Euler, Leonhard
Euler, Leonhard
(b. Basel, Switzerland, 15 April 1707; d. St. Petersburg, Russia, 18 September 1783)
mathematics, mechanics, astronomy, physics.
Life . Euler’s forebears settled in Basel at the end of the sixteenth century. His greatgreatgrandfather, Hans Georg Euler, had moved from Lindau, on the Bodensee (Lake Constance). They were, for the most part, artisans; but the mathematician’s father, Paul Euler, graduated from the theological department of the University of Basel. He became a Protestant minister, and in 1706 he married Margarete Brucker, daughter of another minister. In 1708 the family moved to the village of Riehen, near Basel, where Leonhard Euler spent his childhood.
Euler’s father was fond of mathematics and had attended Jakob Bernoulli’s lectures at the university; he gave his son his elementary education, including mathematics. In the brief autobiography dictated to his eldest son in 1767, Euler recollected that for several years he diligently and thoroughly studied Christoff Rudolf’s Algebra, a difficult work (dating, in Stifel’s edition, from 1553) which only a very gifted boy could have used. Euler later spent several years with his maternal grandmother in Basel, studying at a rather poor local Gymnasium; mathematics was not taught at all, so Euler studied privately with Johann Burckhardt, an amateur mathematician. In the autumn of 1720, being not yet fourteen, Euler entered the University of Basel in the department of arts to get a general education before specializing. The university was small; it comprised only a few more than a hundred students and nineteen professors. But among the latter was Johann I Bernoulli, who had followed his brother Jakob, late in 1705, in the chair of mathematics. During the academic year, Bernoulli delivered daily public lectures on elementary mathematics; besides that, for additional pay he conducted studies in higher mathematics and physics for those who were interested. Euler laboriously studied all the required subjects, but this did not satisfy him. According to the autobiography:
... I soon found an opportunity to be introduced to a famous professor Johann Bernoulli.... True, he was very busy and so refused flatly to give me private lessons; but he gave me much more valuable advice to start reading more difficult mathematical books on my own and to study them as diligently as I could; if I came across some obstacle or difficulty, I was given permission to visit him freely every Saturday afternoon and he kindly explained to me everything I could not understand.... and this, undoubtedly, is the best method to succeed in mathematical subjects.^{1}
In the summer of 1722, Euler delivered a speech in praise of temperance, “De temperantia,” and received his prima laurea, a degree corresponding to the bachelor of arts. The same year he acted as opponent (respondens) at the defense of two theses—one on logic, the other on the history of law. In 1723 Euler received his master’s degree in philosophy. This was officially announced at a session on 8 June 1724; Euler made a speech comparing the philosophical ideas of Descartes and Newton. Some time earlier, in the autumn of 1723, he had joined the department of theology, fulfilling his father’s wish. His studies in theology, Greek, and Hebrew were not very successful, however; Euler devoted most of his time to mathematics. He finally gave up the idea of becoming a minister but remained a wholehearted believer throughout his life. He also retained the knowledge of the humanities that he acquired in the university; he had an outstanding memory and knew by heart the entirety of Vergil’s Aeneid. At seventy he could recall precisely the lines printed at the top and bottom of each page of the edition he had read when he was young.
At the age of eighteen, Euler began his independent investigations. His first work, a small note on the construction of isochronous curves in a resistant medium,^{2} appeared in Acta eruditorum (1726); this was followed by an article in the same periodical on algebraic reciprocal trajectories (1727).^{3} The problem of reciprocal trajectories was studied by Johann I Bernoulli, by his son Nikolaus II, and by other mathematicians of the time. Simultaneously Euler participated in a competition announced by the Paris Académie des Sciences which proposed for 1727 the problem of the most efficient arrangement of masts on a ship. The prize went to Pierre Bouguer, but Euler’s work^{4} received the accessit. Later, from 1738 to 1772, Euler was to receive twelve prizes from the Academy.
For mathematicians beginning their careers in Switzerland, conditions were hard. There were few chairs of mathematics in the country and thus little chance of finding a suitable job. The income and public recognition accorded to a university professor of mathematics were not cause for envy. There were no scientific magazines, and publishers were reluctant to publish books on mathematics, which were considered financially risky. At this time the newly organized St. Petersburg Academy of Sciences (1725) was looking for personnel. In the autumn of that year Johann I Bernoulli’s sons, Nikolaus II and Daniel, went to Russia. On behalf of Euler, they persuaded the authorities of the new Academy to send an invitation to their young friend also.
Euler received the invitation to serve as adjunct of physiology in St. Petersburg in the autumn of 1726, and he began to study this discipline, with an effort toward applying the methods of mathematics and mechanics. He also attempted to find a job at the University of Basel. A vacancy occurred in Basel after the death of a professor of physics, and Euler presented as a qualification a small composition on acoustics, Dissertatio physica de sono (1727).^{5} Vacancies were then filled in the university by drawing lots among the several chosen candidates. In spite of a recommendation from Johann Bernoulli, Euler was not chosen as a candidate, probably because he was too young—he was not yet twenty. But, as O. Spiess has pointed out, this was in Euler’s favor;^{6} a much broader field of action lay ahead of him.
On 5 April 1727 Euler left Basel for St. Petersburg, arriving there on 24 May. From this time his life and scientific work were closely connected with the St. Petersburg Academy and with Russia. He never returned to Switzerland, although he maintained his Swiss citizenship.
