The shortest path between two truths in the real domain passes through the complex domain.

~Jacques Salomon HadamardThe 236th day of the year; 236 is the sum of twelve consecutive primes, 3 + 5 + 7 + 11 + 13 + 17 + 19 + 23 + 29 + 31 + 37 + 41

**EVENTS**

**79 -**Thousands were killed when the cities of Pompeii and Herculaneum were buried by the eruption of Mount Vesuvius.*VFR An estimated 20,000 people died. When discovered, the sites became astonishing archaeological time capsules.

1563 Tycho Brahe watched a spectacular conjunction of Jupiter and Saturn, and found that the time of the closest approach was days away from the predictions in the Ptolemaic Tables. He emerged from the experience with a life long passion for accuracy and exactitude and a devotion to the verdict of the sky. *Timothy Ferris, Coming of Age in the Milky Way

**1609**Galileo presented this telescope to the Doge in the Presence Chamber of the Doge's Palace and was confirmed in the professorship for life with his salary doubled! [Letter of 29 Aug 1609 from Galileo to his brother‑in‑law in Florence, quoted in Fahie, pp. 82‑83.] '... an object which is at a distance of nine miles will appear as if it were only one mile away, ... one can detect ships and sails of the enemy at sea ... we can see him two or more hours earlier than he can possibly see us, ....' [Galileo's letter to the Doge on 24 Aug 1609, quoted in Scandone, pp.12‑14 ; in Van Helden, pp. 7-8]. Through the connections of his friend Paolo Sarpi, Galileo presents an eight-powered telescope to the Venetian Senate. He is rewarded by a doubling of his salary and life- tenure at the University of Padua. He is disappointed by the fine print. *Galileo Project (

*I love the idea that the Greek name "telescope" was created by an actual Greek mathematician. It was created in 1611 by the Greek mathematician Giovanni Demisiani for one of Galileo Galilei's instruments presented at a banquet at the Accademia dei Lincei.*)

**1654**Pascal wrote a letter to Fermat, discussing Fermat’s solution to the “problem of points.”

*http://www.york.ac.uk/depts/maths/histstat/pascal.pdf

I was not able to tell you my entire thoughts regarding the problem of the points

by the last post,and at the same time, I have a certain reluctance at doing it for fear lest

this admirable harmony which obtains between us and which is so dear to me should

begin to flag, for I am afraid that we may have different opinions on this subject. I

wish to lay my whole reasoning before you, and to have you do me the favor to set me

straight if I am in error or to indorse me if I am correct. I ask you this in all faith and

sincerity for I am not certain even that you will be on my side.

When there are but two players, your theory which proceeds by combinations is

very just. But when there are three, I believe I have a proof that it is unjust that you

should proceed in any other manner than the one I have. But the method which I

have disclosed to you and which I have used universally is common to all imaginable

conditions of all distributions of points, in the place of that of combinations (which I do

not use except in particular cases when it is shorter than the general method), a method

Which is good only in isolated cases and not good for others.

I am sure that I can make it understood, but it requires a few words from me and a

little patience from you. (I wish I had known this phrase early in my teaching career… it seems it would have been frequently handy)

1971 The Soviet Union issued a stamp for the centenary of the birth of the British physicist, Ernest Rutherford. Beside his picture is a diagram of the movement of atomic particles which involves a hyperbola. [Scott #3888].*VFR

**2006**And then there were only eight.... the International Astronomical Union decided to rescind Pluto’s status as a planet and reclassify it as another entity called a “dwarf planet”. *FFF, pg 537

**BIRTHS**

**1561 Bartholomeo Pitiscus**born. He coined the word “Trigonometry,” and ﬁrst used it in print in 1595.*VFR

**1846 Professor Enoch Beery Seitz, the most distinguished mathematician of his**

day (Fairfield county, Ohio, August 24, 1846,- Kirksville, Missouri, October 8, 1883)

day (Fairfield county, Ohio, August 24, 1846,- Kirksville, Missouri, October 8, 1883)

**He began his mathematical course in 1872 by contributing solutions to the problems proposed in the "Stairway" department of the Schoolday Magazine, conducted by Artemas Martin. His masterlv and original solutions to difflcult Average and Probability problems, poon attracted universal attention among mathematicians. Dr. Martin, being desirous to know what works he had treating on that difflcult subject, was greatly surprised to learn that he had no works upon the subject, but had learned what he knew about that difficult department of mathematical science by**

studying the problems and solutions in the Shohlday Magazine. He then contributed to the Analyst, the Mathematical Visitor, the Mathematical Magazine, the School Visitor, and the Educational limes, of London, England.

studying the problems and solutions in the Shohlday Magazine. He then contributed to the Analyst, the Mathematical Visitor, the Mathematical Magazine, the School Visitor, and the Educational limes, of London, England.

