Monday, 19 October 2026

On This Day in Math - October 19On This Day in Math - October 19

    




I am a great believer in the simplicity of things and as you probably know I am inclined to hang on to broad & simple ideas like grim death until evidence is too strong for my tenacity.
~Sir Ernest Rutherford

The 292nd day of the year; The continued fraction representation of pi  is [3; 7, 15, 1, 292, 1, 1, 1, 2...]; the convergent obtained by  truncating before the surprisingly large term 292 yields the excellent  rational approximation 355/113 for pi. 
The approximation was found by Chinese mathematician and astronomer Zu Chongzhi(429–500 AD), using Liu Hui's algorithm which is based on the areas of regular polygons approximating a circle*Wik (My mnemonic for this, "1,1,3,3,5,5; divide in the niddle, put big over little." 

292 is the number of ways to make change for 1 dollar (or for 1 Euro), using only 1, 5 and 25 cent coins (base five coins).

292! + 291! ± 1 are 595-digit twin primes. (Are there smaller sums of consecutive factorials like this that are twin primes?)

EVENTS


1698 Halley began a scientific voyage on HMS Paramore & set out to measure magnetic variation & search for Terra Incognita *Kate Morant‏@KateMorant
This was the first time a sea voyage had been planned for the sole purpose of scientific discovery. 
Halley’s primary goal was to investigate the variation of the Earth’s magnetic compass (magnetic declination) — the angle between true north and magnetic north — in different parts of the Atlantic Ocean.
On his first voyage he sailed to the South Atlantic, reaching about 52° South latitude before being forced to turn back due to crew mutiny and illness.
The next year a second voyage continued his magnetic observations along the coasts of South America, Africa, and the mid-Atlantic.
Halley produced the first magnetic variation chart (1701), showing lines of equal magnetic declination — the first known use of isogonic lines on a map. *PB





1752 Franklin described his kite experiment in a letter written in Philadelphia and addressed to Peter Collinson, who had earlier provided Franklin with some simple apparatus for performing electrical experiments.  The kite was not struck by lightning, but Franklin notices the loose strands of the rain soaked  hemp rope  standing out straight and recognized the phenomena as indicating static electric charge, and reached out a finger and got a mild shock.
On the same date his experiment was described in the Pennsylvania Gazette.
*Julian Rubin web site

The kite experiment was described in The Pennsylvania Gazette on October 19, 1752 as follows:

Franklin's Statement:

Philadelphia, October 19, 1752

As frequent Mention is made in the News Papers from Europe, of the Success of the Philadelphia Experiment for drawing the Electric Fire from Clouds by Means of pointed Rods of Iron erected on high Buildings, &c. it may be agreeable to the Curious to be informed, that the same Experiment has succeeded in Philadelphia, tho' made in a different and more easy Manner, which any one may try, as follows.

Make a small Cross of two light Strips of Cedar, the Arms so long as to reach to the four Corners of a large thin Silk Handkerchief when extended; tie the Corners of the Handkerchief to the Extremities of the Cross, so you have the Body of a Kite; which being properly accommodated with a Tail, Loop and String, will rise in the Air, like those made of Paper; but this being of Silk is fitter to bear the Wet and Wind of a Thunder Gust without tearing. To the Top of the upright Stick of the Cross is to be fixed a very sharp pointed Wire, rising a Foot or more above the Wood. To the End of the Twine, next the Hand, is to be tied a silk Ribbon, and where the Twine and the silk join, a Key may be fastened. This Kite is to be raised when a Thunder Gust appears to be coming on, and the Person who holds the String must stand within a Door, or Window, or under some Cover, so that the Silk Ribbon may not be wet; and Care must be taken that the Twine does not touch the Frame of the Door or Window. As soon as any of the Thunder Clouds come over the Kite, the pointed Wire will draw the Electric Fire from them, and the Kite, with all the Twine, will be electrified, and the loose Filaments of the Twine will stand out every Way, and be attracted by an approaching Finger. And when the Rain has wet the Kite and Twine, so that it can conduct the Electric Fire freely, you will find it stream out plentifully from the Key on the Approach of your Knuckle. At this Key the Phial may be charged; and from Electric Fire thus obtained, Spirits may be kindled, and all the other Electric Experiments be perform'd, which are usually done by the Help of a rubbed Glass Globe or Tube; and thereby the Sameness of the Electric Matter with that of Lightning completely demonstrated.




1759 Gauss writes,in a letter to his former teacher, E. A. W. von Zimmermann, when he showed up at the Göttingen University library, "I cannot deny, that I found it very unpleasant that most of my beautiful discoveries in indefinite analysis were not original. What consoles me is this. All of Euler's discoveries that I have so far found, I have made also, and still more so. I have found a more general, and, I think, more natural viewpoint; yet I still see an immeasurable field before me..." *Animating Creativity, The LaRouche Youth Movement web page.



1892: The first long-distance telephone line opened between the cities of New York and Chicago, although it could only handle one call at a time.
Seated at a telephone in the American Telephone and Telegraph Company’s office in Quincy street, Chicago Mayor Washburne conducted Chicago’s end of the above conversation. At the. other end of the wire was Mayor Grant of New York. With this simple ceremony the long-distance telephone between Chicago and New York was formally placed in service.

Sixty persons were present to see it done. They were telephone men, merchants, and newspaper men. There were 150 people around Mayor Grant at the company’s office in Cortland street. New York, and the company so managed matters that everybody got a chance to test the workings of the line. They invited all to stand beneath two funnels fastened to the gas fixture and keep perfectly still. They did so and heard the “Star Spangled Banner” played by a cornetist in New York. Then the New York crowd gathered around similar funnels while cornetist Cobb of Johnny Hand’s orchestra played the national anthem for them. *chicagology.com

This was not the first long distance call in the US, that had happened fifteen years earlier in California. The world's first long-distance telephone line, established in 1877, connected French Corral with Bowman Lake (previously known as French Lake) at the headwaters of the Yuba River. It was strung across trees and poles for a distance of 60 mi (97 km) in Nevada County, California, passing through Birchville, Sweetland, North San Juan, Cherokee, North Columbia, Lake City, North Bloomfield, Moores Flat, Graniteville, and Milton.
The line was operated by the Ridge Telephone Company for the service of Milton Mining and Water Company, as well as other water companies. The line was an improvement over the system used in nearby Downieville, California The site is now a California Historical Landmark. *Wik Unfortunately, it seems no one made note of the first conversation.

"One Ringy Dingy"



1901 Alberto Santos-Dumont won the French Aero Club’s Deutsch Prize, rounding the Eiffel Tower and landing at Parc Saint Cloud in twenty-nine minutes and thirty seconds in his dirigible. Later it became common that a crowd would gather to see the aviator driving his Baladeuse (The Wanderer), a personal sized dirigible, over the streets as if it were a carriage or automobile.
A few years later, on October 23, 1906, Santos-Dumont won the Archdeacon prize by flying his Hargrave box kite inspired aircraft at Bagatelle in Paris. He was hailed by many in Europe as the first to fly, despite the fact that the Wright Brothers had achieved such a feat three years earlier in the United Sates. But Orville and Wilbur Wright kept their invention under wraps, avoiding any public exhibitions while they sought a patent. Most aeronauts in Europe considered them to be bluffing., *theappendix.net

1948 The National Bureau of Standards authorized construction of its Standards Western Automatic Computer. The machine, which would be built at the Institute for Numerical Analysis in Los Angeles, had an objective to compute using already-developed technology. This was in contrast to the machine’s cousin, the Standards Eastern Automatic Computer, which tested components and systems for computer *CHM
*CHM



1965 The London Times reported that an archaeologist has located what he believes to be the tomb of Archimedes.*VFR

The 1965 report referred to an archaeological find in Syracuse, Sicily, by the Italian archaeologist Salvatore Ciancio. He argued that a rock-cut burial discovered in the Grotticelle necropolis was the long-lost tomb of Archimedes. His case was published that year as La Tomba di Archimede.