In spite of having been invited to St. Petersburg to study physiology, Euler was at once given the chance to work in his real field and was appointed an adjunct member of the Academy in the mathematics section. He became professor of physics in 1731 and succeeded Daniel Bernoulli, who returned to Basel in 1733 as a professor of mathematics. The young Academy was beset with numerous difficulties, but on the whole the atmosphere was exceptionally beneficial for the flowering of Euler’s genius. Nowhere else could he have been surrounded by such a group of eminent scientists, including the analyst, geometer, and specialist in theoretical mechanics Jakob Hermann, a relative; Daniel Bernoulli, with whom Euler was connected not only by personal friendship but also by common interests in the field of applied mathematics; the versatile scholar Christian Goldbach, with whom Euler discussed numerous problems of analysis and the theory of numbers; F. Maier, working in trigonometry; and the astronomer and geographer J.N. Delisle.
In St. Petersburg, Euler began his scientific activity at once. No later than August 1727 he started making reports on his investigations at sessions of the Academy; he began publishing them in the second volume of the academic proceedings, Commentarii Academiae scientiarum imperialis Petropolitanae (1727) (St. Petersburg, 1729). The generous publication program of the Academy was especially important for Euler, who was unusually prolific. In a letter written in 1749 Euler cited the importance that the work at the Academy had for many of its members:
... I and all others who had the good fortune to be for some time with the Russian Imperial Academy cannot but acknowledge that we owe everything which we are and possess to the favorable conditions which we had there.^{7}
In addition to conducting purely scientific work, the St. Petersburg Academy from the very beginning was also obliged to educate and train Russian scientists, and with this aim a university and a Gymnasium were organized. The former existed for nearly fifty years and the latter until 1805. The Academy was also charged to carry out for the government a study of Russian territory and to find solutions for various technological problems. Euler was active in these projects. From 1733 on, he successfully worked with Delisle on maps in the department of geography. From the middle of the 1730’s he studied problems of shipbuilding and navigation, which were especially important to the rise of Russia as a great sea power. He joined various technological committees and engaged in testing scales, fire pumps, saws, and so forth. He wrote articles for the popular periodical of the Academy and reviewed works submitted to it (including those on the quadrature of the circle), compiled the Einleitung zur RechenKunst^{8} for Gymnasiums, and also served on the examination board.
Euler’s main efforts, however, were in the mathematical sciences. During his fourteen years in St. Petersburg he made brilliant discoveries in such areas as analysis, the theory of numbers, and mechanics. By 1741 he had prepared between eighty and ninety works for publication. He published fiftyfive, including the twovolume Mechanica.^{9}
As is usual with scientists, Euler formulated many of his principal ideas and creative concepts when he was young. Neither the dates of preparation of his works nor those of their actual publication adequately indicate Euler’s intellectual progress, since a number of the plans formulated in the early years in St. Petersburg (and even as early as the Basel period) were not realized until much later. For example, the first drafts of the theory of motion of solid bodies, finished in the 1760’s, were made during this time. Likewise Euler began studying hydromechanics while still in Basel, but the most important memoirs on the subject did not appear until the middle of the 1750’s; he imagined a systematic exposition of differential calculus on the basis of calculus of finite differences in the 1730’s but did not realize the intention until two decades later; and his first articles on optics appeared fifteen years after he began studying the subject in St. Petersburg. Only by a complete study of the unpublished Euler manuscripts would it be possible to establish the progression of his ideas more precisely.
Because of his large correspondence with scientists from many countries, Euler’s discoveries often became known long before publication and rapidly brought him increasing fame. An index of this is Johann I Bernoulli’s letters to his former disciple—in 1728 Bernoulli addressed the “most learned and gifted man of science Leonhard Euler”; in 1737 he wrote, the “most famous and wisest mathematician”; and in 1745 he called him the “incomparable Leonhard Euler” and “mathematicorum princeps.” Euler was then a member of both the St. Petersburg and Berlin academies. (That certain frictions between Euler and Schumacher, the rude and despotic councillor of the St. Petersburg Academy, did Euler’s career no lasting harm was due to his tact and diplomacy.) He was later elected a member of the Royal Society of London (1749) and the Académie des Sciences of Paris (1755). He was elected a member of the Society of Physics and Mathematics in Basel in 1753.
At the end of 1733 Euler married Katharina Gsell, a daughter of Georg Gsell, a Swiss who taught painting at the Gymnasium attached to the St. Petersburg Academy. Johann Albrecht, Euler’s first son, was born in 1734, and Karl was born in 1740. It seemed that Euler had settled in St. Petersburg for good; his younger brother, Johann Heinrich, a painter, also worked there. His quiet life was interrupted only by a disease that caused the loss of sight in his right eye in 1738.
In November 1740 Anna Leopoldovna, mother of the infant Emperor Ivan VI, became regent, and the atmosphere in the Russian capital grew troubled. According to Euler’s autobiography, “things looked rather dubious.”^{10} At that time Frederick the Great, who had succeeded to the Prussian throne in June 1740, decided to reorganize the Berlin Society of Sciences, which had been founded by Leibniz but allowed to degenerate during Frederick’s father’s reign. Euler was invited to work in Berlin. He accepted, and after fourteen years in Russia he sailed with his family on 19 June 1741 from St. Petersburg. He arrived in Berlin on 25 July.
Euler lived in Berlin for the next twentyfive years. In 1744 he moved into a house, still preserved, on the Behrenstrasse. The family increased with the birth of a third son, Christoph, and two daughters; eight other children died in infancy. In 1753 Euler bought an estate in Charlottenburg, which was then just outside the city. The estate was managed by his mother, who lived with Euler after 1750. He sold the property in 1763.