**He took a mathematical course in the Ohio Wesleyan University in 1870, but did not finish it or graduate. In 1879,he was elected one of the teachers in the Greenville High School, which position he held till 1879. On the 24th of June, 1875, he married Miss Anna E. Kerlin, one of Dark county's most refined ladies. In 1879, he was elected to the chair of mathematics in the Missouri State Normal schlool, Kirksville, Missouri, which position he held till death called him from the confines of earth, ere his star of fame had reached the zenith of its glory. He was striken by that "demon**

of death," typhoid fever, and passed the mysterious shades, to be numbered with the silent majority, on the 8th of October, 1883. On March the llth, 1880,he was elected a member of the London Mathematical Society, being the fifth American so honored. *The American Mathematical Monthly Vol. 1, No. 1, Jan., 1894

of death," typhoid fever, and passed the mysterious shades, to be numbered with the silent majority, on the 8th of October, 1883. On March the llth, 1880,he was elected a member of the London Mathematical Society, being the fifth American so honored. *

He is often called "Teacher of the Great", for his many distinguished students: "When Professor Seitz went to Kirksville, in spite of the youth of the institution, he found an enthusiastic and capable body of students. He entered upon his work with his usual energy and the results of it are still felt throughout the country. He had in his class in algebra at one time, in the autumn of 1880, John J. Pershing who was destined to be the head of the armies of the United States In the World War, and Enoch Crowder who became head of the draft boards in the same conflict. He also had as a student at Kirksville. B F. Carroll, who later became governor of the state of Iowa, and John. R. Kirk who became president of the same institution in which he was then a student of Professor Seitz." *Obit in The Herald-Advertiser of Huntington, W.Va.

**Rudolf Oskar Robert Williams Geiger**(24 Aug 1894, 22 Jan 1981) German meteorologist, one of the founders of microclimatology, the study of the climatic conditions within a few metres of the ground surface. His observations, made above grassy fields or areas of crops and below forest canopies, elucidated the complex and subtle interactions between vegetation and the heat, radiation, and water balances of the air and soil.*TIS

**1943 Karen Uhlenbeck**is a leading expert on partial differential equations. She is currently Professor, and Sid W. Richardson Regents Chairholder, Department of Mathematics, University of Texas, Austin. *Univ of Texas

**DEATHS**

**1595 Thomas Digges**(1546?, 24 Aug 1595)

English astronomer and mathematician who (with his father, Leonard) was a pioneer in the use of the telescope. He was the leader of the English Copernicans. His observations of the new star of 1572, published in his Alae seu scalae mathematicae (1573) were second only to Tycho Brahe in accuracy. He used his observations of the supernova to justify the heliocentric system. In mathematics, he wrote on platonic and archimedian solids. *TIS After his father's death he was adopted and taught by John Dee. Digges was one of the first to translate (parts of) Copernicus into English. *Renaissance Mathematicus

**1670 William Neil**died. He was an English mathematician who was the first to calculate the arc-length of the cubical parabola.*SAU

**1739 Takebe Katahiro**was a Japanese mathematician who wrote most of Seki's Encyclopaedia.*SAU

**1796 (Nicholas Léonard) Sadi Carnot**(born 1 Jun 1796, 24 Aug 1832) was a French physicist. He became a captain of engineers in the army, and spent much of his life investigating the design of steam engines. His book Reflections on the Motive Power of Heat (1824) contained a theorem which says that a maximum efficiency of heat engine can be obtained by a reversible engine, and that efficiency depends only on the temperatures of the hot and the cool sources of the engine. This theorem played an essential role for the subsequent development of thermodynamics. It was written to promote the construction of steam engines and other heat engines in France, whose industrial development was lagging behind England's. *TIS

