Saturday, 26 September 2026

Two verses from a poem by James Clerk Maxwell.

     Two verses from a poem by James Clerk Maxwell.  Think deeply on them at your peril, student!


 A vision of a Wrangle,  of a University, of Pedantry, and of Philosophy

Deep St. Mary's bell had sounded,
    And the twelve notes gently rounded
    Endless chimneys that surrounded
        My abode in Trinity.
    (Letter G, Old Court, South Attics),
    I shut up my mathematics,
    That confounded hydrostatics —
        Sink it in the deepest sea!

    In the grate the flickering embers
  Served to show how dull November’s
  Fogs had stamped my torpid members,
      Like a plucked and skinny goose.
  And as I prepared for bed, I
  Asked myself with voice unsteady,
  If of all the stuff I read, I
      Ever made the slightest use.

The rest, I fear you may seek, on the internet, for a peek.  

Friday, 25 September 2026

On This Day in Math - September 26

  



"mathematics is not yet ready for such problems"

~Paul Erdos in reference to Collatz's problem

[What is the Collatz Conjecture?The rules: Pick any positive whole number. If it is even, divide it by 2. If it is odd, multiply it by 3 and add 1.The process: Repeat these steps with your new number.The conjecture:You will always get to the number one.]

It takes 29 iterations for the number 269 to reach 1. This is the 269th day of the year, (on non-leap years, the 269th day is Sep 26, and the date is written 26/9 in much of Europe. This is the only day of the year which presents itself in this way. (Are there any days that work using month/day?)


269 is a regular prime, an Eisenstein prime with no imaginary part, a long prime, a Chen prime, a Pillai prime, a Pythagorean prime, a twin prime, a sexy prime, a Higgs prime, a strong prime, and a highly cototient number. So many new terms to look up... Well? Look them up.

269 is also the Hypotenuse of a Primitive Pythagorean triple, (69, 260 269)

269 is the smallest natural number that cannot be represented as the determinant of a 10 × 10 (0,1)-matrix

Prime Curios offers this interesting convention of prime numbers, "The longest official game of chess on record (269 moves) took place in Yugoslavia on 2/17/89 and ended in a draw. Note that 2, 17, 89, and 269 are all prime numbers." And I'm guessing that Yugoslavia was a Prime country in its day.

Prime Curios also had this interesting tidbit, "The smallest prime whose square, 72361, is a concatenation of primes in two ways, i.e., (7, 23, 61) and (7, 2, 3, 61).)

269 is the largest prime factor of 9! + 1 = 362881.

269 Like all Pythagorean Primes (of the form 4n+1) is the sum of two squares, conjectured by Fermat, proved by Euler. 269 = 10^2 + 13^2.

269 is also the difference of two squares, as 135^2 - 134^2,




EVENTS


1679 On September 26, 1679, a fierce fire consumed the Stellaburgum — Europe’s finest observatory, built by the pioneering astronomer Johannes Hevelius in the city of Danzig, present-day Poland, decades before the famous Royal Greenwich Observatory and Paris Observatory existed.

And while he rebuilt the observatory, it simply did not compare with the original. He never fully recovered from the loss. His resilience in continuing was in large part fueled by the miraculous salvation of one of his manuscripts — his fixed-star catalog, which contained the results of thousands of calculations of the positions of the stars made over decades of patient observation. The small leather-bound notebook was the sole manuscript to survive the fire, presumably saved by Hevelius’s 13-year-old daughter Katharina Elisabeth, the sole family member in Danzig at the time of the fire, who had a key to her father’s study. Half a millennium later, it was rediscovered. In 1971, it made its way to Utah’s Brigham Young University, becoming the one-millionth acquisition by the institution’s library.
 Nearly two centuries before Maria Mitchell, Elisabeth Hevelius essentially became the first Western female astronomer. After his death, Elisabeth, who had assisted him in the catalog all along, took it upon herself to finish Hevelius’s lifelong quest. She completed the book, dedicating it to the generous Polish monarch. The finished catalog included more than 600 new stars that Johannes and Elisabeth had observed, as well as a dozen new constellations, whose names, as given by Hevelius, astronomers still use today.
*History of Astronomy @HistAstro
*Maria Popova at brainpickings.org

One of the constellations named by Hevelius was Leo Minor, nestled between the Big Bear and the Big Lion.




1732,  In Dec. of 1729, Goldbach wrote to Euler to ask, "Do you know about Fermat's remark that all numbers of the form \( 2^{2^{x}} +1 \) are prime?"   Less than three years later Euler shows that F5, 4294967297, the fifth Fermat "prime" is, in fact, not prime, but divisible by 641. He goes on to show that it is also the sum of two squares, in two different ways.
\(2^{32}+1)^2 = 65536^2+1= 62264^2+204496^2\)

Euler



Fermat




1775 John Adams writes to his wife, Abigail (Smith) Adams  to entreat her to teach his children geometry and... "I have seen the Utility of Geometry, Geography, and the Art of drawing so much of late, that I must intreat you, my dear, to teach the Elements of those Sciences to my little Girl and Boys. It is as pretty an Amusement, as Dancing or Skaiting, or Fencing, after they have once acquired a Taste for them. No doubt you are well qualified for a school Mistress in these Studies, for Stephen Collins tells me the English Gentleman, in Company with him, when he visited Braintree, pronounced you the most accomplished Lady, he had seen since he left England.—You see a Quaker can flatter, but don't you be proud. *Natl. Archives

Adams had studied some mathematics at Harvard (where geometry, trigonometry, and surveying were part of the curriculum), but his real talents lay in rhetoric, law, and politics. He was never known for facility with numbers.

Abigail, meanwhile, had almost no access to formal schooling—very typical for girls in colonial New England. What she knew of arithmetic and mathematics she learned at home, largely self-taught. We don’t have evidence that she was a “better mathematician” in the technical sense, but she was certainly better at education in practice. She managed the family farm accounts during John’s long absences, dealt with business matters, and taught their children. John Quincy Adams later praised her influence as formative in his education. *PB notes

Abigail Adams 



1874 James Clerk Maxwell in a letter to Professor Lewis Campbell describes Galton, "Francis Galton, whose mission it seems to be to ride other men's hobbies to death, has invented the felicitous expression 'structureless germs'. " *Lewis Campbell and William Garnett (eds.), The Life of James Clerk Maxwell (1884), 299.