Euler’s energy in middle age was inexhaustible. He was working simultaneously in two academies—Berlin and St. Petersburg. He was very active in transforming the old Society of Sciences into a large academy—officially founded in 1744 as the Académie Royale des Sciences et des Belles Lettres de Berlin. (The monarch preferred his favorite language, French, to both Latin and German.) Euler was appointed director of the mathematical class of the Academy and member of the board and of the committee directing the library and the publication of scientific works. He also substituted for the president, Maupertuis, when the latter was absent. When Maupertuis died in 1759, Euler continued to run the Academy, although without the title of president. Euler’s friendship with Maupertuis enabled him to exercise great influence on all the activities of the Academy, particularly on the selection of members.
Euler’s administrative duties were numerous: he supervised the observatory and the botanical gardens; selected the personnel; oversaw various financial matters; and, in particular, managed the publication of various calendars and geographical maps, the sale of which was a source of income for the Academy. The king also charged Euler with practical problems, such as the project in 1749 of correcting the level of the Finow Canal, which was built in 1744 to join the Havel and the Oder. At that time he also supervised the work on pumps and pipes of the hydraulic system at Sans Souci, the royal summer residence.
In 1749 and again in 1763 he advised on the organization of state lotteries and was a consultant to the government on problems of insurance, annuities, and widows’ pensions. Some of Euler’s studies on demography grew out of these problems. An inquiry from the king about the best work on artillery moved Euler to translate into German Benjamin Robins’ New Principles of Gunnery. Euler added his own supplements on ballistics, which were five times longer than the original text (1745).^{11} These supplements occupy an important place in the history of ballistics; Euler himself had written a short work on the subject as early as 1727 or 1728 in connection with the testing of guns.^{12}
Euler’s influence upon scientific life in Germany was not restricted to the Berlin Academy. He maintained a large correspondence with professors at numerous German universities and promoted the teaching of mathematical sciences and the preparation of university texts.
From his very first years in Berlin, Euler kept in regular working contact with the St. Petersburg Academy. This contact was interrupted only during military actions between Prussia and Russia in the course of the Seven Years’ War—although even then not completely. Before his departure from the Russian capital, Euler was appointed an honorary member of the Academy and given an annual pension; on his part he pledged to carry out various assignments of the Academy and to correspond with it. During the twentyfive years in Berlin, Euler maintained membership in the St. Petersburg Academy à tous les titres, to quote N. Fuss. On its commission he finished the books on differential calculus and navigation begun before his departure for Berlin edited the mathematical section of the Academy journal; kept the Academy apprised, through his letters, of scientific and technological thought in Western Europe; bought books and scientific apparatus for the Academy; recommended subjects for scientific competitions and candidates to vacancies; and served as a mediator in conflicts between academicians.
Euler’s participation in the training of Russian scientific personnel was of great importance, and he was frequently sent for review the works of Russian students and even members of the Academy. For example, in 1747 he praised most highly two articles of M.V. Lomonosov on physics and chemistry; and S.K. Kotelnikov, S. Y. Rumovski, and M. Sofronov studied in Berlin under his supervision for several years. Finally, Euler regularly sent memoirs to St. Petersburg. About half his articles were published there in Latin, and the other half appeared in French in Berlin.
During this period, Euler greatly increased the variety of his investigations. Competing with d’Alembert and Daniel Bernoulli, he laid the foundations of mathematical physics; and he was a rival of both A. Clairaut and d’Alembert in advancing the theory of lunar and planetary motion. At the same time, Euler elaborated the theory of motion of solids, created the mathematical apparatus of hydrodynamics, successfully developed the differential geometry of surfaces, and intensively studied optics, electricity, and magnetism. He also pondered such problems of technology as the construction of achromatic refractors, the perfection of J.A. Segner’s hydraulic turbine, and the theory of toothed gearings.
During the Berlin period Euler prepared no fewer than 380 works, of which about 275 were published, including several lengthy books: a monograph on the calculus of variations (1744);^{13} a fundamental work on calculation of orbits (1745);^{14} the previously mentioned work on artillery and ballistics (1745); Introductio in analysin infinitorum (1748);^{15} a treatise on shipbuilding and navigation, prepared in an early version in St. Petersburg (1749);^{16} his first theory of lunar motion (1753);^{17} and Institutiones calculi differentialis (1755).^{18} The last three books were published at the expense of the St. Petersburg Academy. Finally, there was the treatise on the mechanics of solids, Theoria motus corporum solidorum seu rigidorum (1765).^{19} The famous Lettres à une princesse d’Allemagne sur divers sujets de physique et de philosophie, which originated in lessons given by Euler to a relative of the Prussian king, was not published until Euler’s return to St. Petersburg.^{20} Written in an absorbing and popular manner, the book was an unusual success and ran to twelve editions in the original French, nine in English, six in German, four in Russian, and two in both Dutch and Swedish. There were also Italian, Spanish, and Danish editions.
In the 1740’s and 1750’s Euler took part in several philosophical and scientific arguments. In 1745 and after, there were passionate discussions about the monadology of Leibniz and of Christian Wolff. German intellectuals were divided according to their opinions on monadology. As Euler later wrote, every conversation ended in a discussion of monads. The Berlin Academy announced as the subject of a 1747 prize competition an exposé and critique of the system. Euler, who was close to Cartesian mechanical materialism in natural philosophy, was an ardent enemy of monadology, as was Maupertuis. It should be added that Euler, whose religious views were based on a belief in revelation, could not share the religion of reason which characterized Leibniz and Wolff. Euler stated his objections, which were grounded on arguments of both a physical and theological nature, in the pamphlet Gedancken von den Elementen der Cörper... (1746).^{21} His composition caused violent debates, but the decision of the Academy gave the prize to Justi, author of a rather mediocre work against the theory of monads.