But the claim did not hold up. The archaeological authorities in Syracuse, particularly the distinguished archaeologist Bernabò Brea, disputed Ciancio's identification at the time. The supposed tomb lacked the crucial identifying feature described by Cicero—a sphere and cylinder associated with Archimedes' mathematical work.  (Archimedes proved that a sphere fits tightly inside a cylinder. The sphere has 2/3 the volume and surface area of that cylinder. He was so proud of this discovery that he asked for this shape to be carved on his tomb. *PB) 
Later archaeological study has made the case even weaker. UNESCO's archaeological documentation dates the prominent "Archimedes' Tomb" at Grotticelle to the Roman period—roughly the late 1st century BC to early 1st century AD, about two centuries after Archimedes died in 212 BC. It is now understood as a Roman funerary chamber, not Archimedes' tomb.  





In 1973, a US Federal Judge signed his decision following a lengthy court trial which declared the ENIAC patent invalid and belatedly credited physicist John Atanasoff with developing the first electronic digital computer, the Atanasoff- Berry Computer or the ABC. Built in 1937-42 at Iowa State University by Atanadoff and a graduate student, Clifford Berry, it introduced the ideas of binary arithmetic, regenerative memory, and logic circuits. These ideas were communicated from Atanasoff to John Mauchly, who used them in the design of the better-known ENIAC built and patented several years later.*TIS



1994 The Pentium FDIV bug error was isolated to the Pentium Pro chip by Professor Thomas R. Nicely at Lynchburg College, Virginia, USA while working on Brun's constant (the sum of the reciprocals of the odd twin primes).   Nicely had noticed some inconsistencies in the calculations on June 13, 1994 shortly after adding a Pentium system to his group of computers, but was unable to eliminate other factors (such as programming errors, motherboard chipsets, etc.) until October 19, 1994. On October 24, 1994 he reported the issue to Intel.   The bug was rarely encountered by average users (Byte magazine estimated that 1 in 9 billion floating point divides with random parameters would produce inaccurate results) *Wik



2014 Small chance that Comet C/2013 A1 (Siding Spring), discovered in the beginning of 2013, might collide with Mars. At the moment, based on the observation arc of 74 days, the nominal close approach distance between the red planet and the comet might be as little as 0.00073 AU, that is approximately 109,200 km! Distance to Mars’ natural satellite Deimos will be smaller by 6000 km, making it 103,000 km. On the 19th October 2014, the comet might reach apparent magnitude of -8…-8.5, as seen from Mars! *Spaceobs.org
Fortunately Mars, and all three Mars orbiters were spared.  
Comet Siding Spring as seen by Hubble on 11 March 2014

*Wik






BIRTHS


1795 Arthur Jules Morin​ (19 October 1795 – 7 February 1880) was a French physicist. He conducted experiments in mechanics and invented the Morin dynamometer.
In 1850, he was elected a foreign member of the Royal Swedish Academy of Sciences. His name is one of the 72 names inscribed on the Eiffel Tower.*Wik (He was also the director of my favorite Paris Museum, Musee des Arts et Métiers.) In the issue of Nature which appeared on 5 February 1880 the following report appears:-
We regret to state that General Morin, the well-known director of the Conservatoire des Arts et Métiers, is lying in a very precarious state in consequence of a severe cold. Great anxiety is felt for him at the Institute, of which he is one of the most respected and popular members. The General is aged 85 years. In the following issue of Nature, his death in Paris on 7 February was reported. *SAU



1871 John Miller (19 Oct 1871 in Glasgow, Scotland - 14 July 1956 in Victoria Infirmary, Glasgow, Scotland) studied at Glasgow and Göttingen. He returned to Glasgow to the Royal College of Science and Technology (the precursor to Strathclyde University). He became President of the EMS in 1913. *SAU



1903 Jean Frédéric Auguste Delsarte (October 19, 1903, Fourmies – November 28, 1968, Nancy) was a French mathematician known for his work in mathematical analysis, in particular, for introducing mean-periodic functions and generalized shift operators. He was one of the founders of the Bourbaki group.*Wik
From left to right: Simone Weil (accompanying her brother André), Charles Pisot , André Weil (hidden), Jean Dieudonné (sitting), Claude Chabauty , Charles Ehresmann , and Jean Delsarte.




1910 Subrahmanyan Chandrasekhar (19 Oct 1910; 21 Aug 1995) Indian-born American astrophysicist who (with William A.Fowler) won the 1983 Nobel Prize for Physics for formulating the currently accepted theory on the later evolutionary stages of massive stars. He was one of the first scientists to combine the disciplines of physics and astronomy. Early in his career he demonstrated that there is an upper limit, now called the Chandrasekhar limit, to the mass of a white dwarf star. A white dwarf is the last stage in the evolution of a star such as the Sun. When the nuclear energy source in the center of a star such as the Sun is exhausted, it collapses to form a white dwarf. Further, it shows that stars much more massive than the Sun must either explode or form black holes. *TIS

*Linds Hall Org


1939 Doris J. Schattschneider (née Wood ;October 19, 1939  -  ) is an American mathematician, a retired professor of mathematics at Moravian College. She is known for writing about tessellations and about the art of M. C. Escher, for helping Martin Gardner validate and popularize the pentagon tiling discoveries of amateur mathematician Marjorie Rice,  and for co-directing with Eugene Klotz the project that developed The Geometer's Sketchpad.

Marjorie Rice was an amateur mathematician and San Diego mother of five who became fascinated by Martin Gardner's descriptions of tessellations by pentagonal tiles in Scientific American. She investigated, and devising her own notation system, had found a previously unknown type of pentagon tiling by February 1976. She drew up several tessellations by these new pentagon tiles and mailed her discoveries to Martin Gardner. He, in turn, sent Rice's work to Schattschneider, who was an expert in tiling patterns. Schattschneider was skeptical at first, but upon careful examination, was able to validate Rice's results. Schattschneider not only helped Martin Gardner publicize the pentagon tilings discoveries of Rice, but lauded her work as a significant discovery by an amateur mathematician.

In 1995, at a regional meeting of the Mathematical Association of America held in Los Angeles, Schattschneider convinced Rice and her husband to attend her lecture on Rice's work. At the conclusion of the talk, Schattschneider introduced the amateur mathematician who had advanced the study of tessellation. "And everybody in the room . . . gave her a standing ovation."

Schattschneider won the Mathematical Association of America's Carl B. Allendoerfer Award for excellence in expository writing in Mathematics Magazine in 1979, for her article "Tiling the plane with congruent pentagons".

In 1993, she received the Deborah and Franklin Haimo Award for Distinguished College or University Teaching of Mathematics.

In 2012, she became a fellow of the American Mathematical Society.