1924  Jean Hoerni, a pioneer of the transistor, is born in Switzerland. A physicist, Hoerni in 1959 invented the planar process, which, combined with Robert Noyce's technique for placing a layer of silicon dioxide on a transistor, led to the creation of the modern integrated circuit. Hoerni's planar process allowed the placement of complex electronic circuits on a single chip. *CHM

early integrated circuit


1960 On this day in 1960, U.S. presidential candidates Richard Nixon and John F. Kennedy debated each other. It was a landmark event: Never before had the major-party nominees for president faced each other in a nationally televised debate. One candidate looked tired and ill, gray, and sweaty, while the other was (comparatively) energetic, neat, and clean—with a fresh tan too. The latter was Kennedy, who went on to win by one of the narrowest majorities in the history of U.S. presidential elections. *Britannica

The 1960 United States presidential debates were a series of debates held during the 1960 presidential election. Four presidential debates were held between Republican nominee Richard Nixon and Democratic nominee John F. Kennedy. All four presidential debates were the first series of debates conducted for any US presidential election. The next presidential debate did not occur until 1976, after which debates would become a regular feature of all presidential campaigns.*Wik 





1991 The first two year closed mission of Biosphere 2 began just outside Tucson, Arizona. Four men and four women entered the Biosphere 2 on this day in 1991. For two years, the eight participants lived in this huge glass and steel structure in the Arizona desert completely closed off from the rest of the world. It also contained 4,000 species of plants, animals and microbes. *On This Day in Chemistry

Biosphere II , or Biosphere 2 , is an experimental facility built to replicate a closed, artificial ecological system located in Oracle , Arizona , in the desert at the foot of the Santa Catalina Mountains . Biosphere 2 was constructed between 1987 and 1991 by Space Biosphere Ventures, a company founded by John Polk Allen and Margret Augustine. The structure aimed to recreate a viable ecosystem within a massive, enclosed dome. One of its objectives was to assess the feasibility of similar biospheres for future space colonization . The experiment was named Biosphere 2 , considering Earth to be " Biosphere 1. " The necessary funding, estimated at $200 million, was provided by Edward Bass between 1985 and 2007. . *Wik




1999 The Kobe meteorite fell on September 26 (local time 20:23), 1999, in Kita-ku in the north of Kobe city, Japan. The meteorite fall was widely observed in Kobe and the surrounding area, and was photographed by an amateur photographer in Imabari city, 200 km southwest of Kobe. The meteorite struck a house with an explosive sound but otherwise caused only minor property damage. The approximately 20 fragments of the meteorite had a total mass of 136 g. *terrapub.co.jp



 2011 Astronauts had this view of the aurora on September 26, 2011. Credit: NASA

We’ve had some great views of the aurora submitted by readers this week, but this one taken from the International Space Station especially highlights the red color seen by many Earth-bound skywatchers, too. Karen Fox from the Goddard Space Flight Center says the colors of the aurora depend on which atoms are being excited by the solar storm. In most cases, the light comes when a charged particle sweeps in from the solar wind and collides with an oxygen atom in Earth’s atmosphere. This produces a green photon, so most aurora appear green. However, lower-energy oxygen collisions as well as collisions with nitrogen atoms can produce red photons — so sometimes aurora also show a red band as seen here. *Universe Today




BIRTHS


1688 Willem 's Gravesande (26 September 1688 – 28 February 1742)was a Dutch mathematician who expounded Newton's philosophy in Europe. In 1717 he became professor in physics and astronomy in Leiden, and introduced the works of his friend Newton in the Netherlands.
His main work is Physices elementa mathematica, experimentis confirmata, sive introductio ad philosophiam Newtonianam or Mathematical Elements of Natural Philosophy, Confirm'd by Experiments (Leiden 1720), in which he laid the foundations for teaching physics. Voltaire and Albrecht von Haller were in his audience, Frederic the Great invited him in 1737 to come to Berlin.
His chief contribution to physics involved an experiment in which brass balls were dropped with varying velocity onto a soft clay surface. His results were that a ball with twice the velocity of another would leave an indentation four times as deep, that three times the velocity yielded nine times the depth, and so on. He shared these results with Émilie du Châtelet, who subsequently corrected Newton's formula E = mv to E = mv2. (Note that though we now add a factor of 1/2 to this formula to make it work with coherent systems of units, the formula as expressed is correct if you choose units to fit it.) *Wik

's Gravesande is also remembered for his invention of a simple experiment you may have tried in middle school science.  It is a simple experiment demonstrating thermal expansion, which has been used in physics education since. This is known today as "'s Gravesande's experiment" or "'s Gravesande's ring". The apparatus consists of a small metal ball on a chain or handle, and a metal ring on a stand. The ring is just big enough so that when the ring and ball are at the same temperature, the ball fits through the ring. However, if the ball is heated by dipping it into boiling water or playing the flame of a spirit lamp over it, the metal will expand, and the ball will no longer fit through the ring. When the ball has cooled down, it will fit through the ring again.






1754 Joseph-Louis Proust (26 Sep 1754; 5 Jul 1826) French chemist who proved (1808) that the relative quantities of any given pure chemical compound's constituent elements remain invariant, regardless of the compound's source, and thus provided crucial evidence in support of John Dalton's “law of definite proportions,” which holds that elements in any compound are present in fixed proportion to each other. *TIS




1731  Giovanni Francesco Giuseppe Malfatti, also known as Gian Francesco or Gianfrancesco (26 September 1731 – 9 October 1807) was an Italian mathematician. He was born in Ala, Trentino, Italy and died in Ferrara.

Malfatti studied at the College of San Francesco Saverio in Bologna where his mentors included Vincenzo Riccati, F. M. Zanotti and Gabriele Manfredi. He moved to Ferrara in 1754, and became a professor at the University of Ferrara when it was re-established in 1771. In 1782 he was one of the founders of the Societa Italiana delle Scienze, later to become the Accademia nazionale delle scienze detta dei XL.

In 1803, Malfatti posed the problem of carving three circular columns out of a triangular block of marble, using as much of the marble as possible, and conjectured that three mutually-tangent circles inscribed within the triangle would provide the optimal solution. These tangent circles are now known as Malfatti circles after his work, despite the earlier work of Japanese mathematician Ajima Naonobu and of Malfatti's countryman Gilio di Cecco da Montepulciano on the same problem and despite the fact that the conjecture was later proven false. Several triangle centers derived from these circles are also named after both Ajima and Malfatti 

For most triangles a larger area can be achieved by a greedy algorithm that inscribes a single circle of maximal radius within the triangle, inscribes a second circle within one of the three remaining corners of the triangle, the one with the smallest angle, and inscribes a third circle within the largest of the five remaining pieces. The difference in area for an equilateral triangle is small, just over 1%, but as Howard Eves (1946) pointed out, for an isosceles triangle with a very sharp apex, the optimal circles (stacked one atop each other above the base of the triangle) have nearly twice the area of the Malfatti circles.