In 1751 a sensational new argument began when S. König published some critical remarks on Maupertuis’s principle of least action (1744) and cited a letter of Leibniz in which the principle was, in König’s opinion, formulated more precisely. Submitting to Maupertuis, the Berlin Academy rose to defend him and demanded that the original of Leibniz’ letter (a copy had been sent to König from Switzerland) be presented. When it became clear that the original could not be found, Euler published, with the approval of the Academy, “Exposé concernant l’examen de la lettre de M. de Leibnitz” (1752),^{22} where, among other things, he declared the letter a fake. The conflict grew critical when later in the same year Voltaire published his Diatribe du docteur Akakia, médecin du pape, defending König and making laughingstocks of both Maupertuis and Euler. Frederick rushed to the defense of Maupertuis, quarreling with his friend Voltaire and ordering the burning of the offensive pamphlet. His actions, however, did not prevent its dissemination throughout Europe. The argument touched not only on the pride of the principal participants but also on their general views: Maupertuis and, to a lesser degree, Euler interpreted the principle of least action theologically and teleologically; König was a follower of Wolff and Voltaire—the greatest ideologist of free thought.
Three other disputes in which Euler took part (all discussed below) were much more important for the development of mathematical sciences: his argument with d’Alembert on the problem of logarithms of negative numbers, the argument with d’Alembert and Daniel Bernoulli on the solution of the equation of a vibrating string, and Euler’s polemics with Dollond on optical problems.
As mentioned earlier, after Maupertuis died in 1759, Euler managed the Berlin Academy, but under the direct supervision of the king. But relations between Frederick and Euler had long since spoiled. They differed sharply, not only in their views but in their tastes, treatment of men, and personal conduct. Euler’s bourgeois manners and religious zeal were as unattractive to the king as the king’s passion for bons mots and freethinking was to Euler. Euler cared little for poetry, which the king adored; Frederick was quite contemptuous of the higher realms of mathematics, which did not seem to him immediately practical. In spite of having no one to replace Euler as manager of the Academy, the king, nonetheless, did not intend to give him the post of president. In 1763 it became known that Frederick wanted to appoint d’Alembert, and Euler thus began to think of leaving Berlin. He wrote to G. F. Müller, secretary of the St. Petersburg Academy, which had tried earlier to bring him back to Russia. Catherine the Great then ordered the academicians to send Euler another offer.
D’Alembert’s refusal to move permanently to Berlin postponed for a time the final decision on the matter. But during 1765 and 1766 grave conflicts over financial matters arose between Euler and Frederick, who interfered actively with Euler’s management of the Academy after the Seven Years’ War. The king thought Euler inexperienced in such matters and relied too much on the treasurer of the Academy. For half a year Euler pleaded for royal permission to leave, but the king, wellaware that the Academy would thus lose its best worker and principal force, declined to grant his request. Finally he had to consent and vented his annoyance in crude jokes about Euler. On 9 June 1766, Euler left Berlin, spent ten days in Warsaw at the invitation of Stanislas II, and arrived in St. Petersburg on 28 July. Euler’s three sons returned to Russia also. Johann Albrecht became academician in the chair of physics in 1766 and permanent secretary of the Academy in 1769. Christoph, who had become an officer in Prussia, successfully resumed his military career, reaching the rank of majorgeneral in artillery. Both his daughters also accompanied him.
Euler settled in a house on the embankment of the Neva, not far from the Academy. Soon after his return he suffered a brief illness, which left him almost completely blind in the left eye; he could not now read and could make out only outlines of large objects. He could write only in large letters with chalk and slate. An operation in 1771 temporarily restored his sight, but Euler seems not to have taken adequate care of himself and in a few days he was completely blind. Shortly before the operation, he had lost his house and almost all of his personal property in a fire, barely managing to rescue himself and his manuscripts. In November 1773 Euler’s wife died, and three years later he married her half sister, Salome Abigail Gsell.
Euler’s blindness did not lessen his scientific activity. Only in the last years of his life did he cease attending academic meetings, and his literary output even increased—almost half of his works were produced after 1765. His memory remained flawless, he carried on with his unrealized ideas, and he devised new plans. He naturally could not execute this immense work alone and was helped by active collaborators: his sons Johann Albrecht and Christoph; the academicians W. L. Krafft and A. J. Lexell; and two new young disciples, adjuncts N. Fuss, who was invited in 1772 from Switzerland, and M. E. Golovin, a nephew of Lomonosov. Sometimes Euler simply dictated his works; thus, he dictated to a young valet, a tailor by profession, the twovolume Vollstàndige Anleitung zur Algebra (l770),^{23} first published in Russian translation.
But the scientists assisting Euler were not mere secretaries; he discussed the general scheme of the works with them, and they developed his ideas, calculated tables, and sometimes compiled examples. The enormous, 775page Theoria motuum lunae... (1772)^{24} was thus completed with the help of Johann Albrecht, Krafft, and Lexell—all of whom are credited on the title page. Krafft also helped Euler with the threevolume Dioptrica (l7691771).^{25} Fuss, by his own account, during a sevenyear period prepared 250 memoirs, and Golovin prepared seventy. Articles written by Euler in his later years were generally concise and particular. For example, the fiftysix works prepared during 1776 contain about the same number of pages (1,000) as the nineteen works prepared in 1751.
Besides the works mentioned, during the second St. Petersburg period Euler published three volumes of Institutiones calculi integralis (1768–l770),^{26} the principal parts of which he had finished in Berlin, and an abridged edition of Scientia navalis—Théorie complette de la construction et de la manoeuvre des vaisseaux (1773).^{27} The last, a manual for naval cadets, was soon translated into English, Italian, and Russian, and Euler received for it large sums from the Russian and French governments.
