Wednesday, 11 November 2026

The Father of ovariotomy

Ephraim McDowell (November 11, 1771 – June 25, 1830) was an American physician and pioneer surgeon. The first person to successfully remove an ovarian tumor, he has been called "the father of ovariotomy" as well as founding father of abdominal surgery.



McDowell was born in Rockbridge County, Virginia, the ninth child of Samuel and Mary McDowell. His father was a veteran of the French and Indian War and a colonel during the American Revolution. In 1784 Samuel McDowell was appointed land commissioner and moved his family to Danville, Kentucky. There, he presided over ten conventions that resulted in the drafting of the Kentucky Constitution.[4][page needed] Samuel was the 2nd great-grandfather of First Lady Mary Todd Lincoln, making her Ephraim McDowell's great-grandniece.

McDowell received his early education at the classical seminary of Worley and James, then spent three years as a medical student under Dr. Alexander Humphreys in Staunton, Virginia. He attended lectures in medicine at the University of Edinburgh, Scotland, from 1793 to 1794 and studied privately with John Bell. He never received a diploma, but in 1825, the University of Maryland conferred on him an honorary M.D. degree.

In 1795, McDowell returned from Scotland, settled in Danville, Kentucky, and began his practice as a surgeon. McDowell perfected the modern surgical technique of lithotomy for removal of stones obstructing the urinary bladder. One of his most famous patients was James K. Polk, for whom he removed a urinary stone and repaired a hernia.

On December 13, 1809, McDowell was called to see Jane Todd Crawford in Green County, Kentucky, 60 miles from Danville. Her physicians thought that Mrs. Crawford was beyond term pregnant. McDowell diagnosed an ovarian tumor. Mrs. Crawford begged him to keep her from a slow and painful death. He then described her condition and that an operation for cure had never been performed. He said that the best surgeons in the world thought it impossible. Mrs.Crawford said she understood and wanted to proceed. McDowell told her he would remove the tumor if she would travel to his home in Danville. She agreed and rode the 60 miles on horseback.

On Christmas morning, 1809, McDowell began his operation. The surgery was performed without benefit of anesthetic or antisepsis, neither of which was then known to the medical profession. The tumor McDowell removed weighed 22.5 pounds (10.2 kg). He determined that it would be difficult to remove completely, so he tied a ligature around the fallopian tube near the uterus and cut open the tumor. He described the tumor as the ovarium and fimbrious part of the fallopian tube that was very much enlarged. The whole procedure took 25 minutes. Crawford made an uncomplicated recovery. She returned to her home in Green County 25 days after the operation and lived another 32 years. This was the first successful removal of an ovarian tumor in the world.

All attempts at abdominal exploration before 1809 had resulted in peritonitis and death. Descriptions of McDowell include phrases like "neat and clean" or "scrupulously clean." He was not only neat, but meticulous. In his report on the operation, he described the removal of blood from the peritoneal cavity and bathing the intestines with warm water. 

McDowell did not publish a description of his procedure until 1817, after he had performed two more such operations. This was widely criticized in the English surgical literature. There is evidence that he performed at least 12 operations for ovarian pathology.

"Having never seen so large a substance extracted, nor heard of an attempt, or success attending any operation such as this required, I gave to the unhappy woman information of her dangerous situation. The tumor appeared full in view, but was so large we could not take it away entire. We took out fifteen pounds of a dirty, gelatinous looking substance. After which we cut through the fallopian tube, and extracted the sac, which weighed seven pounds and one half. In five days I visited her, and much to my astonishment found her making up her bed." 

From 1809 and 1818, McDowell wrote about four separate ovariotomies following Crawford's. All four were performed on enslaved women, three of whom survived and one of whom died. It is unclear whether the enslaved women he performed surgeries on gave consent or received sufficient time to recover following the procedure.

A commemorative stamp honoring Ephraim McDowell, was issued December 3, 1959, the 150th anniversary of successful ovarian operation


In 1802, McDowell married Sarah Shelby, daughter of war hero and two-time Kentucky governor Isaac Shelby. They had two sons and four daughters. 

McDowell played a prominent role in his community. He was also a founder, original corporator, and member of the primary board of trustees of Centre College in Danville. McDowell became a member of the Philadelphia Medical Society in 1817. McDowell was the great-great-grandfather of General John Campbell Greenway, whose statue was placed in the National Statuary Hall Collection by the state of Arizona in 1930. He was cousin to woman's suffrage leader Madeline McDowell Breckinridge.