Eventually it was shown that the Malfatti circles are never optimal. *Wik





Malfatti's Circles, *Wik



1784 Christopher Hansteen (26 Sep 1784; 15 Apr 1873) Norwegian astronomer and physicist noted for his research in geomagnetism. In 1701 Halley had already published a map of magnetic declinations, and the subject was studied by Humboldt, de Borda, and Gay-Lussac, among others. Hansteen collected available data and also mounted an expedition to Siberia, where he took many measurements for an atlas of magnetic strength and declination.*TIS



1854 Percy Alexander MacMahon (26 Sept 1854 , 25 Dec 1929) His study of symmetric functions led MacMahon to study partitions and Latin squares, and for many years he was considered the leading worker in this area. His published values of the number of unrestricted partitions of the first 200 integers which proved extremely useful to Hardy and Littlewood in their own work on partitions. He gave a Presidential Address to the London Mathematical Society on combinatorial analysis in 1894. MacMahon wrote a two volume treatise Combinatory analysis (volume one in 1915 and the second volume in the following year) which has become a classic. He wrote An introduction to combinatory analysis in 1920. In 1921 he wrote New Mathematical Pastimes, a book on mathematical recreations. *SAU



1887 Sir Barnes (Neville) Wallis (26 Sep 1887; 30 Oct 1979) was an English aeronautical designer and military engineer whose famous 9000-lb bouncing "dambuster" bombs of WW II destroyed the German Möhne and Eder dams on 16 May 1943. He designed the R100 airship, and the Vickers Wellesley and Wellington bombers. The specially-formed RAF 617 Squadron precisely delivered his innovative cylindrical bombs which were released from low altitude, rotating backwards at high speed that caused them to skip along the surface of the water, right up to the base of the dam. He later designed the 5-ton Tallboy and 10-ton Grand Slam earthquake bombs (which used on many enemy targets in the later years of the war). Postwar, he developed ideas for swing-wing aircraft. *TIS (His courtship with his wife has been written by his daughter, Mary Stopes-Roe from the actual courtship in the entertaining, but perhaps overpriced book, Mathematics With Love: The Courtship Correspondence of Barnes Wallis, Inventor of the Bouncing Bomb.)



1891 Hans Reichenbach (September 26, 1891, April 9, 1953) was a leading philosopher of science, educator and proponent of logical empiricism. Reichenbach is best known for founding the Berlin Circle, and as the author of The Rise of Scientific Philosophy.*Wik



1924 Jean Hoerni, (September 26,  1924 – January 12, 1997)a pioneer of the transistor, is born in Switzerland. A physicist, Hoerni in 1959 invented the planar process, which, combined with Robert Noyce's technique for placing a layer of silicon dioxide on a transistor, led to the creation of the modern integrated circuit. Hoerni's planar process allowed the placement of complex electronic circuits on a single chip. *CHM



1926 Colin Brian Haselgrove (26 September 1926 , 27 May 1964) was an English mathematician who is best known for his disproof of the Pólya conjecture in 1958. the Pólya conjecture stated that 'most' (i.e. more than 50%) of the natural numbers less than any given number have an odd number of prime factors. The conjecture was posited by the Hungarian mathematician George Pólya in 1919.. The size of the smallest counter-example is often used to show how a conjecture can be true for many numbers, and still be false. *Wik


1927 Brian Griffiths (26 Sept 1927 , 4 June 2008) He was deeply involved in the 'School Mathematics Project', he served as chairman of the 'Joint Mathematical Council', and chaired the steering group for the 'Low Attainers Mathematics Project' from 1983 to 1986. This project became the 'Raising Achievement in Mathematics Project' in 1986 and he chaired this from its foundation to 1989. *SAU

There is contemporary evidence that LAMP → RAMP produced positive effects, but the evidence is mostly program reports and case-study/teacher-research data (not large randomized trials), so the results are encouraging rather than definitive.  *PB notes





DEATHS


1766 Giulio Carlo Fagnano dei Toschi died. He is important for the identity

\pi = 2i\log{1 - i \over 1 +i}

and for his rectification of the lemmiscate. *VFR An Italian mathematician who worked in both complex numbers and on the geometry of triangles.*SAU
The lemniscate is of particular interest because, even if it has little relevance today, it
was
the catalyst for immeasurably important mathematical development in the 18th and 19th centuries. The figure 8-shaped curve first entered the minds of mathematicians in 1680, when Giovanni Cassini presented his work on curves of the form, appropriately known as the ovals of Cassini. Only 14 years later, while deriving the arc length of the lemniscate, Jacob Bernoulli became the first mathematician in history to define arc length in terms of polar coordinates.
The first major result of work on the lemniscate came in 1753, when, after reading Giulio Carlo di Fagnano’s papers on dividing the lemniscate using straightedge and compass, Leonhard Euler proved that:


Jacobi called December 23,1751 "the birthday of elliptic functions", as this was the day that Euler began reviewing the papers of Fagnanao who was being considered for membership in the Berlin Academy. *Raymond Ayoub, The lemniscate and Fagnano's contributions to elliptic integrals


1802 Jurij Vega (23 Mar 1754, 26 Sept 1802) wrote about artillery but he is best remembered for his tables of logarithms and trigonometric functions. Vega calculated π to 140 places, a record which stood for over 50 years. This appears in a paper which he published in 1789.
In September 1802 Jurij Vega was reported missing. A search was unsuccessful until his body was found in the Danube near Vienna. The official cause of death was an accident but many suspect that he was murdered. *SAU




1867 James Ferguson (31 Aug 1797, 26 Sep 1867) Scottish-American astronomer who discovered the first previously unknown asteroid to be detected from North America. He recorded it on 1 Sep 1854 at the U.S. Naval Observatory, where he worked 1848-67. This was the thirty-first of the series and is now known as 31 Euphrosyne, named after one of the Charites in Greek mythology. It is one of the largest of the main belt asteroids, between Mars and Jupiter. He was involved in some of the earliest work in micrometry was done at the old U.S. Naval Observatory at Foggy Bottom in the midst of the Civil War using a 9.6 inch refractor. He also contributed to double star astronomy. Earlier in his life he was a civil engineer, member of the Northwest Boundary Survey, and an assistant in the U.S. Coast Survey *TIS



1868 August Ferdinand Mobius (17 November 1790 – 26 September 1868) 1790 August Möbius (17 Nov 1790; 26 Sep 1868)August Ferdinand Möbius was a German astronomer, mathematician and author. He is best known for his work in analytic geometry and in topology, especially remembered as one of the discoverers of the Möbius strip, which he had discovered in 1858. A Möbius strip is a two-dimensional surface with only one side. It can be constructed in three dimensions as follows. Take a rectangular strip of paper and join the two ends of the strip together so that it has a 180 degree twist. It is now possible to start at a point A on the surface and trace out a path that passes through the point which is apparently on the other side of the surface from A. Although his most famous work is in mathematics, Möbius did publish important work on astronomy.*TIS

He discovered his famous strip in September 1858. Johann Benedict Listing discovered the same surface two months earlier.*VFR (It is somewhat amazing that we call it after Mobius when Listing discovered it first and published, and it seems, Mobius did not. However Mobius did seem to have thought on the four color theorem before Guthrie, or anyone else to my knowledge.)