She delivered the Martin Gardner Lecture at MathFest in August 2021.





DEATHS

1586 Egnatio Danti (April 1536 – 10 October 1586), an Italian Dominican who made contributions to architecture, geography and astronomy.Finally, among Danti's publications, we mention Trattato del radio latino (1586) which is Danti's work describing his surveying instrument. This book appeared in the year in which Danti died. The other task he undertook just before his death was to travel to Rome, at the request of Pope Sixtus, to assist the architect Domenico Fontana, who had become architect to the papacy when Sixtus was elected, in moving the Egyptian obelisk from its place in the circus of the Vatican. The obelisk had been brought to Rome in the 1st century AD and Danti and Fontana erected it in 1586 where it now stands in the centre of St Peter's Square in the Vatican. After his return from this trip to Rome, Danti contracted pneumonia from which he died. *SAU




1875 Sir Charles Wheatstone (6 Feb 1802, 19 Oct 1875) English physicist who popularized the Wheatstone bridge, a device that accurately measured electrical resistance and became widely used in laboratories. He didn't actually invent the "Wheatstone Bridge". His contemporary, Samuel Hunter Christie, came up with the idea of the bridge circuit, but Wheatstone set the precedent for using it in the way in which it has been most commonly used. Over time, the device became associated with him and took on his name. He did, however, invent the concertina (1829), the stereoscope (1838), and an early form of the telegraph. He also  developed a chronoscope (1842) to determine the velocity of projectiles at an English gunnery.*TIS (For students of discrete math, or interested in codes, Wheatstone was also the creator of the Playfair Cipher.) A story is told that among friends he was "the life of the party" however he was afraid to speak in public. It was not unlike Wheatstone to set up a speaking engagement and cancel at the very last minute due to an awful case of stage fright. As a result of this condition Michael Faraday commentated much of Whetstone's work to the Royal Society through Faraday's famous Friday night lectures. On one such occasion Wheatstone was scheduled to speak at the Royal society and of course literally ran out the back door of the conference hall at the last minute. Faraday stepped onto the stage and delivered one of his most famous lectures, which was on the discovery of the Electro-magnetic field.

*Wik





1878 Irénée-Jules Bienaymé (28 August 1796 - 19 October 1878) was a French statistician. He built on the legacy of Laplace generalizing his least squares method. He contributed to the fields and probability, and statistics and to their application to finance, demography and social sciences. In particular, he formulated the Bienaymé-Chebyshev inequality concerning the law of large numbers and the Bienaymé formula for the variance of a sum of uncorrelated random variables.*Wik



1890 Émile Léonard Mathieu (15 May 1835 in Metz, France - 19 Oct 1890 in Nancy, France) is remembered especially for his discovery (in 1860 and 1873) of five sporadic simple groups named after him. These were studied in his thesis on transitive functions.*SAU





1899 Francis Guthrie (born 22 January 1831 in London; d. 19 October 1899 in Claremont, Cape Town) was a Cape Colony mathematician and botanist who first posed the Four Colour Problem in 1852. He studied mathematics under Augustus De Morgan, and botany under John Lindley at University College London. Guthrie obtained his B.A. in 1850, and LL.B. in 1852 with first class honours. While colouring a map of the counties of England, he noticed that at least four colours were required so that no two regions sharing a common border were the same colour. He postulated that four colours would be sufficient to colour any map. This became known as the Four Color Problem, and remained one of the most famous unsolved problems in graph theory for more than a century until it was eventually proven in 1976 using a lengthy computer-aided proof by Appel and Haken.
Guthrie arrived in South Africa on 10 April 1861 and was met and entertained by Dr Dale (later Sir Langham Dale), who was instrumental in the establishing of the University of the Cape of Good Hope in June 1873. Guthrie took up the post of mathematics master at the Graaff-Reinet College. While there he gave a course of acclaimed public lectures on botany in 1862 and thus started a lifelong friendship with local resident Harry Bolus. He advised Bolus to take up the study of botany to ease his grief at the loss of his six-year-old son. When Bolus left for Cape Town a few years later, he persuaded Guthrie to move there as well in 1875. For a while, he practised at the Bar and edited a newspaper before becoming the professor of mathematics at the South African College, which later became the University of Cape Town. He remained there from 1876 until he retired in 1898, staying on his farm at Raapenberg.

When Bolus undertook to do the family of Ericaceae for Flora Capensis, he enlisted Guthrie's aid and they collaborated until Guthrie's death. Before his death, Guthrie had made an extensive collection of the Cape Peninsula flora, which was eventually housed as the Guthrie Herbarium in the University of Cape Town Botany Department, and used for teaching and reference. Though Guthrie did not live to see the published work, he had the satisfaction of knowing that the greater part of the work on Erica had been completed. He is buried in the old cemetery attached to St. Thomas's Church in Rondebosch.

He was described as being warm-hearted, good-humoured, patient, and unpretentious. The scope of his interests was diverse and ranged from a lecture titled, "The Heat of the Sun in South Africa", in which he pointed out that it must be possible to transform solar energy into mechanical power, to aeronautics, where he was involved in the development of the first aircraft. Although dubbed the inventor of the first flying machine, no documentation of his work exists.

Some fynbos species from the Bredasdorp area were named after him: Gladiolus guthriei, Erica guthriei and Homoglossum guthriei, as well as the genus Guthriea Bolus. Cyrtanthus guthrieae was named after his daughter Louisa Guthrie, who was also a botanist. The new genus Guthriea was collected by Harry Bolus from Oudeberg in the Graaff-Reinet district, and also recorded from the Wittebergen in the Barkly East district and Mont-aux-Sources in Natal. To date no other species in this genus have been found.

Guthrie was an early member of the South African Philosophical Society (later the Royal Society of South Africa), an active member of the Meteorological Commission and an examiner of the Cape University.

The standard author abbreviation Guthrie is used to indicate this person as the author when citing a botanical name. *Wik 




1937 Sir Ernest Rutherford (30 Aug 1871, 19 Oct 1937) (baron) New Zealand-born British physicist who laid the groundwork for the development of nuclear physics. He worked under Sir J. J. Thomson at Cambridge University (1895-98). Then he collaborated with Frederick Soddy in studying radioactivity. In 1899 he discovered alpha particles and beta particles, followed by the discovery of gamma radiation the following year. In 1905, with Soddy, he announced that radioactive decay involves a series of transformations. In 1907, with Hans Geiger and Ernest Marsden, he devised the alpha-particle scattering experiment that led in 1911 to the discovery of the atomic nucleus. In 1919 he achieved the artificial splitting of light atoms. In 1908 he was awarded the Nobel Prize for Chemistry. *TIS
*Wik


1944 Denes König (21 Sept 1884 in Budapest, Hungary - 19 Oct 1944 in Budapest, Hungary) At Göttingen, König had been influenced by Minkowski's lectures on the four color problem. These lectures contributed to his growing interest in graph theory, on which he lectured in Budapest from 1911. His book, Theorie der endlichen und unendlichen Graphen, was published in 1936, and was a major factor in the growth of interest in graph theory worldwide. It was eventually translated into English under the title Theory of finite and infinite graphs (translated by R McCoart), Birkhauser, 1990; this also contains a biographical sketch by Tibor Gallai​.  König's work on the factorization of bipartite graphs relates closely to the marriage problem of Philip Hall. König's use of graphs to give a simpler proof of a determinant result of Frobenius seems to have led to some hostility between the two men.
After the Nazi occupation of Hungary, König worked to help persecuted mathematicians. This led to his death a few days after the Hungarian National Socialist Party took over the country. *SAU





1972 
Marie-Louise Dubreil-Jacotin (7 July 1905 – 19 October 1972) was a French mathematician, the second woman to obtain a doctorate in pure mathematics in France, the first woman to become a full professor of mathematics in France, the president of the French Mathematical Society, and an expert on fluid mechanics and abstract algebra.