McDowell was a Presbyterian but became an Episcopalian and founded Trinity Episcopal Church in Danville, Kentucky, having donated the land for its first building.

0, McDowell was stricken with an acute attack of violent pain, nausea, and fever. He died on June 25, most likely a victim of appendicitis. His wife died 18 years later. They were buried at "Traveller's Rest", the homestead of Isaac Shelby, south of Danville, Kentucky but were reinterred in 1879, near a monument dedicated to him in Danville.

In 1879, a monument in his honor was erected by the Medical Society of Kentucky in Danville.

In 1929, Isaac Wolfe Bernheim donated a bronze statue of McDowell by Charles Henry Niehaus to the state of Kentucky for placement in the U.S. Capitol's National Statuary Hall Collection. The statue depicts the ovarian tumor that McDowell removed from Jane Crawford, sitting in a bowl on the table behind McDowell. An identical statue by the same artist stands in the rotunda of the Kentucky State Capitol in Frankfort, Kentucky. *Wik


I have live back to back with Jerry and Martha (McDowell) Hinton for 16 years.  Two incredible people who seemed to be best friends with everyone in Western Kentucky. Today while having an art day in my wife, Jeannie's studio, she shared the early details of this post .  It is hard to believe that any of his decedents could better represent the character and civility of Ephraim McDowell than his third great grand niece.


More on Surprisingly Constant

    As I mentioned before, I'm re-posting some of the most popular blogs of recent years.  This one, "Surprisingly Constant" was from 2010, but I've added a bit at the end from the amazing graphics mathematical posts of "3Blue 1 Brown."

Some things never change... and some of the things that don’t change are pretty remarkable. I was recently reminded of two that always seemed non-intuitive, and therefore quite pleasing. Both of these can be proved toward the end of a first year calculus course, and at least one can be explained with a little hand-waving, by a good pre-calc student.

The first is the simple fact that if you take a slice a sphere with a pair of parallel planes that are some distance, d, apart; the surface area of the part of the sphere between those planes is the same no matter where the slices are made. Near the “poles” or near the “equator”, the area is the same. It is nice to be able to tell students that this incredibly interesting fact was known to Archimedes in the first Century of the modern era when he proved that the surface area of a sphere is the same as the lateral area of a cylinder that contains the sphere.

This image is part of an explanation provided at a math site at the University of Regina

The essence of the explanation uses nothing beyond similar triangles. If we approximate the sphere’s surface between the slicing planes as a frustum of a cone, then the slant height (AP) can be shown to be in the same proportion to the height (AB)as the radius of the frustum (QP) is to the radius of the sphere(KP)). This image is also from the U Regina site mentioned above.Another nice thing about this relation is that when you set up the rather fearsome looking integral for the surface area, it reduces through simple algebra to a constant.

For a different look at this with some beautiful graphics, as well as several nice explanations of why the formula for the surface area of a sphere is four times the area of a circle, see this 3Blue, 1Brown video on YouTube.




The second similarly interesting idea is about the volume of a shape I call a bead, for lack of a more precise term. The bead is the solid remaining when you drill through the center of a sphere.The unexpected constant here is that for any radius sphere you start with, the volume of the bead depends only on the height. And perhaps even less expected, is that the volume is the same as the volume of an un-drilled sphere with the same height (i.e., when 2r = h).

I have found a beautiful non-calculus proof of this using an idea from Mamikon Mnatsakanian work with his visual geometry.

On This Day in Math - November 11

   





The British Mathematical Colloquium consists of three days of mathematics
with no dogs and no wives.
~Henry Whitehead

The 315th day of the year; 3152 can be written as the sum of the cubes of five consecutive integers. Find them. (Students may also wish to find the smallest square that can be expressed as the sum of the cubes of two or more consecutive integers.)

315 = 3^2 x 5 x 7  (or 5 x 7 x 9)  In a variation of use of Vandermonde's (and others since) "rising factorials" and "falling factorials" I have adopted the symbol \(9!_(2}\)  for 9x7x5x3x1; and \(9!_(2,3}\) for 9 x 7 x 5.  stopping after three terms.   

315 is a (barely)deficient number, the sum of it's proper divisors is only 309 ...309/315 is about .9809 *Derek Orr @Derektionary  pointed out to me that 256 is the closet to one of any (non-perfect) year day, (255/256 = .996), and for non-powers of two, 136 with a ratio of 134/136 = .985 is the best.