1877 Hermann Günther Grassmann (15 Apr 1809, 26 Sep 1877) German mathematician chiefly remembered for his development of a general calculus of vectors in Die lineale Ausdehnungslehre, ein neuer Zweig der Mathematik (1844; "The Theory of Linear Extension, a New Branch of Mathematics"). *TIS



1910 Thorvald Nicolai Thiele (24 Dec 1838, 26 Sept 1910) He is remembered for having an interpolation formula named after him, the formula being used to obtain a rational function which agrees with a given function at any number of given points. He published this in 1909 in his book which made a major contribution to numerical analysis. He introduced cumulants (under the name of "half-invariants") in 1889, 1897, 1899, about 30 years before their rediscovery and exploitation by R A Fisher. *SAU



1976 Paul (Pál) Turán (18 August 1910, 26 September 1976) was a Hungarian mathematician who worked primarily in number theory. He had a long collaboration with fellow Hungarian mathematician Paul Erdős, lasting 46 years and resulting in 28 joint papers. *SAU

In 1940, because of his Jewish origins, he was arrested by the Nazis and sent to a labour camp in Transylvania, later being transferred several times to other camps. While imprisoned, Turán came up with some of his best theories, which he was able to publish after the war. *Wik



1978 Karl Manne Georg Siegbahn (3 Dec 1886, 26 Sep 1978) Swedish physicist who was awarded the Nobel Prize for Physics in 1924 for his discoveries and investigations in X-ray spectroscopy. In 1914 he began his studies in the new science of x-ray spectroscopy which had already established from x-ray spectra that there were two distinct 'shells' of electrons within atoms, each giving rise to groups of spectral lines, labeled 'K' and 'L'. In 1916, Siegbahn discovered a third, or 'M', series. (More were to be found later in heavier elements.) Refining his x-ray equipment and technique, he was able to significantly increase the accuracy of his determinations of spectral lines. This allowed him to make corrections to Bragg's equation for x-ray diffraction to allow for the finer details of crystal diffraction. *TIS



1990 Lothar Collatz​ (July 6, 1910, , September 26, 1990) was a German mathematician. In 1937 he posed the famous Collatz conjecture, which remains unsolved. The Collatz-Wielandt formula for positive matrices important in the Perron–Frobenius theorem is named after him. *Wik The Collatz conjeture is an iteration problem that deals with the following algorithm..
If a number n is odd, then f(n)= 3n+1
if n is even, then f(n) = 1/2 (n)
Each answer then becomes the new value to input into the function. The problem, or should I say problems, resolve around what happens to the sequence of outcomes when we keep putting the answer back into the function. For example if we begin with 15 we get the following sequence, also called the orbit of the number:
15, 46, 23, 70, 35, 106, 53, 160, 80, 40, 20, 10, 5, 16, 8, 4, 2, 1...
One of the unproven conjectures is that for any number n, the sequence will always end in the number 1. This has been shown to be true for all numbers up to just beyond 10^16. (  A recent note from Wendy Appleby at the Math Connections Group on LinkedIn updated this boundary to ~ 2.95*10^20).  A  second interesting question is how long it takes for a number to return to the value of 1. For the example above, the number 15 took 17 steps to get back to the unit value. Questions such as which three (or other n) digit number has the longest orbit. There are many variations of the problem, but if you are interested in a good introduction, check this link from Simon Fraser University"

Collatz's Problem is often also called the Syracuse Algorithm, Hasse's problem, Thwaite's problem, and Ulam's problem after people who have worked and written on the problem. It is unclear where the problem originated, as it seems to have had a long history of being passed by word of mouth before it was ever written down. It is often attributed to Lothar Collatz from the University of Hamburg who wrote about the problem as early as 1932. The name "Syracuse Problem" was applied by after H. Hasse, an associate of Collatz, visited and discussed the problem at Syracuse University in the 1950's. During the 1960's Stan Ulam circulated the problem at Los Alamos laboratory. One famous quote about the problem is from Paul Erdos who stated, "mathematics is not yet ready for such problems". *Personal 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

# 7 Absolute value/difference,… from old math term history notes

    Absolute Value The word absolute is from a variant of absolve and has a meaning related to free from restriction or condition. The first use of "absolute value" in English seems to have been to apply to real values. Jeff Miller's website on the Earliest Known Uses of Some of the Words of Mathematics says," Absolute value is found in English in 1850 in The elements of analytical geometry; comprehending the doctrine of the conic sections, and the general theory of curves and surfaces of the second order by John Radford Young (1799-1885): "we have AF the positive value of x equal to BA - BF, and for the negative value, BF must exceed BA, that is, F must be on the other side of A, as at F', hence making AF' equal to the absolute value of the negative root of the equation" [University of Michigan Digital Library]." [See the page here] In 1876 Karl Weierstrass applied the term to magnitude of complex numbers. From Miller's site again we find "Absolute value was coined in German as absoluten Betrag by Karl Weierstrass (1815-1897), who wrote:

Ich bezeichne den absoluten Betrag einer complex Groesse x mit |x|. [I denote the absolute value of complex number x by |x|.]"

In "The Words of Mathematics", Steven Schwartzman suggests that the use of the word for real values only became common in the middle of the 20th century. This may be true, but the use for signed numbers also appears in 1889 by Wentworth according to Miller; "In 1889, Elements of Algebra by G. A. Wentworth has: 'Every algebraic number, as +4 or -4, consists of a sign + or - and the absolute value of the number; in this case 4.' " (above). In the 1893 edition of the same book he uses the term again, as shown below, without any symbol.

The revision of Hall and Knight's Algebra, for Colleges and Schools {"Revised and Enlarged for the use of American Schools"} by F. L. Sevenoak in 1905 also uses the term without a sign. By 1934, the word is still used without symbol in Walter W. Hart's Progressive First Algebra,(pg 78), but in the 1939 edition of College Algebra by Rosenbach and Whitman, the symbol is used as shown below

The symbol for absolute value is usually a pair of vertical lines containing the number, as created by Weierstrass in 1876 (see above). |3| is read as "The absolute value of three". The absolute value of a real number is its distance from zero, so |3| = |-3| = 3. In words that says that the absolute value of three is equal to the absolute value of -3 , and that both have a value of three.