Rue Marie-Louise-Dubreil-Jacotin, a street in the 13th arrondissement of Paris within Paris Diderot University, is named after her,  and the University of Poitiers also has a street with the same name. In semigroup theory, the Dubreil-Jacotin semigroups are also named after her, as is the Dubreil-Jacotin–Long equation, "the standard model for internal gravity waves" in fluid mechanics.



1979 Marjorie Lee Browne (September 9, 1914 – October 19, 1979) was a notable mathematics educator, the second African-American woman to receive a doctoral degree in the U.S., and one of the first black women to receive a doctorate in mathematics in the U.S.*Wik
In the 1960s, long before personal computers were widely available, Browne saw how important computing would become for both mathematics and education. At her institution, North Carolina College (now North Carolina Central University), resources were limited, and historically Black colleges and universities (HBCUs) were often left behind when it came to cutting-edge technology. Browne decided her students should not be excluded from the future of mathematics just because of lack of equipment.

So, she wrote a grant proposal to the National Science Foundation and successfully secured funding for an IBM 650 computer—one of the very first digital computers available at a university. This was extraordinary: NCCU became one of the earliest schools in the Southeast to acquire such a machine, and Browne used it not only for her own research but also to teach her students computing at a time when most undergraduates, especially African-American students, had never even seen a computer.

The impact was lasting—her push ensured that generations of students at NCCU were trained in modern mathematical tools, giving them opportunities that otherwise would have been denied. Many of her students went on to become influential educators and mathematicians themselves, carrying forward her commitment to access and excellence.*PBnotes







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

Sunday, 18 October 2026

A Non-calculus Explanation for the Volume of a Bead

   

After I wrote about the "surprising constant" that a bead formed by drilling a hole through the center of a sphere had a volume that was dependent only on the height of the remaining bead. At the time I admitted I could not think of a good "non-calculus" explanation for why the volume for a given bead height was a constant. Afterward Arjen Dijksman,(see his blog) who regularly provides helpful insights, suggested that the volume could be explained using the ideas of Mamikon Mnatsakanian that I discussed here. While I was not able to see Arjen's solution, it did lead me to realize that a "non-calculus" proof existed (with some allowances). Thinking of Mamikon's annular sweep led me to realize that every cross-section through the bead perpendicular to the axis of the drilled hole would be an annulus. In fact, using R as the original sphere's radius, r as the radius of the hole, and h as the distance above the center of the sphere where the cross section was taken, the area of the annulus would be Pi times (R2 - r2-h2), which is just the area of a circle. Now by Cavalieri's Principal, "If, in two solids of equal altitude, the sections made by planes parallel to and at the same distance from their respective bases are always equal, then the volumes of the two solids are equal." Several candidates exist with circular cross-sections; cylinders, cones, and spheres are examples. The cross-sections of the bead went from zero at the top, to a maximum at the center, so the cylinder is excluded. We can exclude the cone since their radii decrease linearly from top to bottom and our bead does not. And since we are already tempted with the idea that the volume of the bead is the same as a bead with a radius equal to half the total height of the bead, why not try to compare those? To make the notation easier, I decided to call the height of the bead 2H (letting H2 equal the value (R2 - r2). So the cross sectional area of the sphere with raidus H at any height, h, above the center will be Pi(H2 - h2). As we have shown above, the cross-sectional area of the bead at the same height h is Pi (R2 - r2-h 2). and since H2 is equal to (R2 - r2) these two are equal. So we have proven that the volume of the bead is the same as the volume of a sphere with the same height;... but did we use calculus? I fear that the proof of Cavalieri's Principal is founded in the calculus, and thus we still have a "calculus-based" explanation...but it's the best I have to offer to date.


Over the last few days I came upon a way to explain the volume of a bead with an (almost) non-calculus approach. My solution was inspired by a comment posted by Arjen Dijksman. I admitted I didn't understand his suggestion to use Mamikon's visual calculus, so he did what good teachers do. He posted a very clear explanation that even I could not miss. It's a beautiful blog, pretty math... check it out.. and Thanks loads Arjen.

On This Day in Math - October 18

  




All models are wrong, some models are useful.

~George Box

The 291st day of the year; 291 is the largest number that is not the sum of distinct non-trivial powers.

ϕ(291)=192  The number of integers less than, and relatively prime to 291 is equal to it's reversal, 192.

291 is also equal to the nth prime + n.... but for which n, children?

Because 291 = 6 x 47 + 9, it can be written as the difference of two squares, 291 = 50^2 - 47^2. (An interesting note is that every power of 2^n is either one more or one less than some member of the 6n+9 sequence. The converse is not true, 21 is easy counterexample.




EVENTS

1092 Walcher, the Prior of the monastery in Great Malvern, U.K., carried out the first known Western Experiment to improve astronomical predictions when he pointed an astrolabe toward a lunar eclipse. At this time his astrolabe was one of only a few in Europe. *Jonathan Lyons, The House of Wisdom: How the Arabs Transformed Western Civilization.
Walcher was from Lotharingia, a region influenced by the new scientific ideas coming from Spain, and arrived in England around 1091. Using an astrolabe to measure the time of several solar and lunar eclipses with an accuracy of about fifteen minutes, he computed a set of tables giving the time of the new moons from 1036 through 1111, which were considered important for medical astrology. His later observations revealed significant errors in his tables, reflecting the limitations of early medieval astronomical theory.

In his later De Dracone (ca. 1116), Walcher drew on the knowledge of Arabic astronomy that his master, Petrus Alfonsi, had brought from Spain. De Dracone discussed the motion of the lunar nodes (the head and tail of the dragon) and their significance for the computation of lunar and solar eclipses.In De Dracone, Walcher recorded angles in degrees, minutes, and seconds, although he wrote these numbers using Roman, rather than Arabic numerals.

Walcher was Prior of Malvern Priory from 1120 to 1135. Walcher's gravestone in St Anne's Chapel at the Priory Church records his abilities:

"In this chest lies Doctor Walcher, a worthy philosopher, a good astronomer, a Lotharingian, a pious and humble man, a monk, the prior of his sheepfold, a geometer and abacist. The people mourn, the clergy grieve on all sides. The first day of October brought death to this elderly man. May each believer pray that he may live in heaven. 1135."