EVENTS
1572 Tycho Brahe first observed a supernova in the constellation Cassiopeia. Cornelius Gemma, the son of Gemma Frisius, made the first recorded observation of it on 9 November. Cornelius, Tycho, and others all observed the nova and determined it to be superlunary, thereby signalling a change in the superlunar sphere contradicting Aristotelian cosmology. *RMAT
(Brahe was at the beginning of his career in 1572, and it was this supernova that inspired him to devote his lifetime to making accurate measurements of the positions of the stars and planets.) For two weeks it was brighter than any other star in the sky and visible in daytime. By month's end, it began to fade but it remained visible to the naked eye for about 16 months until Mar 1574. *TIS  



1619 During the night, while living in Neuberg on the Danube, Descartes had a dream that he was visited by the Angel of Truth who revealed to him that mathematics was the sole key needed to unlock the secrets of nature. *Sheldrake, The Presence of the Past: Morphic Resonance and the Habits of Nature
This dream is often cited as a pivotal moment in his philosophical and scientific development, solidifying his belief in the power of reason and mathematical logic to unravel the mysteries of nature.   *Google AI



1675 In a manuscript Leibniz struggled with the product and quotient rules for differentiation. At first he thought d(uv)= du dv.  *VFR  It would not be until the 21st that he completes the product rule. *F Cajori, History of Mathematics, (pg 208) Leibniz had previously used d twelve days earlier in the denominator, but in the margin he explains that dx is the same as his previous x/d, the difference of two neighboring x's.  Within a fortnight he had created the two basic symbols of calculus that have lasted for almost 350 years.



1744 in a letter of November 11, 1744, Cramer gave Euler a complete description of his rule for solving systems of linear equations. This is noteworthy, because Cramer's Rule would not appear in print until six years later, where it was an appendix in his very influential book “Introduction to the analysis of algebraic curves”.  Even more interesting is that the passage in Cramer's letter is virtually identical, word for word, to a three-page passage in the Introduction [Cramer 1750, pp. 657-659]. *VFR
*Wik


1844 Both the terms vector and scalar were introduced by William Rowan Hamilton (1805-1865). Both terms appear in "On quaternions" a paper presented by Hamilton at a meeting of the Royal Irish Academy on November 11, 1844. This paper adopts the convention of denoting a vector by a single (Greek) letter, and concludes with a discussion of formulae for applying rotations to vectors by conjugating with unit quaternions. *Jeff Miller, Earliest Known Uses of Some of the Words of Mathematics
The term vector, and radius vector had been used much earlier. OED gives the earliest use of "vector" in Astronomy, from a technical dictionary of 1704: J. Harris Lexicon Technicum I. s.v., "A Line supposed to be drawn from any Planet moving round a Center, or the Focus of an Ellipsis, to that Center or Focus, is by some Writers of the New Astronomy, called the Vector; because 'tis that Line by which the Planet seems to be carried round its Center." The term is drawn from the Latin for "to carry".



1912 Bragg's law was first presented by Lawrence Bragg to the Cambridge Philosophical Society. Bragg's law confirmed the existence of real particles at the atomic scale, as well as providing a powerful new tool for studying crystals in the form of X-ray and neutron diffraction. Lawrence Bragg and his father, William Henry Bragg, were awarded the Nobel Prize in physics in 1915 for their work in determining crystal structures beginning with NaCl, ZnS, and diamond. They are the only father-son team to jointly win. Lawrence Bragg was 25 years old, making him the youngest physics Nobel laureate. *Wik 
Bragg’s original notebook where he first wrote down his law for diffraction of X-rays. *

Prof Stuart Mangles@plasmaStu

 The work, titled "The Diffraction of Short Electromagnetic Waves by a Crystal," was subsequently published in the Proceedings of the Cambridge Philosophical Society in 1913.