For complex numbers the absolute value is also called magnitude or length of the complex number. Complex numbers are sometimes drawn as a vector using an Argand Diagram, and the length of the vector Z=a+bi is |a+bi|. Stated another way, the value of |a+bi|= 

A symbol for the Absolute Difference of two numbers, or the absolute value of the difference was created by Oughtred around 1630. Miller writes, "The tilde was introduced for this purpose by William Oughtred (1574-1660) in the Clavis Mathematicae (Key to Mathematics), composed about 1628 and published in London in 1631, according to Smith, who shows a reversed tilde (Smith 1958, page 394)." This seems no longer to be common in basic maths classes in England today (current coments anyone?). After posting a request for information to the Historia Matematica discussion group about the use of the tilde to indicate absolute difference in England I received the following update from Herbert Prinz:

"In modern English texts on navigation, nautical astronomy or its history, the tilde,~, is frequently used to express the function | a - b |, where |x| stands for absolute value. E. g. Cotter, The Complete Nautical Astronomer, 1969. I am not sure when this practice started. In older texts on the same subject, say, Moore, The Practical Navigator, 1800, one does not find the tilde used in this way. For one, because instructions were given mostly verbally without the use of any symbols at all. And second, the distinction from '-' was unnecessary, as it was always understood, if not explicitly stated, that one must subtract the smaller.  While talking about symbols, I should add that shortly after Robert Recorde began using the equal sign, =, now common, Viete used the same symbol for the absolute difference between two numbers.   

 

In England the absolute value is often referred to as the modulus function, and the two bars that make up the symbol are sometimes called "modulus signs" according to a note posted by Vicky Neale on the Ask NRich math site. The term modulus is used both in America and England to represent the magnitude or length of a complex number. The term is also used in a number of other specialty ways in mathematics, the best known being the "congruence modulus". The modulus of a congruence, often shortened to "mod" is the base value with which the congruence is computed. We say A is Congruent to B modulus C, if A divided by C and B divided by C have the same remainder. C is called the modulus of congruence. It would be written A≡B [mod C]

Modulus comes almost unchanged from the Latin from the diminutive of modus (measure or amount), modulus for a small measure. Vicky also pointed out that at one time the term was used for, "A unit of payment used at Trinity College.... Fellows received some number of moduli". Ms Neale also said she was unfamiliar with the use of the ~ for absolute difference.

It was Gauss, Disquisitiones arithmeticae in 1801, who introduced the term modulus of congruence, and the abreviation, "mod". Cajori credits Jean Argand for the first use of modulus for the length of a vector in 1814. I am not sure when the British public schools started to use the term for the absolute value of a number, and would love to know if someone has old books with these terms (or others for the same idea).

Thursday, 24 September 2026

On This Day in Math - September 25

 

"


I am undecided whether or not the Milky Way​ is but one of countless others all of which form an entire system. Perhaps the light from these infinitely distant galaxies is so faint that we cannot see them.

~ Johann H Lambert

This is the 268th day of the year, 268 is the smallest number whose product of digits is 6 times the sum of its digits. (A good classroom exploration might be to find numbers in which the product of the digits is n x the sum of the digits for various values of n.. more generally, for what percentage of numbers is the sum a factor of the product at all?)

The two odd numbers adjacent to 6*268 form a pair of twin primes, and the next two odd numbers after 268 are a pair of twin primes. And the 268th prime, is the smaller of a pair of twin primes.

268 is the sum of two consecutive primes, 268 = 131 + 137

Prime Curios offers this little mental conversion, 268 inches of 1/8 inch copper wire weighs 1 pound. There is no AWG standard gauge wire that is 1/8 of an inch diameter, but AWG 8 is really close. For students, what would a similar length of 1/4 inch diameter copper wire weigh?

Many people know that N! has N digits for N= 22, 23, and 24.  Surprisingly, to me, there are also three consecutive numbers for which N! has 2N digits, 266, 267, and 268.  For N! has 3N digits, only two consecutive numbers, 2712 and 2713.For N! having 4N digits, there are again two consecutive  occurrences,  27175 and 27176. For 5N we go back to three consecutive digits,  271819, 271820, 271821  Note the increase by a power of ten as a limit, and the higher you go, the closer they approach  e * 10^n. It has been conjectured that there are always at two or three consecutive numbers for every digit, but never more. The first 100 such numbers are found at A058814 - OEIS Thanks to Derek Orr and Frank Kampas for some help and direction on this. 


EVENTS


1493 Columbus set sail on his second voyage to America.


303  On Sept. 25, 303 C.E. bishop-martyr St. Fermin (b. 272) is beheaded in Amiens, France; starting in in 1591 the San Fermin Festival in Pamplona, Spain is founded, featuring eight 3/4-ton bulls chasing drunken revelers down a 900-yard cobblestone street corridor; originally held on Sept. 25, it begins running from noon on July 6 to midnight on July 14 starting in 1592; by the 20th cent. there are eight bull runs during the 9-day festival, one each morning at 8 a.m. - advice: stay in front? *HistoryScoper



1513 On September 25th, 1513, Vasco Nunez de Balboa crossed the Isthmus of Panama and first sighted the Pacific Ocean (it would take four days for his group to work their way down the mountain to the ocean.. Balboa was accompanied by 190 Spaniards and several hundred slaves. His "discovery" spurred those looking for a passage to the Pacific. Balboa spent a number of months exploring the West Coast of Central America. Within six years he would be found guilty of treason and beheaded by rivals for his supposed "river of gold".



1608 The oldest written mention of the telescope: In a letter of introduction from the Council of Zeeland to Zeeland’s Delegates to the States General (the Netherlands parliament) in Den Haag asking them to organise an audience with Prince Maurice of Nassau for a spectacle maker from Middelburg who had invented a “…certain device by means of which all things at a very great distance can be seen as if they were nearby, by looking through glasses…”; the oldest written mention of the telescope. On an unknown day between 25th and 29th September: Hans Lipperhey (1570 – 1619) the spectacle maker from Middelburg (who was actually a German from Wesel) demonstrates his new invention at the court of Prince Maurice, where a peace conference in the Dutch-Spanish War is taking place along with the first visit to Europe of the Ambassador of Siam. Lipperhey’s demonstration is described in detail in a French flyer describing the Ambassadors visit and the news of the new invention is thus spread rapidly throughout Europe.

26th July 1609 Julian calendar (5th August 1609 Gregorian calendar): Thomas Harriot (1560 – 1621) makes a sketch of the moon using a telescope.

21st August 1609: Galileo demonstrates his telescope to the aristocrats of Venice.

24th August 1609: Galileo presents his telescope to the Doge and Senate of Venice.

25th August 1609: Galileo is granted a lifetime contract as professor for mathematics at the University of Padua with a salary of 1000 Florins but with the subsidiary clause that he would never receive a raise in salary.

When Galileo first used a telescope as an astronomical instrument is not known but it was at least a couple of months later.

It is highly probable that Simon Marius (1573 – 1624) court astronomer in Ansbach Franconia used a telescope as an astronomical instrument before Galileo but it is not possible to determine when.

7th January 1610: Galileo discovers the first three moons of Jupiter.