As head of the Priory he would have been a very influential figure in the county of Worcestershire.*Wik


1604  On the night of Oct. 17/18, 1604, Johannes Kepler was viewing a triple conjunction of Mars, Jupiter, and Saturn, when he got his first glimpse of a nova, a new star.  He did not discover the nova – it had first been glimpsed several days earlier – and it was not an unprecedented event, as there had been novae in 1572, 1596, and 1600.  But Kepler’s name would get attached to this one, for several reasons.  First, the star would grow in brightness until it was so powerful that it could be seen with the naked eye in the daytime. We now recognize it as a supernova, a term not used until the twentieth century. There has been no supernova like it since the nova of 1604, and it is referred to by astronomers as Kepler’s nova, or SN 1604.
Second, Kepler carefully measured the distance of the nova from half-a-dozen nearby stars, and would continue to do so for the course of an entire year, and he found that the nova did not shift even a minute of arc in its position (astronomers would say it exhibited no parallax, or shift in position), and that therefore it really was a star, out there with all the other stars, and not some nearby phenomenon.  Aristotle had maintained that the heavens are immutable and do not change.  Tycho Brahe had first argued against this Aristotelian doctrine, when he measured the position of the nova of 1572 (Tycho’s nova) and found that it exhibited no detectable parallax.  So Kepler found new evidence to affirm Tycho’s conclusion.
Third, Kepler wrote and published a book about the new star.  He called it De stella nova in pede serpentarii (The new star in the foot of Serpentarius, Kepler’s name for the constellation we now call Ophiuchus).  The book contained a star map of Serpentarius and the surrounding constellations, which we reproduce here (first image).  Several planets are labelled, as you can see in a detail (third image). Between the two feet of Serpentarius, the labels alpha (α) and eta (η) indicate the positions of Saturn and Jupiter, as they were seen on Dec. 17, 1603.  The two are quite close together, in conjunction.  This event, known as a Great Conjunction, was especially noteworthy for astrologers, as Jupiter and Saturn come into conjunction only once every twenty years.  And it was why astronomers were looking so carefully at this part of the sky, and discovered the nova.  *Linda Hall Org






1640 Pierre de Fermat (1601–1665) explains his ‘little theorem’ to Bernard Frenicle de Bessey in a follow up to two previous letters. ("On the subject of progressions, I have sent to you in advance the propositions that serve to determine the properties of powers minus one"). The theorem, which states that np−1 ≡ 1 (mod p) if p is prime and relatively prime to n, was proved by Euler in 1736 by induction on n.[Scientific American, December 1982]
Fermat actually made three statements:
1) When the exponent, n, is composite, 2n-1 is also composite,
2) When the exponent, n, is prime, 2n -2 is divisible by 2*n,
3) When the exponent, n, is prime, the number 2n -1 can not be divided by any number less than 2n+1

*Jacqueline Stedall, Mathematics Emerging


In this same letter Fermat mentions Fermat Primes, He had mentioned them earlier in August in a letter to de Bessy but the exact date is unknown,  In it Fermat writes that he is "almost persuaded" that all numbers of the form 2^(2*n) +1 are prime and explicitly lists  3,5,17,257,65537,4294967297  saying he lacks a proof.  ..... and for good reason,In 1732, Leonhard Euler showed that  4294967297=641×6700417. *PBNotes
  




1740  In a letter to Johann Bernoulli, Euler uses imaginary in the exponent. exi + e-xi = 2 cos(x) {note Euler used square root of -1 rather than i. Euler would be the first to use i for the imaginary constant, but not until a paper he presents in St. Petersburg in 1777.} Cajori seems to imply, but does not state explicitly, that this is the first time an imaginary has been used as an exponent.






1933 Participants in the first fully international conference on nuclear physics in Rome from October 11–18, 1931, with those mentioned in the text in boldface. Foreground (left to right): Otto Stern (1888–1969), Peter Debye (1884–1966), Owen W. Richardson (1879–1959), Robert A. Millikan (1868–1973), Arthur H. Compton (1892–1962), Marie Curie (1867–1934), Guglielmo Marconi (1874–1937), Niels Bohr (1885–1962), Francis W. Aston (1877–1945), Walther Bothe (1891–1957), Bruno Rossi (1905–1993), and Lise Meitner (1878–1968, obscured). Behind Stern and Debye is Werner Heisenberg (1901–1976, obscured), Lé on Brillouin (1889–1969), Patrick M.S. Blackett (1897–1974, above Brillouin), and John S.E. Townsend (1868–1957). Between Curie and Marconi is Jean Perrin (1870–1942) and behind him is Paul Ehrenfest (1880–1933) and Enrico Fermi (1901–1954). In the row just above Ehrenfest (not the top row) and to his left is (left to right) Emil Rupp (1898-1979), Quirino Majorana (1871–1957), and Antonio Garbasso (1871–1933). Above Marconi is Orso Mario Corbino (1876–1937), above Bohr is Giulio Cesare Trabacchi (1884–1959), and above and to the right of Aston against the wall in profile is Franco Rasetti (1901–2001). Behind and to the left of Meitner is Arnold Sommerfeld (1868–1951). Among those missing from the photograph are Hans Geiger (1882–1945), Wolfgang Pauli (1900–1958), and Lé on Rosenfeld. Source: Reale Accademia d'Italia, Atti dei Convegno (ref. 21), frontispiece.  
It was the First Volta Congress — the First Volta Congress on Nuclear Physics.
The meeting’s program title is usually given as “Nuclei and Electrons” *PB



1954, Texas Instruments & Industrial Development Engineering Assoc launch the first transistor radio, Regency TR-1,  (Like many other people, I listened to the beep of Sputnik overhead on one of these straining to see it in the sky above me...."beep...beep....")


1955, a new atomic subparticle called a negative proton (antiproton) was discovered at U.C. Berkeley. The hunt for antimatter began in earnest in 1932, with the discovery of the positron, a particle with the mass of an electron and a positive charge. However, creating an antiproton would be far more difficult since it needs nearly 2,000 times the energy. In 1955, the most powerful "atom smasher" in the world, the Bevatron built at Berkeley could provide the required energy. Detection was accomplished with a maze of magnets and electronic counters through which only antiprotons could pass. After several hours of bombarding copper with protons accelerated to 6.2 billion electron volts of energy, the scientists counted a total of 60 antiprotons.*TIS
The antiproton (symbol p ) is the antiparticle of the proton . Antiprotons are stable but generally have a very short lifespan, since any collision with a proton will cause both particles to annihilate each other in a burst of energy.*Wik

Preparation for the detection of antiprotons BEV-938 by the working group: Emilio Segre , Clyde Wiegand, Edward J. Lofgren, Owen Chamberlain , Thomas Ypsilantis , Berkeley, California, 1955.





1958, Physicist William Higinbotham created what is thought to be the first video game. It was a very simple tennis game, similar to the classic 1970s video game Pong, and it was quite a hit at a Brookhaven National Laboratory open house.  


In 1948 he joined Brookhaven National Laboratory’s instrumentation group. He served as head of that group from 1951 to 1968.


During that time, in October Brookhaven held annual visitors’ days, during which thousands of people would come tour the lab. Higinbotham was responsible for creating an exhibit to show off the instrumentation division’s work.


Most of the existing exhibits were rather dull. Higinbotham thought he could better capture visitors’ interest by creating an interactive demonstration. He later recalled in a magazine interview that he had thought “it might liven up the place to have a game that people could play, and which would convey the message that our scientific endeavors have relevance for society.”

Having worked on displays for radar systems and many other electronic devices, Higinbotham had no trouble designing the simple game display.


Higinbotham made some drawings, and blueprints were drawn up. Technician Robert Dvorak spent about two weeks building the device. After a little debugging, the first video game was ready for its debut. They called the game Tennis for Two.


Tennis for Two had none of the fancy graphics video games use today. The cathode ray tube display simply showed a side view of a tennis court represented by just two lines, one representing the ground and a one representing the net. The ball was just a dot that bounced back and forth. Players also had to keep score for themselves.