The mathematical apparatus of the Dioptrica remained beyond the practical opticist’s understanding; so Fuss devised, on the basis of this work, the Instruction détaillée pour porter les lunettes de toutes les différentes espéces au plus haut degré de perfection dont elles sont susceptibles... (1774).^{28} Fuss also aided Euler in preparing the Éclaircissemens sur les érablissemens publics... (l776),^{29} which was very important in the development of insurance; many companies used its methods of solution and its tables.
Euler continued his participation in other functions of the St. Petersburg Academy. Together with Johann Albrecht he was a member of the commission charged in 1766 with the management of the Academy. Both resigned their posts on the commission in 1774 because of a difference of opinion between them and the director of the Academy, Count V. G. Orlov, who actually managed it.
On 18 September 1783 Euler spent the first half of the day as usual. He gave a mathematics lesson to one of his grandchildren, did some calculations with chalk on two boards on the motion of balloons; then discussed with Lexell and Fuss the recently discovered planet Uranus. About five o’clock in the afternoon he suffered a brain hemorrhage and uttered only “I am dying,” before he lost consciousness. He died about eleven o’clock in the evening.
Soon after Euler’s death eulogies were delivered by Fuss at a meeting of the St. Petersburg Academy^{30} and by Condorcet at the Paris Academy of Sciences.^{31} Euler was buried at the Lutheran Smolenskoye cemetery in St. Petersburg, where in 1837 a massive monument was erected at his grave, with the inscription, “Leonhardo Eulero Academia Petropolitana.” In the autumn of 1956 Euler’s remains and the monument were transferred to the necropolis of Leningrad.
Euler was a simple man, well disposed and not given to envy. One can also say of him what Fontenelle said of Leibniz: “He was glad to observe the flowering in other people’s gardens of plants whose seeds he provided.”
Mathematics . Euler was a geometer in the wide sense in which the word was used during the eighteenth century. He was one of the most important creators of mathematical science after Newton. In his work, mathematics was closely connected with applications to other sciences, to problems of technology, and to public life. In numerous cases he elaborated mathematical methods for the direct solution of problems of mechanics and astronomy, physics and navigation, geography and geodesy, hydraulics and ballistics, insurance and demography. This practical orientation of his work explains his tendency to prolong his investigations until he had derived a convenient formula for calculation or an immediate solution in numbers or a table. He constantly sought algorithms that would be simple to use in calculation and that would also assure sufficient accuracy in the results.
But just as his friend Daniel Bernoulli was first of all a physicist, Euler was first of all a mathematician. Bernoulli’s thinking was preeminently physical; he tried to avoid mathematics whenever possible, and once having developed a mathematical device for the solution of some physical problem, he usually left it without further development. Euler, on the other hand, attempted first of all to express a physical problem in mathematical terms; and having found a mathematical idea for solution, he systematically developed and generalized it. Thus, Euler’s brilliant achievements in the field are explained by his regular elaboration of mathematics as a single whole. Bernoulli was not especially attracted by more abstract problems of mathematics; Euler, on the contrary, was very much carried away with the theory of numbers. All this is manifest in the distribution of Euler’s works on various sciences: twentynine volumes of the Opera omnia (see BIBLIOGRAPHY [1]) pertain to pure mathematics.
In Euler’s mathematical work, first place belongs to analysis, which at the time was the most pressing need in mathematical science; seventeen volumes of the Opera omnia are in this area. Thus, in principle, Euler was an analyst. He contributed numerous particular discoveries to analysis, systematized its exposition in his classical manuals, and, along with all this, contributed immeasurably to the founding of several large mathematical disciplines: the calculus of variations, the theory of differential equations, the elementary theory of functions of complex variables, and the theory of special functions.
Euler is often characterized as a calculator of genius, and he was, in fact, unsurpassed in formal calculations and transformations and was even an outstanding calculator in the elementary sense of the word. But he also was a creator of new and important notions and methods, the principal value of which was in some cases properly understood only a century or more after his death. Even in areas where he, along with his contemporaries, did not feel at home, his judgment came, as a rule, from profound intuition into the subject under study. His findings were intrinsically capable of being grounded in the rigorous mode of demonstration that became obligatory in the nineteenth and twentieth centuries. Such standards were not, and could not be, demanded in the mathematics of the eighteenth century.
It is frequently said that Euler saw no intrinsic impossibility in the deduction of mathematical laws from a very limited basis in observation; and naturally he employed methods of induction to make empirical use of the results he had arrived at through analysis of concrete numerical material. But he himself warned many times that an incomplete induction serves only as a heuristic device, and he never passed off as finally proved truths the suppositions arrived at by such methods.
Euler introduced many of the present conventions of mathematical notation: the symbol e to represent the base of the natural system of logarithms (1727, published 1736); the use of letter f and of parentheses for a function f([x/a] + c) (1734, published 1740); the modern signs for trigonometric functions (1748); the notation fn for the sum of divisors of the number n (1750); notations for finite differences, Δy, Δ^{2}y, etc., and for the sum Σ(1755); and the letter i for , published 1794).
Euler had only a few immediate disciples, and none of them was a firstclass scientist. On the other hand, according to Laplace, he was a tutor of all the mathematicians of his time. In mathematics the eighteenth century can fairly be labeled the Age of Euler, but his influence upon the development of mathematical sciences was not restricted to that period. The work of many outstanding nineteenthcentury mathematicians branched out directly from the works of Euler.
Euler was especially important for the development of science in Russia. His disciples formed the first scientific mathematical school in the country and contributed to the rise of mathematical education. One can trace back to Euler numerous paths from Chebyshev’s St. Petersburg mathematical school.
[In the following, titles of articles are not, as a rule, cited; dates in parentheses signify the year of publication.]
