them. Naturally, he was offered an important position in this new service which he accepted, beginning 3 Jan 1871, and was often the official forecaster of the weather.*TIS
1939 Mario Wschebor ( 3 December 1939, 16 September 2011) was a Uruguayan mathematician and statistician who has a remarkable record of outstanding papers, and an international reputation of speaking at conferences around the world. Yet his career was disrupted by having to flee because of political events. He was also passionate about political and social issues and fought throughout his career for an improved university system. *SAU
In the field of mathematics, he made important contributions to probability and statistics . He was the author of numerous scientific publications, including Level Sets and Extrema of Random Processes and Fields (Wiley, UK, 2009), in collaboration with Jean-Marc Azaïs.
He was a prominent university leader, serving as Dean of the Faculty of Sciences at the University of the Republic from 1987 to 1997, after actively participating in its creation. An important contribution from this period is the Document of the Four Deans , in which he advocated the need for the creation of a national tertiary education system. *Wik
1942 Joseph Ivor Silk FRS (3 December 1942-) was the Savilian Chair of Astronomy at the University of Oxford from 1999 to September 2011. He was educated at Tottenham County School (1954-1960) and went on to study Mathematics at the University of Cambridge (1960-1963). He gained his PhD in Astronomy from Harvard in 1968. Silk took up his first post at Berkeley in 1970, and the Chair in Astronomy in 1978. Following a career of nearly 30 years there, Silk returned to the UK in 1999 to take up the Savilian Chair at the University of Oxford. He is currently Professor of Physics at the Institut d’Astrophysique de Paris, Université Pierre et Marie Curie, and he joined Johns Hopkins University in 2010 as Homewood Professor of Physics and Astronomy.
He is an Emeritus Fellow of New College, Oxford and a Fellow of the Royal Society (elected May 1999). He was awarded the 2011 Balzan Prize for his works on the early Universe. Silk has given more than two hundred invited conference lectures, primarily on galaxy formation and cosmology.
In 2015 he was selected the Gresham Professor of Astronomy. *Wik
DEATHS
1882 James Challis (12 Dec 1803, 3 Dec 1882) British clergyman and astronomer, famous in the history of astronomy for his failure to discover the planet Neptune. Astronomer and mathematician John Couch Adams had studied the known deviations in the orbit of the planet Uranus which indicated a planet even further out. In 1845, Adams gave Astronomer Royal George Airy a calculated orbital path for the unknown planet. But Airy was more interested in the primary job of navigation and timekeeping observations. Airy informed Challis, who did not begin until July 1846, and actually sighted the new planet four times without recognizing it. On 23 Sep 1845, the new planet was instead discovered from Berlin Observatory. Challis admitted that Adam's prediction was within 2° of the planet's position.*TIS
1956 Felix Bernstein (24 Feb 1878 in Halle, Germany - 3 Dec 1956 in Zurich, Switzerland) established his famous theorem on the equivalence of sets while in Cantor's seminar at Halle in 1897. He also worked on transfinite ordinal numbers.Bernstein is best remembered by mathematicians for the Schröder-Bernstein Theorem. This theorem states:
If each of two sets A and B are equivalent to a subset of the other, then A is equivalent to B. *SAU
1983 Elliott Waters Montroll (May 4, 1916 in Pittsburgh, Pennsylvania, USA - December 3, 1983 in Chevy Chase, Maryland, USA) was an American scientist and mathematician.Montroll had an exceptionally varied career: was a Sterling Research Fellow at Yale University where his work on the Ising model of a ferromagnet led him to solve certain Markov chain problems. Following this he was a Research Associate at Cornell University in 1941-42 where he began his studies of the problem of finding the frequency spectrum of elastic vibrations in crystal lattices. He was elected to the National Academy of Sciences (United States) in 1969, and to the American Academy of Arts and Sciences in 1973. His work on traffic flow led to him winning (jointly) the Lanchester Prize of the Operations Research Society of America in 1959. *Wik
2004 Shiing-shen Chern (26 Oct 1911, 3 Dec 2004) Chinese-American mathematician and educator whose researches in differential geometry include the development of the Chern characteristic classes in fibre spaces, which play a major role in mathematics and in mathematical physics. "When Chern was working on differential geometry in the 1940s, this area of mathematics was at a low point. Global differential geometry was only beginning, even Morse theory was understood and used by a very small number of people. Today, differential geometry is a major subject in mathematics and a large share of the credit for this transformation goes to Professor Chern." *TIS
2008 Oliver Gordon Selfridge (May 10, 1926 – December 3, 2008), grandson of Harry Gordon Selfridge, the founder of Selfridges' department stores, was a pioneer of artificial intelligence. He has been called the "Father of Machine Perception."