Visitors loved it. It quickly became the most popular exhibit, with people standing in long lines to get a chance to play.


The first version, used in the 1958 visitor’s day, had an oscilloscope with a tiny display, only five inches in diameter. The next year, Higinbotham improved it with a larger display screen. He also added another feature: the game could now simulate stronger or weaker gravity, so visitors could play tennis on the moon, Earth or Jupiter.


After two years, Tennis for Two was retired. The oscilloscope and computer were taken for other uses, and Higinbotham designed a new visitor’s day display that showed cosmic rays passing through a spark chamber.


Higinbotham, who had already patented 20 inventions, didn’t think his tennis game was particularly innovative. Although he saw that the Brookhaven visitors liked the game, he had no idea how popular video games would later become. ....The long line of people I though was not because this was so great but because all the rest of the things were so dull,” he once said. *BNL dot gov





1962, Dr. James D. Watson of the U.S., Dr. Francis Crick and Dr. Maurice Wilkins of Britain won the Nobel Prize for Medicine and Physiology for their work in determining the double-helix molecular structure of DNA (deoxyribonucleic acid).*TIS

*NobelPrize Org




*Houston Chronicle
1983 physicist Sally Ride (1951-2012) became the first American woman – and 3rd woman of all time – to go into space. She blasted off aboard Challenger, culminating a long journey that started in 1977 when the Ph.D. candidate answered an ad seeking astronauts for NASA missions.  





BIRTHS

1863 Alan Archibald Campbell-Swinton, FRS (October 18, 1863, Scotland - February 19, 1930, London) was a Scottish consulting electrical engineer. He was an earlier experimenter in cathode rays and after 1896 he was frequently called upon by the medical profession to take "Roentgen Pictures" of bones.
He described an electronic method of producing television in a June 18,1908 letter to Nature.
He gave a speech in London in 1911 where he described in great detail how distant electric vision could be achieved. This was to be done by using cathode ray tubes (CRTs) at both the transmitting and receiving ends. This was the first iteration of the electronic television which is still in use today. When Swinton gave his speech others had already been experimenting with the use of cathode ray tubes as a receiver, but the use of the technology as a transmitter was unheard of. *Wik
Indian-head test pattern used during the black-and-white era before 1970. It was displayed when a television station first signed on every day.(Raise your hand if you remember!)🙋




1902 (Ernst) Pascual Jordan (18 October 1902 in Hanover, German Empire; d. 31 July 1980 in Hamburg, Federal Republic of Germany) German physicist who in the late 1920s founded (with Max Born and later Werner Heisenberg) quantum mechanics using matrix methods, showing how light could be interpreted as composed of discrete quanta of energy. Later, (with Wolfgang Pauli and Eugene Wigner), while it was still in its early stages of development, he contributed to the quantum mechanics of electron-photon interactions, now called quantum electrodynamics. He also originated (concurrently with Robert Dicke) a theory of cosmology that proposed to make the universal constants of nature, (such as the universal gravitational constant G), variable over time. *TIS



1919 George Edward Pelham Box (18 October 1919, March 28, 2013, Madison, WI) is a statistician, who has made important contributions in the areas of quality control, time-series analysis, design of experiments, and Bayesian inference.
Box has written research papers and published books. These include Statistics for experimenters (1978), Time series analysis: Forecasting and control (1979, with Gwilym Jenkins) and Bayesian inference in statistical analysis. (1973, with George C. Tiao). Today, his name is associated with important results in statistics such as Box–Jenkins models, Box–Cox transformations, Box–Behnken designs, and others. Box married Joan Fisher, the second of Ronald Fisher's five daughters. In 1978, Joan Fisher Box published a biography of Ronald Fisher, with substantial collaboration of Box. *Wik

 In his obituary for Box, Brad Jones of JMP recounted the following, with another fascinating Box quote,
"The last time I saw him was at the JMP Discovery Summit conference in 2009 where I introduced him to give a speech. George got a standing ovation from a crowd of several hundred fans of design of experiments and particularly his work. I will never forget his remarks as the applause died slowly away.

He said, "I feel like the son of the sultan on his 21st birthday when presented with 21 virgins. I know what to do. I just don't know where to start!"

Box died on 28 March 2013. He was 93 years old
My favorite Box quote (slightly shortened from his actual comment) is 



1926 Marco Victor "Chuck" Berry (born October 18, 1926, St. Louis, Missouri, U.S.—died March 18, 2017, St. Charles county, Missouri) was an American singer, songwriter, and guitarist who was one of the most popular and influential performers in rhythm-and-blues and rock-and-roll music in the 1950s, ’60s, and ’70s.
Raised in a working-class African American neighborhood on the north side of the highly segregated city of St. Louis, Berry grew up in a family proud of its African American and Native American ancestry(??). He gained early exposure to music through his family’s participation in the choir of the Antioch Baptist Church, through the blues and country-western music he heard on the radio, and through music classes, especially at Sumner High School. Berry was still attending high school when he was sent to a Missouri prison for young offenders to serve three years for armed robbery. After his release and return to St. Louis, he worked at an auto plant, studied hairdressing, and played music in small nightclubs.
Chuck Berry, through his energetic guitar riffs and stage presence, became one of the most influential figures in the development of rock music.
Berry traveled to Chicago in search of a recording contract, and Muddy Waters directed him to the Chess brothers. Leonard and Phil Chess signed him for their Chess label, and in 1955 his first recording session produced “Maybellene” (a country-and-western-influenced song that Berry had originally titled “Ida Red”), which stayed on the pop charts for 11 weeks, cresting at number five. Berry followed this success with extensive tours and hit after hit, including “Roll Over Beethoven” (1956), “School Day” (1957), “Rock and Roll Music” (1957), “Sweet Little Sixteen” (1958), “Johnny B. Goode” (1958), and “Reelin’ and Rockin’” (1958). His vivid descriptions of consumer culture and teenage life, the distinctive sounds he coaxed from his guitar, and the rhythmic and melodic virtuosity of his piano player (Johnny Johnson) made Berry’s songs staples in the repertoire of almost every rock-and-roll band. *Britannica 

In 1986, astronomer Carl Sagan and writer Ann Druyan wrote a letter to Chuck Berry for his 60th birthday. They told him that his song "Johnny B. Goode" was on the Voyager Golden Record aboard NASA's Voyager spacecraft, traveling billions of miles through space and lasting for a billion years.





1930 Zygmunt Wilhelm "Z. W." Birnbaum (18 October 1903 – 15 December 2000), often known as Bill Birnbaum, was a Polish-American mathematician and statistician who contributed to functional analysis, nonparametric testing and estimation, probability inequalities, survival distributions, competing risks, and reliability theory.

After first earning a law degree and briefly practicing law, Birnbaum obtained his PhD in 1929 at the University of Lwów under the supervision of Hugo Steinhaus, and was associated with the Lwów School of Mathematics. He visited University of Göttingen, Germany from 1929 to 1931, first working as an assistant for Edmund Landau.

After studying insurance mathematics and earning a diploma in actuarial science with Felix Bernstein in Göttingen, he worked as an actuary in Vienna during 1931–1932, and was then transferred to Lwów where he continued working as an actuary. After obtaining a position as a correspondent for a Polish newspaper, he arrived in New York as a reporter in 1937. He became a Professor of Mathematics at the University of Washington in 1939 (with help from Harold Hotelling and letters of reference from Richard Courant, Albert Einstein, and Edmund Landau).