Theory of Numbers . Problems of the theory of numbers had attracted mathematicians before Euler. Fermat, for example, established several remarkable arithmetic theorems but left almost no proofs. Euler laid the foundations of number theory as a true science.
A large series of Euler’s works is connected with the theory of divisibility. He proved by three methods Fermat’s lesser theorem, the principal one in the field (1741, 1761, 1763); he suggested with the third proof an important generalization of the theorem by introducing Euler’s function φ(n), denoting the number of positive integers less than n which are relatively prime to n: the difference a^{φn}1 is divisible by n if a is relatively prime to n. Elaborating related ideas, Euler came to the theory of nic residues (1760). Here his greatest discovery was the law of quadratic reciprocity (1783), which, however, he could not prove. Euler’s discovery went unnoticed by his contemporaries, and the law was rediscovered, but incompletely proved, by A. M. Legendre (1788). Legendre was credited with it until Chebyshev pointed out Euler’s priority in 1849. The complete proof of the law was finally achieved by Gauss (1801). Gauss, Kummer, D. Hilbert, E. Artin, and others extended the law of reciprocity to various algebraic number fields; the most general law of reciprocity was established by I. R. Shafarevich (1950).
Another group of Euler’s works, in which he extended Fermat’s studies on representation of prime numbers by sums of the form m x^{2}+n y^{2}, where m, n, x, and y are positive integers, led him to the discovery of a new efficient method of determining whether a given large number N is prime or composite (1751, et seq.). These works formed the basis for the general arithmetic theory of binary quadratic forms developed by Lagrange and especially by Gauss.
Euler also contributed to socalled Diophantine analysis, that is, to the solution, in integers or in rational numbers, of indeterminate equations with integer coefficients. Thus, by means of continued fractions, which he had studied earlier (1744, et seq.), he gave (1767) a method of calculation of the smallest integer solution of the equation x^{2}d y^{2}=1 (d being a positive nonsquare integer). This had been studied by Fermat and Wallis and even earlier by scientists of India and Greece. A complete investigation of the problem was soon undertaken by Lagrange. In 1753 Euler proved the impossibility of solving x^{3}+y^{3}=z^{3} in which x, y, and z are integers, xyz ≠0 (a particular case of Fermat’s last theorem); his demonstration, based on the method of infinite descent and using complex numbers of the form , is thoroughly described in his Vllstàndige Anleitung zur Algebra, the second volume of which (1769) has a large section devoted to Diophantine analysis.
In all these cases Euler used methods of arithmetic and algebra, but he was also the first to use analytical methods in number theory. To solve the partition problem posed in 1740 by P. Naudé, concerning the total number of ways the positive integer n is obtainable as a sum of positive integers m < n, Euler used the expansions of certain infinite products into a power series whose coefficients give the solution (1748). In particular, in the expansion the righthand series is one of theta functions, introduced much later by C. Jacobi in his theory of elliptic functions. Earlier, in 1737, Euler had deduced the famous identity where the sum extends over all positive integers n and the product over all primes p (1744), the lefthand side is what Riemann later called the zetafunction ζ(ς)
Using summation of divergent series and induction, Euler discovered in 1749 (1768) a functional equation involving ζ(s), ζ(1s), and Γ(s), which was rediscovered and established by Riemann, the first scientist to define the zetafunction also for complex values of the argument. In the nineteenth and twentieth centuries, the zetafunction became one of the principal means of analytic number theory, particularly in the studies of the laws of distribution of prime numbers by Dirichlet, Chebyshev, Riemann, Hadamard, de la VallèePoussin, and others.
Finally, Euler studied mathematical constants and formulated important problems relevant to the theory of transcendental numbers. His expression of the number e in the form of a continued fraction (1744) was used by J. H. Lambert (1768) in his demonstration of irrationality of the numbers e and π. F. Lindemann employed Euler’s formula Ln(1) = πί (discovered as early as 1728) to prove that is transcendental (1882). The hypothesis of the transcendence of a^{b}, where a is any algebraic number ≠0,1 and b is any irrational algebraic number—formulated by D. Hilbert in 1900 and proved by A. Gelfond in 1934—presents a generalization of Euler’s corresponding supposition about rationalbase logarithms of rational numbers (1748).
Algebra . When mathematicians of the seventeenth century formulated the fundamental theorem that an algebraic equation of degree n with real coefficients has n roots, which could be imaginary, it was yet unknown whether the domain of imaginary roots was restricted to numbers of the form a + bi, which, following Gauss, are now called complex numbers. Many mathematicians thought that there existed imaginary quantities of another kind. In his letters to Nikolaus I Bernoulli and to Goldbach (dated 1742), Euler stated for the first time the theorem that every algebraic polynomial of degree n with real coefficients may be resolved into real linear or quadratic factors, that is, possesses n roots of the form a + bi (1743). The theorem was proved by d’Alembert (1748) and by Euler himself (1751). Both proofs, quite different in ideas, had omissions and were rendered more precise during the nineteenth century.
Euler also aspired—certainly in vain—to find the general form of solution by radicals for equations of degree higher than the fourth (1738, 1764). He elaborated approximating methods of solutions for numerical equations (1748) and studied the elimination problem. Thus, he gave the first proof of the theorem, which was known to Newton, that two algebraic curves of degrees m and n, respectively, intersect in mn points (1748, 1750). It should be added that Euler’s Vollständige Anleitung zur Algebra, published in many editions in English, Dutch, Italian, French, and Russian, greatly influenced nineteenth and twentiethcentury texts on the subject.