1918 Armistice Day. At the eleventh hour of the eleventh day of the eleventh month World War I ended.*VFR

In 1925, the discovery of cosmic rays was announced in Madison, Wisconsin by Robert A. Millikan who coined their name.*TIS  After the discovery of radioactivity by Henri Becquerel in 1896, it was generally believed that atmospheric electricity, ionization of the air, was caused only by radiation from radioactive elements in the ground or the radioactive gases or isotopes of radon they produce. In 1909 Theodor Wulf developed an electrometer, a device to measure the rate of ion production inside a hermetically sealed container, and used it to show higher levels of radiation at the top of the Eiffel Tower than at its base. However, his paper published in Physikalische Zeitschrift was not widely accepted. In 1911 Domenico Pacini observed simultaneous variations of the rate of ionization over a lake, over the sea, and at a depth of 3 meters from the surface. Pacini concluded from the decrease of radioactivity underwater that a certain part of the ionization must be due to sources other than the radioactivity of the Earth. *Wik
Millikan's original oil-drop apparatus, circa 1909–1910, *Wik



1930  Albert Einstein and his colleague Leo Szilard designed a refrigerator that avoided the need for seals that could go bad. Instead of the mechanical pumps used in existing commercial refrigerators, the Einstein-Szilard refrigerator used an electromagnetic pump that required no moving parts. The two were motivated by contemporary newspaper reports of a Berlin family who had been killed when a seal in their refrigerator failed and leaked toxic fumes into their home. Einstein and Szilard received a US patent on November 11, 1930, for their invention.

Einstein had other patents such as an expandable blouse, an electrical sound system for hearing aids, and a self-focusing camera.

A much more interesting telling of this story, and many more, can be found in the book, Beer and thew Nobel Prize by  Thomas M. Annesley, Professor of Clinical Chemistry at The University of Michigan Medical School.





1945, Glenn T. Seaborg appeared as a guest on "Quiz Kids." One of the children on the show, Richard Williams, asked Seaborg if any new elements, in addition to plutonium and neptunium, had been discovered at the Metallurgical Laboratory in Chicago during the war. Since the discovery information had already been declassified for announcement at the forthcoming ACS national meeting on Nov. 16, Seaborg shared the news that two new elements (americium and curium) with atomic numbers 95 and 96 had been discovered.
Seaborg then told Williams, "So now you'll have to tell your teachers to change the 92 elements in your schoolbook to 96 elements." Seaborg later recalled in his 1979 Priestley Medal address that many kids did, in fact, tell their teachers to change the number of elements. "Judging from some of the letters I received from such youngsters, they were not entirely successful in convincing their teachers," he said.
*http://pubs.acs.org





1954 Algeria issued a stamp honoring Saint Augustine of Hippo (354–430). He is best remembered for his quote about mathematicians being in league with the devil. [Scott #261] *VFR  (The Quote, "Quapropter bono christiano, sive mathematici, sive quilibet impie divinantium, maxime dicentes vera, cavendi sunt, ne consortio daemoniorum animam deceptam, pacto quodam societatis irretiant." has been translated to "The good Christian should beware the mathematician and all those who make empty prophecies. The danger already exists that the mathematicians have made a covenant with the devil to darken the spirit and to confine man in the bonds of hell." Some suggest this is a mistranslation. The Latin word 'mathematici' derives from the Greek meaning of 'something learned' and refers mainly to astrologers. This was the chief branch of mathematics at the time but has been replaced in modern times by a plethora of other branches. According to the Shorter Oxford English Dictionary, 3rd edition, the word "mathematician" still meant astrologer as late as 1710.) *Wik




1979 Greg Maggs and Robert Kolstad complete the world’s longest slide rule. It is 323 feet long and 9.5 inches wide and is located in the University of Illinois College of Law building, Champaign.  The previous record, 320 feet 11.1 inches in length completed in March, 1979, by students of Alvirne High School, Hudson, New Hampshire. *Guinness  This record was broken in 2001 with a 350 feet 6.6 inch model. To my knowledge, this is currently the World's Longest documented Slide Rule, called The Texas Magnum by Skip Solberg and Jay Francis. It was demonstrated on February 28, 2001 in the Lockeed-Martin Aircraft Assembly Facility at Air Force Plant 4 in Fort Worth, Texas. The Texas Magnum was designed as a traditional Mannheim style slide rule. The A, C, D and L scales are included. *International Slide Rule Museum

A little over two decades later I ran across the smallest slide rule I have ever seen in an Antique shop in Cadiz, Ky.  It was a sterling silver tie clip with a working center bar and slide, two inches long.