8th January 1610: Marius discovers the first three moons of Jupiter independently of Galileo. *Renaissance Mathematicus,


Lipperhey’s Patent Application





1654 Fermat writes to Pascal defending his combinatorial method that Pascal had previously regarded as incorrect.*VFR In the same letter he announced the following two results for odd primes expanding his sums of two primes Christmas letter to Fr Mersenne from 14 years earlier:

p = X2 + 2y2 Iff p is equivalent to 1 or 3 mod 8,  {3, 11, 17, 43,...}

p = X2 + 3y2 Iff p is equivalent to 1 mod 3 {4, 7, 13, 19, ...}  


His statue is in the town named for him, Descartes.  It is located 48 mikes away and is on  the same Creuse River my part time French home in Argenton-sur-creuse overlooks.  Originally called Le Haye, the name was changed to Le Haye-Descartes (1802), then later to Descartes (1967).  It is also the birthplace of Pierre Ballue (a common spelling of my last name).  

His family home was nearby in Chatellerault, and he left La Haye in 1606 (about age ten) to attend the college of Henry IV at La Fleche.  Then in about 1615-16 he attended the University of Poitiers ro become a lawyer as his father's wishes.  From there to Paris,  And soon he departed France and spent almost all of the rest of his life in the Dutch Republic, and then in Sweden where he died.


Beautiful Argenton on the Creuse, phot from my study,





1820 Arago announces electromagnetism ... Francois Arago announced that a copper wire between the poles of a voltaic cell, could laterally attract iron filings to itself (Ann. de Chim. et de Physique., xv. p.93). His discovery came in the same year that Oersted discovered that an electric current flowing in a wire would deflect a neighboring compass needle. Arago in the same publication described how he had successfully succeeded in causing permanent magnetism in steel needles laid at right angles to the copper wire. Arago and André-Marie Ampère, discussed and experimented with forming the copper wire into a helix to intensify the magnetizing action. However, it was not until 1825 that the electromagnet in its familiar form was invented by William Sturgeon. *TIS




1938  A brief story in The Oregonian of Portland, Oregon:  "Charles Keville walked into the temporary morgue and looked at a body that had been identified as his."
" 'Nope,' he said,  'That ain't me', and walked out again."  *
Dudes Posting Their W’s

1944 Denmark issued a stamp commemorating the 300th anniversary of the birth of Ole Roemer,*VFR
Danish astronomer who, in 1676, first demonstrated that light travels at a finite speed. Rømer also invented the modern thermometer showing the temperature between two fixed points, namely the points at which water respectively boils and freezes.

Rømer made his discovery regarding the speed of light while working at the Royal Observatory in Paris and studying Jupiter's moon Io. He estimated that light takes about 11 minutes to travel from the Sun to Earth. Using today's knowledge of the Sun-Earth distance, this would amount to a speed of light of approximately 220,000 kilometers per second, compared to today's accepted value of just under 300,000 kilometers per second.

In scientific literature, alternative spellings such as "Roemer", "Römer", or "Romer" are common.


1960 NEW MATH. New mathematics is found in Time magazine of Feb. 3, 1958, in the heading, "The new mathematics" [OED].
New math is found again in an article which appeared in numerous newspapers on Sept. 25, 1960: “But the ‘new math’ is being promoted energetically by such influential bodies as the U. S. Office of Education, the National Science Foundation, the National Education Association, the Mathematical Association of America, the College Entrance Examination Board and the Carnegie Corporation.”
* Jeff Niller
cartoon about parental confusion during "New Math" introduction.  "In the words of the great Tom Leher, "Math so easy that only a child could do it."




On this day in 1988, Faà di Bruno was beatified by Pope John Paul II in St Peter's Square in Rome.   is best known for his formula for the nth derivative of a composition of functions. Faà di Bruno's formula is an identity in mathematics generalizing the chain rule to higher derivatives. It is named after Francesco Faà di Bruno (1855, 1857), although he was not the first to state or prove the formula.  In 1800, more than 50 years before Faà di Bruno, the French mathematician Louis François Antoine Arbogast had stated the formula in a calculus textbook, which is considered to be the first published reference on the subject.  
#SAU 





1989 IBM announces plans to develop a new design for transmitting information within a computer, called Micro Channel Architecture, which it said could transfer data at 160 million bytes per second or eight times faster than the fastest speed at the time. Although IBM was hoping to make its system the industry standard, manufacturers of IBM-compatible computers largely chose other methods. *CHM

*CHM





BIRTHS

1644 Olaus Roemer, Danish astronomer, born. He was the first to measure the speed of light. *VFR (25 Sep 1644;23 Sep 1710) Astronomer who demonstrated conclusively that light travels at a finite speed. He measured the speed by precisely measuring the length of time between eclipses of Jupiter by one of its moons. This observation produces different results depending on the position of the earth in its orbit around the sun. He reasoned that meant light took longer to travel the greater distance when earth was traveling in its orbit away from Jupiter.*TIS "Ole Rømer took part in several other achievements considering measurement. He developed a temperature scale that is now famous as the Fahrenheit scale. Fahrenheit improved and distributed his ideas after visiting Rømer. In his last years, he was even given the position as second Chief of the Copenhagen Police and invented the first street oil lamps in the city of Copenhagen.
Further achievements and inventions may be added to Rømer's biography, like his innovative water supply system and his urban planning concept. " *Yovista.blogspot






1819 George Salmon (25 September 1819 – 22 January 1904) made many discoveries about ruled surfaces and other surfaces. *SAU His publications in algebraic geometry were widely read in the second half of the 19th century. A Treatise on Conic Sections remained in print for over fifty years, going though five updated editions in English, and was translated into German, French and Italian. *Wik
Salmon statue at Trinity College, Dublin
*MacTutor, SAU




1825 Carl Harald Cramer,(25 September 1893 ,5 October 1985) was a Swedish mathematical statisticians and is one of the prominent figures in the statistical theory. He was once described by John Kingman as "one of the giants of statistical theory". 
In number theory, Cramér's conjecture,in 1936 states that
p_{n+1}-p_n=O((\log p_n)^2),\
where pn denotes the nth prime number, O is big O notation, and "log" is the natural logarithm. Intuitively, this means the gaps between consecutive primes are always small, and it quantifies asymptotically just how small they can be. This conjecture has not been proven or disproven.
*Wik
Big O notation is a mathematical notation that describes the limiting behavior of a function when the argument tends towards a particular value or infinity.


1846 Wladimir (Peter) Köppen (25 Sep 1846; 22 Jun 1940) German meteorologist and climatologist best known for his delineation and mapping of the climatic regions of the world. He played a major role in the advancement of climatology and meteorology for more than 70 years. The climate classification system he developed remains popular because it uses easily obtained data (monthly mean temperatures and precipitation) and straightforward, objective criteria. He recognized five principal climate groups: (A) Humid tropical -winterless climates; (B) Dry - evaporation constantly exceed precipitation; (C) humid mid-latitude, mild winters; (D) humid mid-latitude, severe winters; and (E) Polar - summerless climates. *TIS




1857 Sergey Petrovich Degayev (also spelled Degaev; Russian: Серге́й Петрович Дегаев; 1857 in Moscow – 1921 in Bryn Mawr, Pennsylvania) was a Russian revolutionary terrorist, Okhrana agent, and the murderer of inspector of secret police Georgy Sudeykin. After emigrating to the United States, Degayev took the name Alexander Pell and became a prominent American mathematician, the founder of school of Engineering at the University of South Dakota. The Dr. Alexander Pell scholarship is named in his honor.