Birnbaum was actively involved in reliability work with Boeing through the Boeing Scientific Research Laboratories during the late 1950s and 1960s, and was a key member of the "Seattle school of reliability", a group which also included Tom Bray, Gordon Crawford, James Esary, George Marsaglia, Al Marshall, Frank Proschan, Ron Pyke, and Sam Saunders.

Birnbaum served as Editor of the Annals of Mathematical Statistics (1967–1970) and as President of the Institute of Mathematical Statistics (1964). He received a Guggenheim Fellowship in 1960 (spent at the Sorbonne, Paris), and a Fulbright Program Fellowship in 1964 (spent at the University of Rome). *Wik




1938 Phillip Griffiths (October 18, 1938, Raleigh, North Carolina -  ) is an American mathematician, known for his work in the field of geometry, and in particular for the complex manifold approach to algebraic geometry. He was a major developer in particular of the theory of variation of Hodge structure in Hodge theory and moduli theory.*Wik





1945 Dusa McDuff FRS CorrFRSE (born 18 October 1945) is an English mathematician who works on symplectic geometry. She was the first recipient of the Ruth Lyttle Satter Prize in Mathematics, was a Noether Lecturer, and is a Fellow of the Royal Society. She is currently the Helen Lyttle Kimmel '42 Professor of Mathematics at Barnard College.

Margaret Dusa Waddington was born in London, England, on 18 October 1945 to Edinburgh architect Margaret Justin Blanco White, second wife of biologist Conrad Hal Waddington, her father.Her sister is the anthropologist Caroline Humphrey, and she has an elder half-brother C. Jake Waddington by her father's first marriage. Her mother was the daughter of Amber Reeves, the noted feminist, author and lover of H. G. Wells. McDuff grew up in Scotland where her father was Professor of Genetics at the University of Edinburgh. McDuff was educated at St George's School for Girls in Edinburgh and, although the standard was lower than at the corresponding boys' school, The Edinburgh Academy, McDuff had an exceptionally good mathematics teacher.She writes:
"I always wanted to be a mathematician (apart from a time when I was eleven when I wanted to be a farmer's wife), and assumed that I would have a career, but I had no idea how to go about it: I didn't realize that the choices which one made about education were important and I had no idea that I might experience real difficulties and conflicts in reconciling the demands of a career with life as a woman."

Turning down a scholarship to the University of Cambridge to stay with her boyfriend in Scotland, she enrolled at the University of Edinburgh. She graduated with a BSc Hons in 1967, going on to Girton College, Cambridge as a doctoral student. Here, under the guidance of mathematician George A. Reid, McDuff worked on problems in functional analysis. She solved a problem on Von Neumann algebras, constructing infinitely many different factors of type II1, and published the work in the Annals of Mathematics.

After completing her doctorate in 1971 McDuff was appointed to a two-year Science Research Council Postdoctoral Fellowship at Cambridge. Following her husband, the literary translator David McDuff, she left for a six-month visit to Moscow. Her husband was studying the Russian Symbolist poet Innokenty Annensky. Though McDuff had no specific plans it turned out to be a profitable visit for her mathematically. There, she met Israel Gelfand in Moscow who gave her a deeper appreciation of mathematics. McDuff later wrote:

[My collaboration with him]... "was not planned: it happened that his was the only name which came to mind when I had to fill out a form in the Inotdel office. The first thing that Gel'fand told me was that he was much more interested in the fact that my husband was studying the Russian Symbolist poet Innokenty Annensky than that I had found infinitely many type II-sub-one factors, but then he proceeded to open my eyes to the world of mathematics. It was a wonderful education, in which reading Pushkin, Mozart and Salieri played as important a role as learning about Lie groups or reading Cartan and Eilenberg. Gel'fand amazed me by talking of mathematics as though it were poetry. He once said about a long paper bristling with formulas that it contained the vague beginnings of an idea which he could only hint at and which he had never managed to bring out more clearly. I had always thought of mathematics as being much more straightforward: a formula is a formula, and an algebra is an algebra, but Gel'fand found hedgehogs lurking in the rows of his spectral sequences!"

On returning to Cambridge McDuff started attending Frank Adams's topology lectures and was soon invited to teach at the University of York. In 1975 she separated from her husband, and was divorced in 1978.[6][10] At the University of York, she "essentially wrote a second PhD"[9] while working with Graeme Segal. At this time a position at Massachusetts Institute of Technology (MIT) opened up for her, reserved for visiting female mathematicians. Her career as a mathematician developed further while at MIT, and soon she was accepted to the Institute for Advanced Study where she worked with Segal on the Atiyah–Segal completion theorem. She then returned to England, where she took up a lectureship at the University of Warwick.[

Around this time she met mathematician John Milnor who was then based in Princeton University. To live closer to him she took up an untenured assistant professorship at the Stony Brook University. Now an independent mathematician, she began work on the relationship between diffeomorphisms and the classifying space for foliations. She has since worked on symplectic topology. In the spring of 1985, McDuff attended the Institut des Hautes Études Scientifiques in Paris to study Mikhael Gromov's work on elliptic methods. Since 2007, she has held the Helen Lyttle Kimmel chair at Barnard College.

In 1984 McDuff married Milnor, now a professor at Stony Brook University, and a Fields medallist, Wolf Prize winner and Abel Prize Laureate.

For the past 30 years McDuff has been a contributor to the development of the field of symplectic geometry and topology. She gave the first example of symplectic forms on a closed manifold that are cohomologous but not diffeomorphic and also classified the rational and ruled symplectic four-manifolds, completed with François Lalonde. More recently, partly in collaboration with Susan Tolman, she has studied applications of methods of symplectic topology to the theory of Hamiltonian torus actions. She has also worked on embedding capacities of 4-dimensional symplectic ellipsoids with Felix Schlenk, which gives rise to some very interesting number-theoretical questions. It also indicates a connection between the combinatorics of J-holomorphic curves in the blow up of the projective plane and the numbers that appear as indices in embedded contact homology. With Katrin Wehrheim, she has challenged the foundational rigor of a classic proof in symplectic geometry.

With Dietmar Salamon, she co-authored two textbooks Introduction to Symplectic Topology and J-Holomorphic Curves and Symplectic Topology








DEATHS


1786 Alexander Wilson
 FRSE (1714 – 16 October 1786) was a Scottish surgeon, type-founder, astronomer, mathematician and meteorologist. He was the first scientist to record the use of kites in meteorological investigations. Wilson noted that sunspots viewed near the edge of the Sun's visible disk appear depressed below the solar surface, a phenomenon referred to as the Wilson effect. When the Royal Danish Academy of Sciences and Letters announced a prize to be awarded for the best essay on the nature of solar spots, Wilson submitted an entry. On 18 February 1772 the Academy presented Wilson with a gold medal for his work on sunspots.*Wik