Infinite Series . In Euler’s works, infinite series, which previously served mainly as an auxiliary means for solving problems, became a subject of study. One example, his investigation of the zetafunction, has already been mentioned. The point of departure was the problem of summation of the reciprocals of the squares of the integers
which had been vainly approached by the Bernoulli brothers, Stirling, and other outstanding mathematicians. Euler solved in 1735 a much more general problem and demonstrated that for any even integer number 2k > 0,
ζ(2k)=a_{2k}π^{s k},
where a_{2k} are rational numbers (1740), expressed through coefficients of the EulerMaclaurin summation formula (1750) and, consequently, through Bernoulli numbers (1755). The problem of the arithmetic nature of ζ(2k + 1) remains unsolved.
The summation formula was discovered by Euler no later than 1732 (1738) and demonstrated in 1735 (1741); it was independently discovered by Maclaurin no later than 1738 (1742). The formula, one of the most important in the calculus of finite differences, represents the partial sum of a series, , by another infinite series involving the integral and the derivatives of the general term u(n). Later Euler expressed the coefficients of the latter series through Bernoulli numbers (1755). Euler knew that although this infinite series generally diverges, its partial sums under certain conditions might serve as a brilliant means of approximating the calculations shown by James Stirling (1730) in a particular case of
By means of the summation formula, Euler in 1735 calculated (1741) to sixteen decimal places the value of Euler’s constant,
C = 0.57721566...,
belonging to an asymptotic formula,
which he discovered in 1731 (1738).
The functions studied in the eighteenth century were, with rare exceptions, analytic, and therefore Euler made great use of power series. His special merit was the introduction of a new and extremely important class of trigonometric Fourier series. In a letter to Goldbach (1744), he expressed for the first time an algebraic function by such a series (1755),
He later found other expansions (1760), deducing in 1777 a formula of Fourier coefficients for expansion of a given function into a series of cosines on the interval (0,π), pointing out that coefficients of expansion into a series of sines could be deduced analogously (1798). Fourier, having no knowledge of Euler’s work, deduced in 1807 the same formulas. For his part, Euler did not know that coefficients of expansion into a series of cosines had been given by Clairaut in 1759.
Euler also introduced expansion of functions into infinite products and into the sums of elementary fractions, which later acquired great importance in the general theory of analytic functions. Numerous methods of transformation of infinite series, products, and continued fractions into one another are also his.
Eighteenthcentury mathematicians distinguished convergent series from divergent series, but the general theory of convergence was still missing. Algebraic and analytic operations on infinite series were similar to those on finite polynomials, without any restrictions. It was supposed that identical laws operate in both cases. Several tests of convergence already known found almost no application. Opinions, however, differed on the problem of admissibility of divergent series. Many mathematicians were radically against their employment. Euler, sure that important correct results might be arrived at by means of divergent series, set about the task of establishing the legitimacy of their application. With this aim, he suggested a new, wider definition of the concept of the sum of a series, which coincides with the traditional definition if the series converges; he also suggested two methods of summation (1755). Precise grounding and further development of these fruitful ideas were possible only toward the end of the nineteenth century and the beginning of the twentieth century.^{32}
The Concept of Function . Discoveries in the field of analysis made in the middle of the eighteenth century (many of them his own) were systematically summarized by Euler in the trilogy Introductio in analysin infinitorum (1748),^{15}Institutiones calculi differentialis (1755),^{18} and Institutiones calculi integralis (17681770). The books are still of interest, especially the first volume of the Introductio. Many of the problems considered there, however, are now so far developed that knowledge of them is limited to a few specialists, who can trace in the book the development of many fruitful methods of analysis.
In the Introductio Euler presented the first clear statement of the idea that mathematical analysis is a science of functions; and he also presented a more thorough investigation of the very concept of function. Defining function as an analytic expression somehow composed of variables and constants—following in this respect Johann I Bernoulli (1718)— Euler defined precisely the term “analytic expression”: functions are produced by means of algebraic operations, and also of elementary and other transcendental operations, carried out by integration. Here the classification of functions generally used today is also given; Euler speaks of functions defined implicitly and by parametric representation. Further on he states his belief, shared by other mathematicians, that all analytic expressions might be given in the form of infinite power series or generalized power series with fractional or negative exponents. Thus, functions studied in mathematical analysis generally are analytic functions with some isolated singular points. Euler’s remark that functions are considered not only for real but also for imaginary values of independent variables was very important.
Even at that time, however, the class of analytic functions was insufficient for the requirements of analysis and its applications, particularly for the solution of the problem of the vibrating string. Here Euler encountered “arbitrary” functions, geometrically represented in piecewise smooth plane curves of arbitrary form—functions which are, generally speaking, nonanalytic (1749). The problem of the magnitude of the class of functions applied in mathematical physics and generally in analysis and the closely related problem of the possibility of analytic expression of nonanalytic functions led to a lengthy polemic involving many mathematicians, including Euler, d’Alembert, and Daniel Bernoulli. One of the results of this controversy over the problem of the vibrating string was the general arithmetical definition of a function as a quantity whose values somehow change with the changes of independent variables; the definition was given by Euler in Institutiones calculi differentialis.^{18} He had, however, already dealt with the interpretation of a function as a correspondence of values in his introductio.
Elementary Functions . The major portion of the first volume of the Introductio is devoted to the theory of elementary functions, which is developed by means of algebra and of infinite series and products. Concepts of infinitesimal and infinite quantity are used, but those of differential and integral calculus are lacking. Among other things, Euler here for the first time described the analytic theory of trigonometric functions and gave a remarkably simple, although nonrigorous, deduction of Moivre’s formula and also of his own (1743),
e^{±xi} = cos x ± i sin x.