Selfridge was born in England, educated at Malvern College and Middlesex School and then earned an S.B. from MIT in mathematics in 1945. He then became a graduate student of Norbert Wiener's at MIT, but did not write up his doctoral research and never earned a Ph.D. While at MIT, he acted as one of the earlier reviewers for Wiener's Cybernetics book in 1949. He was also technically a supervisor of Marvin Minsky, and helped organize the first ever public meeting on Artificial Intelligence (AI) with Minsky in 1955.
Selfridge wrote important early papers on neural networks and pattern recognition and machine learning, and his "Pandemonium" paper (1959) is generally recognized as a classic in artificial intelligence. In it, Selfridge introduced the notion of "demons" that record events as they occur, recognize patterns in those events, and may trigger subsequent events according to patterns they recognize. Over time, this idea gave rise to Aspect-oriented programming.
In 1968, in their formative paper "The Computer as a Communication Device", J. C. R. Licklider and Robert Taylor introduced a concept known as an OLIVER (Online Interactive Expediter and Responder) which was named in honor of Selfridge.
Selfridge spent his career at Lincoln Laboratory, MIT (where he was Associate Director of Project MAC), Bolt, Beranek and Newman, and GTE Laboratories where he became Chief Scientist. He served on the NSA Advisory Board for 20 years, chairing the Data Processing Panel. Selfridge retired in 1993.
Selfridge also authored four children's books, "Sticks", "Fingers Come In Fives", "All About Mud", and "Trouble With Dragons". *Wik
2010 Cora Susana Sadosky de Goldstein (May 23, 1940 – December 3, 2010) was an Argentine mathematician and Professor of Mathematics at Howard University. She wrote over fifty papers in harmonic analysis and operator theory. She promoted women in mathematics as well encouraging greater participation of African-Americans in mathematics.
She was appointed a visiting professorship for women (VPW) in science and technology from the National Science Foundation (NSF) for 1983–1984 and spent it at the Institute for Advanced Study. She received a second VPW in 1995 which she spent as visiting professor at the University of California at Berkeley. She received a Career Advancement Award from the NSF in 1987–1988 which allowed her to spend the year as a member of the classical analysis program at Mathematical Sciences Research Institute (MSRI), where she later returned as a research professor.
She was elected president of the Association for Women in Mathematics (AWM) for 1993–1995. The Sadosky Prize of the AWM is named in her honor.*Wik
Sadosky was born in Buenos Aires, Argentina, the daughter of mathematicians Manuel Sadosky and Corina Eloísa "Cora" Ratto de Sadosky. At the age of 6, she moved with her parents to France and Italy. *PB Notes
Credits :
*CHM=Computer History Museum
*FFF=Kane, Famous First Facts
*NSEC= NASA Solar Eclipse Calendar
*RMAT= The Renaissance Mathematicus, Thony Christie
*SAU=St Andrews Univ. Math History
*TIA = Today in Astronomy
*TIS= Today in Science History
*VFR = V Frederick Rickey, USMA
*Wik = Wikipedia
*WM = Women of Mathematics, Grinstein & Campbell
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