1793 John Wilson (6 Aug 1741 in Applethwaite, Westmoreland, England - 18 Oct 1793 in Kendal, Westmoreland, England) In 1764 Wilson was elected a Fellow of Peterhouse and he taught mathematics at Cambridge with great skill, quickly gaining an outstanding reputation for himself. However, he was not to continue in the world of university teaching, for in 1766 he was called to the bar having begun a legal career on 22 January 1763 when he was admitted to the Middle Temple. It was a highly successful career, too.
He is best known among mathematicians for Wilson's theorem which states that
... if p is prime then 1 + (p - 1)! is divisible by p
This result was first published by Waring, without proof, and attributed to Wilson. Leibniz appears to have known the result. It was first proved by Lagrange in 1773 who showed that the converse is true, namely
... if n divides 1 + (n - 1)! then n is prime.
Almost certainly Wilson's theorem was a guess made by him, based on the evidence of a number of special cases, which neither he nor Waring knew how to prove. *SAU





1845 Jean-Dominique Comte de Cassini (30 June 1748 in Paris, France - 18 Oct 1845 in Thury, France)  French mathematician and surveyor who worked on his father's map of France.  He was the son of César-François Cassini de Thury and was born at the Paris Observatory. In 1784 he succeeded his father as director of the observatory; but his plans for its restoration and re-equipment were wrecked in 1793 by the animosity of the National Assembly. His position having become intolerable, he resigned on September 6, and was thrown into prison in 1794, but released after seven months. He then withdrew to Thury, where he died fifty-one years later.
He published in 1770 an account of a voyage to America in 1768, undertaken as the commissary of the French Academy of Sciences with a view to testing Pierre Le Roy’s watches at sea. A memoir in which he described the operations superintended by him in 1787 for connecting the observatories of Paris and Greenwich by longitude-determinations appeared in 1791. He visited England for the purposes of the work, and saw William Herschel at Slough. He completed his father’s map of France, which was published by the Academy of Sciences in 1793. It served as the basis for the Atlas National (1791), showing France in departments.
Cassini’s Mémoires pour servir à l’histoire de l’observatoire de Paris (1810) embodied portions of an extensive work, the prospectus of which he had submitted to the Academy of Sciences in 1774. The volume included his Eloges of several academicians, and the autobiography of his great-grandfather, Giovanni Cassini.*Wik



1871 Charles Babbage,(26 Dec 1792-18 Oct 1871) computer pioneer. His obsession for mechanizing computation made him into an embittered and crotchety old man. He especially hated street musicians, whose activities, he figured, ruined a quarter of his working potential. *VFR   English mathematician and pioneer of mechanical computation, which he pursued to eliminate inaccuracies in mathematical tables. By 1822, he had a small calculating machine able to compute squares. He produced prototypes of portions of a larger Difference Engine. (Georg and Edvard Schuetz later constructed the first working devices to the same design which were successful in limited applications.) In 1833 he began his programmable Analytical Machine, a forerunner of modern computers. His other inventions include the cowcatcher, dynamometer, standard railroad gauge, uniform postal rates, occulting lights for lighthouses, Greenwich time signals, heliograph opthalmoscope. He also had an interest in cyphers and lock-picking. *TIS
A portion of the difference engine



1917 Ruth Gentry (February 22, 1862 – October 18, 1917) was a pioneering American woman mathematician during the late 19th century and the beginning of the 20th century. She was the first Indiana-born woman to acquire a PhD degree in mathematics, and most likely the first woman born in Indiana to receive a doctoral degree in any scientific discipline.

Ruth Ellen Gentry was the youngest of three children born to Jeremiah Gentry (1827–1906) and Lucretia (Wilcox) Gentry (1830–1909). Jeremiah was a farmer and stock trader who moved to Hendricks County, Indiana from Bullitt County, Kentucky, when he was five years old, and remained there the rest of his life. Ruth and her siblings, Oliver (1853–1878) and Mary Frances (1860–1929), were born and grew up on the family farm near Stilesville, Indiana. Ruth's early education took place there as well.

Gentry attended Indiana State Normal School, a teachers' college that had opened in 1870 but did not yet award bachelor's degrees. After graduating in 1880, she taught at preparatory schools for ten years. In 1885, she decided to get her bachelor's degree at the University of Michigan—at that time one the few American colleges to admit women as undergraduates. She studied mathematics for a year and then went back to teaching school, moving to Florida for the years 1886–88 to teach at DeLand Academy and College (which changed its name while she was there to DeLand University).

Gentry did her graduate work starting in 1890 at Bryn Mawr College, which at that time was one of the only institutions of higher education in the country to admit women for graduate studies. In 1891 she was a Fellow in Mathematics at Bryn Mawr. Following her first year, she was awarded the Association of College Alumnae European Fellowship, becoming the first mathematician and second recipient of the honor.[3] She used the fellowship to study in Europe in 1891–92. Gentry went first to Germany in the hope of being allowed to sit in on lectures by German mathematicians at one of the country's universities (which at the time did not admit women). After she had been turned down by numerous professors, Lazarus Fuchs of the University of Berlin secured permission for her to attend lectures by himself and Ludwig Schlesinger. This arrangement lasted only one semester before being revoked by university administrators. She remained in Europe for an additional semester, attending lectures in mathematics at the Sorbonne in Paris.

Upon her return to Bryn Mawr, Gentry was appointed a fellow in mathematics for 1892–93, after which she stayed on another year as a fellow by courtesy of the school. She became Charlotte Scott's first graduate student, and in 1894 she finished her doctoral work at Bryn Mawr. Her thesis, On the Forms of Plane Quartic Curves, was not published until 1896, which is why she is sometimes described as one of Scott's first two students, along with Isabel Maddison.

After earning her PhD, Gentry taught at Vassar College, becoming the first person on the mathematics faculty at Vassar to hold a doctoral degree. In 1900 she was made associate professor.

Two years later, suffering from health issues, Gentry left Vassar to become the associate principal and head of the mathematics department at Miss Gleim's, a private school in Pittsburgh, Pennsylvania. In 1905 she left this position and became a volunteer nurse. She traveled in the United States and Europe for a time, but suffered from further health problems. Her illness progressed until she died of breast cancer in Indianapolis, Indiana at the age of 55 on October 18, 1917. She is buried in Stilesville Cemetery in Stilesville, Indiana.

Gentry's main interest was in geometry, especially the study of quartic curves, which was the content of her thesis.




1931 Thomas Alva Edison (11 Feb 1847-18 Oct 1931) Inventor, died in West Orange, NJ. He invented the first phonograph (1877) and the prototype of the practical incandescent electric light bulb (1879). His many inventions led to his being internationally known as "the wizard of Menlo Park", from the name of his first laboratory. By the late 1880s he was contributing to the development of motion pictures. By 1912 he was experimenting with talking pictures. His many inventions include a storage battery, a Dictaphone, and a mimeograph. Meanwhile, he had become interested in the development of a system for widespread distribution of electric power from central generating stations. He held over 1,000 patents.In 1962 his second laboratory and home in West Orange, NJ, would be designated a National Historic Site.*TIS





1974  Charles Ernest Weatherburn (18 June 1884 – 18 October 1974) was an Australian-born mathematician.

Weatherburn graduated from the University of Sydney an MA in 1906. After being awarded a scholarship he studied at Trinity College, Cambridge sitting the Mathematical Tripos examinations in 1908. Weatherburn was awarded a First Class degree. On his return to Australia, Weatherburn taught at Ormond College of the University of Melbourne.

In 1923 was appointed chair of mathematics in Canterbury College, University of New Zealand. He returned to Australia in 1929 as chair of mathematics at the University of Western Australia, a post he held until he retired in 1950.

He died in Perth, Western Australia in 1974.






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