  And on a tip from Ted Courant, I found these even smaller cuff link working slide rules, 1.125" long




1997 Proof by John Friedlander and Henryk Iwaniec that there are infinitely many prime numbers of the form m2 + n4, for positive integers m and n submitted to Proceedings of the National Academy of Sciences (USA) "Using a parity-sensitive sieve to count prime values of a polynomial." *Theorem of the Day

2015 In 1966 Chen Jingrun made a giant step toward a proof of Goldbach's conjecture when he stated Chen's Theorem: Every sufficiently large even number can be written as the sum of two primes, or a prime and a semi-prime. On November 11, 2015;  Tomohiro Yamada gave an explicit value for "sufficiently large" when he proved that Chen's theorem is true for all numbers greater than  approximately 17 (101872344071119348) *HT to John Cook







BIRTHS

1729 Birthdate of Louis Antoine de Bougainville.
 Although he began as a mathematician (under d’Alembert’s influence he wrote the first textbook on the integral calculus in 1752), he became famous as an explorer. He was the first Frenchman to sail around the world. But he was no great navigator, in spite of his mathematical ability. *VFR (The largest of the Solomon Islands is named after him, as is the colorful tropical climbing plant bougainvillaea. (see image at top))



1851 Adolphe-Louis Jacques Bertillon (11 Nov 1851 in Paris, France - 7 July 1922 in Valmondois, near Paris, France) Bertillon was a French statistician who applied statistics to social sciences. *SAU


1875 Vesto Melvin Slipher (11 Nov 1875; died 8 Nov 1969) American astronomer whose systematic observations (1912-25) of the extraordinary radial velocities of spiral galaxies provided the first evidence supporting the expanding-universe theory. Slipher spectroscopically measured the displacement of their spectral lines by the Doppler effect by which the wavelength of light from an object moving away from an observer will shifted toward the red end of the spectrum. Earlier, Slipher had determined the rotation periods of some of the planets by spectroscopic means. With Lowell (1912), he found Uranus had a  rotation period of  10.8 hours. He also produced comparable data for Venus, Mars, Jupiter, and Saturn and showed that Venus's period was much longer than expected. *TIS




1904 John Henry Constantine Whitehead (11 November 1904–8 May 1960), known as Henry, was a British mathematician and was one of the founders of homotopy theory. He was born in Chennai (then known as Madras), in India, and died in Princeton, New Jersey, in 1960. *Wik
Whitehead's work in differential geometry culminated in the paper "On the Covering of a Complete Space by the Geodesics Through a Point" (1935), containing pioneering contributions to this area of mathematics. He always retained his interest in geometry but soon focused on topology. He made substantial contributions to combinatorial homotopy and Stiefel manifolds and set up a school of topology at Oxford. *TIS One of his better quotes was, "It is the snobbishness of the young to suppose that a theorem is trivial because the proof is trivial."





1905 Sigekatu Kuroda (黒田 成勝, Kuroda Shigekatsu, 11 November 1905 – 3 November 1972) was a Japanese mathematician who worked in number theory and mathematical logic.
In 1942 he became a professor at the newly founded Nagoya Imperial University, where he stayed for over twenty years. He was responsible for much of the effort in setting up its Department of Mathematics.

He was married to the renowned number theorist Teiji Takagi's daughter Yakeo. The couple had three sons, all of whom became mathematicians, including S.-Y. Kuroda, who was a professor of linguistics at the University of California, San Diego.

He published a text on the foundations of algebraic number theory with Tomio Kubota in 1963.








1911 Caleb Gattegno (November 11, 1911; Alexandria, Egypt- July 28, 1988, Paris, France) was born in Alexandria, Egypt. He is best known for his innovative approaches to teaching and learning mathematics (Visible & Tangible Math). Creator of the Geoboard, and founder of the Cuisenaire Company which manufactures educational manipulatives. *Wik




1930 Hugh Everett III (November 11, 1930 – July 19, 1982) was an American physicist who first proposed the many-worlds interpretation (MWI) of quantum physics, which he termed his "relative state" formulation.
Discouraged by the scorn of other physicists for MWI, Everett ended his physics career after completing his Ph.D. Afterwards, he developed the use of generalized Lagrange multipliers for operations research and applied this commercially as a defense analyst and a consultant. He was married to Nancy Everett née Gore. They had two children: Elizabeth Everett and Mark Oliver Everett, who became frontman of the musical band Eels.