After December 1883, all the posts in the Empire were plastered with posters showing Degayev's photographs and announcing 5000 roubles for information as to his whereabouts and 10,000 roubles for help in catching him. Still the conspirators had a good lead on their hunters and successfully arrived in Paris. At a winter 1884 meeting, Narodnaya Volya, led by V. A. Karaulov, Lev Tikhomirov and German Lopatin, fulfilled its end of the bargain and granted Degayev his life on the condition that he never again appear in the Russian Empire. Lev Tikhomirov personally verified that he boarded a steamship bound for South America.
From South America Degayev moved to the United States; there he joined his wife, Lyubov Degayeva. His brother, Vladimir Degayev, who worked at the time in a Russian consulate in the United States and moonlighted as a foreign correspondent for a few Russian publications printed an article claiming that Sergey Degayev was killed in New Zealand, discouraging searches for him by both Russian police and Russian revolutionaries.

Both Vladimir and Sergey Degayevs were registered in the USA under the name Polevoi after their maternal grandfather Nikolai Polevoy. After his naturalization Alexander (Sergey) took the name Alexander Pell and his wife took the name Emma Pell. At first they were poor; Sergey worked as a stevedore and as an unskilled labourer while his wife worked as a cook and a laundress. In 1895 Alexander was enrolled into a PhD program in Johns Hopkins University with majors in mathematics and astronomy and a minor in English. During his study he was financially supported by his wife who continued to work as a cook. He received his doctorate in 1897 for the dissertation On the Focal surfaces of the Congruences of Tangents to a Given Surface.

The University of South Dakota was established in the frontier town of Vermillion and started its classes in 1882. In 1897 they decided that they needed a professor of mathematics. They asked Professor L. S. Hulburt from Johns Hopkins if he could suggest a suitable candidate. He replied that he "could suggest a first class mathematician who had the disadvantage of having a strong Russian brogue". The reply from South Dakota was "Send your Russian mathematician along, brogue and all".


Alexander Pell (Sergey Degayev) and Emma Pell (Lyubov Degayeva), South Dakota
Alexander Pell was immensely popular among his students who referred to him as the "class father" and "Jolly Little Pell" (who could "crack jokes faster than the freshmen could crack nuts"). He was a good researcher, a member of the American Mathematical Society and the author of many journal publications. He was also an accomplished administrator who organized the School of Engineering of the University of South Dakota and became its first Dean (1905).

Alexander Pell had a habit of providing financial support from his own resources, and providing accommodation in his house to a few of his students. One such student was Anna Johnson, the future accomplished mathematician Anna Johnson Pell Wheeler. Anna Johnson received her A.B. degree under Pell's supervision in 1903 and continued her study at the University of Iowa and then at the University of Göttingen. In 1904 Emma Pell died. 
Three years later Alexander Pell went to Göttingen and married Anna in July 1907. They both returned to Vermillion where Anna taught classes in the theory of functions and differential equations and Alexander was the Dean of Engineering. In 1908 Pell resigned from the University of South Dakota and went with Anna to Chicago. There Anna completed her doctorate under E. H. Moore, while Pell took a position at the Armour Institute of Engineering (currently Illinois Institute of Technology). In 1911 Pell suffered a stroke and was unable to work thereafter. The same year the Pells moved to South Hadley, Massachusetts where Anna taught at Mount Holyoke College. In 1918 they moved again to Bryn Mawr, Pennsylvania where Anna taught at Bryn Mawr College. Alexander Pell died in Bryn Mawr in 1921.

Alexander Pell (Sergey Degayev) and Emma Pell (Lyubov Degayeva), South Dakota




1888 Stefan Mazurkiewicz (25 Sept 1888 , 19 June 1945) His main work was in topology and the theory of probability. His notion of dimension of a compact set preceded that of Menger and Urysohn by seven years. Mazurkiewicz applied topological methods to the theory of functions, obtaining powerful results. His theory gave particularly strong results when applied to the Euclidean plane, giving deep knowledge of its topological structure. *SAU



1992 Lisa Sauermann (born 25 September 1992) is a German mathematician known for her performance in the International Mathematical Olympiad, where in 2011 she had the single highest (and perfect) score. She won four gold medals (2008–2011) and one silver medal (2007) at the olympiad, representing Germany.

Sauermann attended Martin-Andersen-Nexö-Gymnasium Dresden when she was in 12th grade. She won the Franz Ludwig Gehe Prize in 2011 and the gold medal in the age group III, the 11th–12th grade competition. As a result, she won a trip to the Royal Academy of Sciences in Stockholm. To achieve this, she presented a new mathematical theorem with a proof in a work entitled "Forests with Hypergraphs".

In 2011 she began studying mathematics at the University of Bonn. In 2014, she completed her bachelor thesis on algebraic geometry under Michael Rapoport. She became a graduate student studying with Jacob Fox at Stanford University where she obtained her PhD in 2019, receiving two prizes for her dissertation titled "Modern Methods in Extremal Combinatorics". After her graduation she worked as an assistant professor at Stanford before spending a year at the Institute for Advanced Study in Princeton. In 2021 became an assistant professor at MIT and received the European Prize in Combinatorics at Eurocomb for her work in combinatorics. In 2023 she accepted a tenured professorship at University of Bonn, where she currently works,  her main field of work as of 2023 being probabilistic combinatorics. In 2022, she was awarded a Sloan fellowship, and in 2023, she received the von Kaven Award.

Her sister, Anne, two years her junior, was a successful participant in math and science Olympiads at the national level. *Wik








DEATHS

1777 Johann Heinrich Lambert (26 Aug 1728, 25 Sep 1777) Swiss-German mathematician, astronomer, physicist, and philosopher who provided the first rigorous proof that pi ( the ratio of a circle's circumference to its diameter) is irrational, meaning it cannot be expressed as the quotient of two integers. He also devised a method of measuring light intensity. *TIS In 1766 Lambert wrote Theorie der Parallellinien which was a study of the parallel postulate. By assuming that the parallel postulate was false, he managed to deduce a large number of non-euclidean results. He noticed that in this new geometry the sum of the angles of a triangle increases as its area decreases. *SAU
Lambert devised a formula for the relationship between the angles and the area of hyperbolic triangles. These are triangles drawn on a concave surface, as on a saddle, instead of the usual flat Euclidean surface. Lambert showed that the angles added up to less than π (radians), or 180°. The amount of shortfall, called the defect, increases with the area. The larger the triangle's area, the smaller the sum of the angles and hence the larger the defect C△ = π — (α + β + γ). 
Lambert solves a geometrical problem, viz. to reconstruct the course of a ship at sea on the basis of observations with a plane table on the shore. The problem is originally in Marinoni's De Re Ichnographica (1751), which Lambert read early on (1752). Lambert here reduces this problem (the most complicated one in Marinoni) using algebraic methods. Since many observations have to be reduced to solve the problem, these studies constitute one of the starting points for Lambert's work on the theory of errors.