**1842 Benjamin Wright**(10 Oct 1770, 24 Aug 1842)American engineer who directed the construction of the Erie Canal. A one-time judge, he helped survey the Erie Canal route. When the Erie Canal was finally funded in 1817, Wright was selected as one of the three engineers to design and build it, then named chief engineer. Wright made the Erie Canal project a school of engineering. Until mid-century, almost every civil engineer in the U.S. had trained with, or been trained by someone who had worked under, Wright on the Erie Canal. Because he trained so many engineers on that project, Wright has been called the "father of American civil engineering." He also engaged in the design and construction at the outset of the first railroads. He was the first Chief Engineer of the Erie Railroad.*TIS

**1888 Rudolf (Julius Emanuel) Clausius**(2 Jan 1822, 24 Aug 1888) was a German mathematical physicist who formulated the second law of thermodynamics and is credited with making thermodynamics a science. Essentially a theoretical physicist, he published his work in thermodynamics in 1865 wherein he stated the First and Second laws of thermodynamics in the following form: (1) The energy of the universe is constant. (2) The entropy of the universe tends to a maximum. In all Clausius wrote eight important papers on the topic. He restated Sadi Carnot's principle of the efficiency of heat engines. The -Clapeyron equation expresses the relation between the pressure and temperature at which two phases of a substance are in equilibrium. *TIS

Anna Margaret Mullikin (March 7, 1893 - August 24, 1975) She was born in Baltimore, Maryland and attended Goucher College, which was then a women's college located in the same city. While there she managed her class basketball team, participated on the swimming team, and earned her A.B. degree in 1915. That same year her name was mentioned in the American Mathematical Monthly [Vol. 22, No. 5 (May 1915),pp. 165-166] for solving the following geometry problem:

A quadrilateral of any shape whatever is divided by a transversal into two quadrilaterals. The diagonals of the original figure and those of the two resulting (smaller) figures are then drawn. Show that their three points of intersection are collinear.In 1918 she entered the graduate program in mathematics at the University of Pennsylvania, earning her master's degree in 1919. She continued her graduate studies at Penn during the 1919-1920 academic year under the direction of the topologist, Robert L. Moore, while also teaching at the Stevens School in Germantown, Pennsylvania, another private preparatory school for girls. In the fall of 1920 she moved to the University of Texas along with Moore, who had convinced the Texas math department to appoint her as an instructor. Mullikin stayed in Texas for only the one academic year before returning to Philadelphia to complete the requirements for her degree from the University of Pennsylvania, with Moore still as her advisor. She received her Ph.D. in mathematics in 1922. Mullikin did not pursue mathematical research after earning her Ph.D. She spent the rest of her professional career as a high school mathematics teacher, first at William Penn High School for Girls in Philadelphia for one year, and then at Germantown High School where she remained until her retirement in 1959. She was appointed head of the mathematics department in 1952. In 1956 she was a joint author with Ethel and Ewart Grove for the textbook Algebra and Its Use. *Agnes Scott College

The published solution was by Vola Barton, also from Goucher College, with the remark "Also solved by Anna Mullikin."

**1982 Giorgio Abetti**(5 Oct 1882,24 Aug 1982)Italian astronomer known for his studies of the sun at the University of Padua where was director at the Arcetri Observatory (1921-52), taking over from his father who also held the post (1894-1921). In 1913, Giorgio Abetti took part, as a geodetic and geophysical astronomer, in the De Filippi expedition in Karakorum, Himalaya and Turkestan. He went on expeditions to observe eclipses of the sun, including one to Siberia to observe the total eclipse on 19 Jun 1936 and in 1952 to Sudan. With the advice of George Hale, he built a solar tower at the observatory (opened 1925). He wrote a popular text on the sun, a handbook of astrophysics (1936) and a popular history of astronomy (1963).*TIS

**1997 Louis Essen**(6 Sep 1908, 24 Aug 1997 )English physicist who invented the quartz crystal ring clock and the first practical atomic clock. These devices were capable of measuring time more accurately than any previous clocks. He built a cesium-beam atomic clock, a device that ultimately changed the way time is measured. Each chemical element and compound absorbs and emits electromagnetic radiation at its own characteristic frequencies. These resonances are inherently stable over time and space. The cesium atom's natural frequency was formally recognized as the new international unit of time in 1967: the second was defined as exactly 9,192,631,770 oscillations or cycles of the cesium atom's resonant frequency, replacing the old second defined in terms of the Earth's motion. *TIS

Credits

*VFR = V Frederick Rickey, USMA

*TIS= Today in Science History

*Wik = Wikipedia

*SAU=St Andrews Univ. Math History

*CHM=Computer History Museum