DEATHS




1938 Typhoid Mary
 (Mary Mallon) , (23 Sep 1869, 11 Nov 1938) famous typhoid carrier in the New York City area in the early 20th century. Fifty-one original cases of typhoid and three deaths were directly attributed to her (countless more were indirectly attributed), although she herself was immune to the typhoid bacillus (Salmonella typhi). The outbreak of Typhus in Oyster Bay, Long Island, in 1904 puzzled the scientists of the time because they thought they had wiped out the deadly disease. Mallon's case showed that a person could be a carrier without showing any outward signs of being sick, and it led to most of the Health Code laws on the books today. She died not from typhoid but from the effects of a paralytic stroke dating back to 25 Dec 1932. *TIS




1954 Horatio Carslaw (12 February 1870, Helensburgh, Dumbartonshire, Scotland – 11 November 1954, Burradoo, New South Wales, Australia) studied at Glasgow and Cambridge. He lectured at the University of Glasgow before moving to a professorship in Sydney, Australia. He worked on a variety of topics in both pure and applied mathematics. He co-authored  Conduction of Heat in Solids, which remains a classic in the field. *SAU






1967 Lester Randolph Ford, Sr. (October 25, 1886 – 11 November 1967) was an American mathematician, editor of the American Mathematical Monthly from 1942 to 1946, and President of the Mathematical Association of America from 1947 to 1948.
Ford circles are named after him.*Wik (Students, if you are not familiar with Ford Circles, and their rich beautiful history and interesting algebraic and geometric relations, look them up for an interesting exploration.  Start here)
He is the father of L. R. Ford Jr, who specializes in network flow problems.





1997  Menahem Max Schiffer (24 September 1911, Berlin – 11 November 1997)) was a German-born American mathematician who worked in complex analysis, partial differential equations, and mathematical physics.
Menachem Max Schiffer studied physics from 1930 at the University of Bonn and then at the Humboldt University of Berlin with Max von Laue, Erwin Schrödinger, Walter Nernst, Erhard Schmidt, Issai Schur and Ludwig Bieberbach. In Berlin he worked closely with Issai Schur. In 1934, after being forced by the Nazis to leave the academic world, he immigrated to Mandatory Palestine.

On the basis of his prior mathematical publications, Schiffer received a master's degree from the Hebrew University of Jerusalem. In 1938, he received his doctorate under the supervision of Michael Fekete. In his dissertation on Conformal representation and univalent functions he introduced the "Schiffer variation", a method for handling geometric problems in complex analysis.

In September 1952, he began to teach at Stanford University, along with George Pólya, Charles Loewner, Stefan Bergman, and Gábor Szegő.

With Paul Garabedian, Schiffer worked on the Bieberbach conjecture with a proof in 1955 of the special case n=4. He was a speaker at the International Congress of Mathematicians (ICM) in 1950 at Cambridge, Massachusetts, and was a plenary speaker at the ICM in 1958 at Edinburgh with plenary address Extremum Problems and Variational Methods in Conformal Mapping. In 1970 he was elected to the United States National Academy of Sciences. He retired from Stanford University as professor emeritus in 1977. *Wik



2003  Andrei Andreevich Bolibrukh  (30 January 1950 – 11 November 2003) was a Soviet and Russian mathematician. He was known for his work on ordinary differential equations especially Hilbert's twenty-first problem (Riemann–Hilbert problem). Bolibrukh was the author of about a hundred research articles on theory of ordinary differential equations including Riemann–Hilbert problem and Fuchsian system.

 After receiving his mathematical education at the Lomonosov Moscow State University, with Mikhail Mikhailovich Postnikov and Alexey Chernavskii as thesis advisers, he started working on the proof of the existence of linear differential equations having a prescribed monodromic group. He applied modern methods of complex analytic geometry to classical problems about ordinary differential equations and was an expert on Hilbert's twenty-first problem. In 1989, Bolibrukh produced his famous counterexamples which invalidated the Josip Plemelj's 1908 solution of Hilbert's twenty-first problem. Bolibrukh dedicated much of his efforts to the Riemann-Hilbert problem in order to find full necessary and sufficient conditions for given monodromy data to be those of a Fuchsian system.