Lambert is a curious historical figure; extremely accomplished, a worthy member of a select company that includes Leonard Euler and Immanuel Kant, except that hardly anyone has ever heard of Lambert, save the optician who measures the luminance of a light source in lamberts, or the cartographer who produces an aviation map using the Lambert conical projection, or the astrophysicist who measures the albedo of a moon of Saturn, using a term for reflectivity that was coined by Lambert. Lambert spent the last 13 years of his working life in Berlin, where he was appointed a member of the Academy of Sciences there. He wrote original works on pyrometry (the measure of heat), photometry (the measure of luminance), hygrometry (measurement of humidity), cartographic projections (he invented 7 new projections, several still in common use), even treatises on non-Euclidean geometry and irrational numbers. *Linda Hall Org


*Wik






1852 Christoph Gudermann (March 25, 1798, September 25, 1852) was born in Vienenburg. He was the son of a school teacher and became a teacher himself after studying at the University of Göttingen, where his advisor was Karl Friedrich Gauss. He began his teaching career in Kleve and then transferred to a school in Münster.
He is most known today for being the teacher of Karl Weierstrass, who took Gudermann's course in elliptic functions, 1839–1840, the first to be taught in any institute. Weierstrass was greatly influenced by this course, which marked the direction of his own research.
Gudermann originated the concept of uniform convergence, in an 1838 paper on elliptic functions, but only observed it informally, neither formalizing it nor using it in his proofs. Instead, Weierstrass elaborated and applied uniform convergence.
His researches into spherical geometry and special functions focused on particular cases, so that he did not receive the credit given to those who published more general works. The Gudermannian function, or hyperbolic amplitude, is named after him.Gudermann died in Münster. *Wik




1877 Urbain-Jean-Joseph Le Verrier (11 May 1811, 25 Sep 1877) French astronomer who predicted the position of a previously unknown planet, Neptune, by the disturbance it caused in the orbit of Uranus. In 1856, the German astronomer Johan G. Galle discovered Neptune after only an hour of searching, within one degree of the position that had been computed by Le Verrier, who had asked him to look for it there. In this way Le Verrier gave the most striking confirmation of the theory of gravitation propounded by Newton. Le Verrier also initiated the meteorological service for France, especially the weather warnings for seaports. *TIS (He died the day after the anniversary of the sighting of his most famous prediction. Between that moment of fame in 1846 and his death, he mistakenly attributed the variability of Mercury's orbit to another small planet he named "Vulcan". It took the theory of General Relativity to explain the variations. He was buried in Montparnasse cemetery in Paris. A large globe sits atop grave. Arago described him as, "the man who discovered a planet with the point of his pen."

1933 Paul Ehrenfest (January 18, 1880, September 25, 1933) was an Austrian and Dutch physicist and mathematician, who made major contributions to the field of statistical mechanics and its relations with quantum mechanics, including the theory of phase transition and the Ehrenfest theorem.
He befriended Albert Einstein on a visit to Prague in 1912 and became a professor in Leiden, where he frequently hosted Einstein. Suffering from depression, in 1933 Ehrenfest killed his disabled son, Wassik, and then himself. 
On 21 December 1904, he married Tatyana Afanasyeva, who collaborated with him in his work. They had two daughters and two sons: Tatyana ('Tanja') (1905–1984) also became a mathematician; Galinka ('Galja') (1910–1979) became an author and illustrator of children's books; Paul, Jr. ('Pavlik') (1915–1939) became a physicist; and Vassily ('Wassik') (1918–1933).
*Wik

Paul, and his wife Tatyana, a Russian-Dutch mathematician and physicist who made contributions to the fields of statistical mechanics and statistical thermodynamics with her husband Paul Ehrenfest.






1955  Franz Rellich (September 14, 1906 – September 25, 1955) was an Austrian-German mathematician. He made important contributions in mathematical physics, in particular for the foundations of quantum mechanics and for the theory of partial differential equations. The Rellich–Kondrachov theorem is named after him.
Among Rellich's most important mathematical contributions are his work in the perturbation theory of linear operators on Hilbert spaces: he studied the dependence of the spectral family 
Although the origins and applications of the problem are in quantum mechanics, Rellich's approach was completely abstract.

Rellich successfully worked on many partial differential equations with degeneracies. For instance, he showed that in the elliptic case, the Monge-Ampère differential equation, while not necessarily uniquely soluble, can have at most two solutions.

Particularly relevant to physics was Rellich's mathematical clarification of the outgoing Sommerfeld conditions.

When in 1933 the great mathematical-physical tradition in Göttingen terminated with the Machtergreifung of the Nazis, Rellich, having taken an active position against Nazism, was among those forced to leave. In 1934 he became Privatdozent in Marburg, in 1942 professor in Dresden, and in 1946 director of the Mathematical Institute in Göttingen, being instrumental in its reconstruction. Heinz Otto Cordes, Erhard Heinz, Konrad Jörgens, and Jürgen Moser were among of his doctoral students. His sister Camilla Juliana Anna was the wife of mathematician Bartel Leendert van der Waerden. Rellich died in Göttingen. *Wik


2021 Joachim Neubüser ( June 18 , 1932 in Belgard , Pomerania ; September 25 , 2021 in Aachen ) was a German mathematician who was primarily concerned with group theory and was a professor at RWTH Aachen .

Neubüser studied at the University of Kiel from 1951 , passing his state examination in 1957 and receiving his doctorate under Wolfgang Gaschütz in 1957 (On homogeneous groups). As a postdoctoral researcher, he was at the University of Manchester in 1957/58 and from 1958 an assistant in Kiel. After receiving his habilitation in 1967 (The subgroup associations of groups of order ≤ 100 with the exception of orders 64 and 96), he was a senior lecturer in Kiel and from 1969 a full professor at RWTH Aachen University (Chair D). He retired in 1997.

He worked primarily in the field of algorithmic group theory and developed programs for this area from the 1960s onwards. In 1986, he initiated the computer algebra system GAP  with algorithms for group theory, and previously, in 1981, the CAS system (Character Algorithm System) for calculations involving group characters. He also dealt with space groups . With Hans Zassenhaus and others, he classified crystallographic groups in four dimensions.

His doctoral students included Wilhelm Plesken , Rolf Bülow and Volkmar Felsch. *Wik





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