During his short career he served as Deputy Director of the Steklov Institute of Mathematics and professor at the Moscow Institute of Physics and Technology. *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

Tuesday, 10 November 2026

Lune, Lens and related terms.....Etymology and History of Math Terms

  Lune, Lens and related terms

The word lune is from Luna, the Roman Goddess of the Moon. The more ancient Indo-European root is leuk, which relates to light. Lunatic is from the same root, perhaps because the ancients believed it was the effects of the moon that accounted for the crazy behavior.
Lune is used in mathematics to describe two different ideas. [see figure below] The most common is the area on a sphere between two semicircles with endpoints at the same poles. Imagine two lines of longitude running from the North Pole to the South pole. The surface of the Earth between the two lines is called a lune. There is also a two dimensional shape called a lune. The crescent area formed between two excentric circles that share a common chord is also called a lune. This shape plays an important part in the mathematics of the ancient Greeks. The definition I have used is from "The Mechanic's Assistant: A Thorough Practical Treatise on Mensuration" by D. M. Knappen, published in 1849. The Wolfram Mathworld web site, which is usually one of the top sources for math topics defines the planer lune this way, "A lune is a plane figure bounded by two circular arcs of unequal radii, i.e., a crescent." These two definitions do NOT seem to be the same to me. Imagine the crescent formed by two excentric circles of the same radius. I wonder why this must be excluded from the Wolfram definition. Under either construction, there are two crescent regions formed. Students will not see many planer lunes in their math experience, but the ones they do seem almost all to be constructed so that the smaller radius circle has its center on the common chord of the two circles. I do not think this is a property of lunes in genral. To be sure, I asked the memebers of the Philomathes Yahoo discussion group, and Colin McLarty responded with, "Neither arc needs to have its center on the common chord, and Hippocrates did a case where neither one does. Since he was interested in squaring lunes, and he was so far as we know pretty much limited to Euclidean means, he necessarily dealt with only very special cases. It is unlikely he ever worried about a precise general definition of "lune" -- esp. whether or not the case of equal radii would qualify to be called a lune." [see a suggested definition from David W. Cantrell farther below]

A spherical lune is sometimes also called a digon, since it is a two-sided polygon (and less appropriately called a bigon since that mixes both Latin and Greek roots... and leads too often to the quip, "let bigons be bigons".)

The plane lune was studied in depth by the Greek mathematician Hippocrates of Chios (around 400 BC) in an attempt to find a way to find a square with the same area as a given circle using only the classic tools of compass and straightedge. He discovered that a lune formed by the chord which is the hypotenuse of a central right angle has an area equal to the area of the right triangle. This lune is still called the Lune of Hippocrates. Later he found two other plane lunes that could also be "squared". A nice site on the lunes which can be squared is here. The problem of "Squaring the Circle" was one of the three great unsolved problems of Greek mathematics. Much later it was proven using algebraic tools that the task was impossible, but the Greeks discovered lots of important mathematical ideas in their search to prove the impossible.

Hippocrates of Chios, the mathematician, is often confused with Hippocrates of Cos, who is considered to be the father of medicine, and for whom the Hippocratic Oath is named. This should not be two unexpected since they both lived at the same time, and came from relatively close islands off the coast of modern day turkey. This link shows a map of the area. There is an arrow pointing out the island of Cos, just northwest of Rhodes. North of Cos just south of Lesbos is the island of Chios. Between them is the Island of Samos, which was the birthplace of Pythagorus.

Two similar looking objects that may be included here are "lens" and "gibbous". The area of intersection between two circles is often called a lens, because it resembles a biconvex lens. The word lens actually is drawn from the word lentil, for its symmilarity to the lentil seed. Gibbous is derived from the Latin root for "hunchback" and can be applied to any object that is convex or rounded, but is most commonly used to describe the phases of the moon between a half-moon and a full-moon.

There is, or once was, a special name for the intersection between two identical circles and is called the Vesci Pescies. Here is a description from "Geometry in Art" by Hilton Andrade De Mello. "The 'Vesica Piscis' is an important symbol based on the circle. It is generated by the intersection of two identical circles, as shown in Figure 9.2 with one circle centered at point A and the other centered at point B. The area common to both circles, shown in blue, is called 'Vesica Piscis' because it resembles a vesicle, i.e., a receptacle. As seen later in this chapter, the “Piscis”, which is Latin for 'fish', is associated with the symbol adopted by early Christianity." Images below are from the e-text of the book.

 

David W. Cantrell suggested what I think are very clear definitions of lune and lens in a discussion on another list, and graciously sent me a copy: ”Given two circular disks, A and B, having a nonempty intersection and such that neither is entirely contained in the other, three regions are formed. (Think of a Venn diagram.) One of the regions, A intersect B, is convex; I suggest that "lens" be used to name that kind of shape. Neither of the other two regions, A-B and B-A, is convex; I suggest that "lune" be used to name that kind of shape. “