This was given earlier by R. Cotes (1716) in a somewhat different formulation, but it was widely used only by Euler. The logarithmic function was considered by Euler in the Introductio only for the positive independent variable. However, he soon published his complete theory of logarithms of complex numbers (1751)—which some time before had ended the arguments over logarithms of negative numbers between Leibniz and Johann Bernoulli and between d’Alembert and Euler himself in their correspondence (17471748). Euler had come across the problem (17271728) when he discussed in his correspondence with Johann I Bernoulli the problem of the graphics of the function y = (1)^{x} and arrived at the equality ln(1)= πi.
Functions of a Complex Variable . The study of elementary functions brought d’Alembert (17471748) and Euler (1751) to the conclusion that the domain of complex numbers is closed (in modern terms) with regard to all algebraic and transcendental operations. They both also made early advances in the general theory of analytic functions. In 1752 d’Alembert, investigating problems of hydrodynamics, discovered equations connecting the real and imaginary parts of an analytic function u(x,y) + iv(x,y). In 1777 Euler deduced the same equations, from general analytical considerations, developing a new method of calculation of definite integrals f f(z) dz by means of an imaginary substitution
z = x + iy
(1793, 1797). He thus discovered (1794) that
Euler also used analytic functions of a complex variable, both in the study of orthogonal trajectories by means of their conformal mapping (1770) and in his works on cartography (1778). (The term projectio conformis was introduced by a St. Petersburg academician, F. T. Schubert [1789].) All of these ideas were developed in depth in the elaboration of the general theory of analytic functions by Cauchy (1825) and Riemann (1854), after whom the abovecited equations of d’Alembert and Euler are named.
Although Euler went from numbers of the form x + iy to the point u(x,y) and back, and used a trigonometric form r(cos φ + i sinφ), he saw in imaginary numbers only convenient notations void of real meaning. A somewhat less than successful attempt at geometric interpretation undertaken by H. Kühn (1753) met with sharp critical remarks from Euler.
Differential and Integral Calculus . Both branches of infinitesimal analysis were enriched by Euler’s numerous discoveries. Among other things in the Institutiones calculi differentialis, he thoroughly elaborated formulas of differentiation under substitution of variables; revealed his theorem on homogeneous functions, stated for f(x,y) as early as 1736; proved the theorem of Nikolaus I Bernoulli (1721) that for z = f(x,y)
deduced the necessary condition for the exact differential of f(x,y); applied Taylor’s series to finding extrema of f(x); and investigated extrema of f(x,y), inaccurately formulating, however, sufficient conditions.
The first two chapters of the Institutiones are devoted to the elements of the calculus of finite differences. Euler approached differential calculus as a particular case, we would say a limiting case, of the method of finite differences used when differences of the function and of the independent variable approach zero. During the eighteenth century it was often said against differential calculus that all its formulas were incorrect because the deductions were based on the principle of neglecting infinitely small summands, e.g., on equalities of the kind a + α = a, where α is infinitesimal with respect to a. Euler thought that such criticism could be obviated only by supposing all infinitesimals and differentials equal to zero, and therefore he elaborated an original calculus of zeroes. This concept, although not contradictory in itself, did not endure because it proved insufficient in many problems; a strict grounding of analysis was possible if the infinitesimals were interpreted as variables tending to the limit zero.
The methods of indefinite integration in the Institutiones calculi integralis (I, 1768) are described by Euler in quite modern fashion and in a detail that practically exhausts all the cases in which the result of integration is expressible in elementary functions. He invented many of the methods himself; the expression “Euler substitution” (for rationalization of certain irrational differentials) serves as a reminder of the fact. Euler calculated many difficult definite integrals, thus laying the foundations of the theory of special functions. In 1729, already studying interpolation of the sequence 1!, 2!,..., n!,..., he introduced Eulerian integrals of the first and second kind (Legendre’s term), today called the betaand gammafunctions (1738). He later discovered a number of their properties.
Particular cases of the betafunction were first considered by Wallis in 1656. The functions B and Γ, together with the zetafunction and the socalled Bessel functions (see below), are among the most important transcendental functions. Euler’s main contribution to the theory of elliptic integrals was his discovery of the general addition theorem (1768). Finally, the theory of multiple integrals also goes back to Euler; he introduced double integrals and established the rule of substitution (1770).
Differential Equations . The Institutiones calculi integralis exhibits Euler’s numerous discoveries in the theory of both ordinary and partial differential equations, which were especially useful in mechanics.
Euler elaborated many problems in the theory of ordinary linear equations: a classical method for solving reduced linear equations with constant coefficients, in which he strictly distinguished between the general and the particular integral (1743); works on linear systems, conducted simultaneously with d’Alembert (1750); solution of the general linear equation of order n with constant coefficients by reduction to the equation of the same form of order n  1 (1753). After 1738 he successfully applied to secondorder linear equations with variable coefficients a method that was highly developed in the nineteenth century; this consisted of the presentation of particular solutions in the form of generalized power series. Another Eulerian device, that of expressing solutions by definite integrals that depend on a parameter (1763), was extended by Laplace to partial differential equations (1777).
One can trace back to Euler (1741) and Daniel Bernoulli the method of variation of constants later elaborated by Lagrange (1777). The method of an integrating factor was also greatly developed by Euler, who applied it to numerous classes of firstorder differential equations (1768) and extended it to higherorder equations (1770). He devoted a number of articles to the Riccati equation, demonstrating its involvement with continued fractions (1744). In connection with his works on the theory of lunar motion, Euler created the widely used device of approximating the solution of the equation dy/dx = f(x,y), with initial condition x = x_{0}, y = y_{0} (1768), extending it to secondorder equations (1769). This Euler method of open polygons was used by Cauchy in the 1820’s to demonstrate the existence theorem for the solution of the abovementioned equation (1835, 1844). Finally, Euler discovered tests for singular solutions of firstorder equations (1768).
Among the large cycle of Euler’s works on partial differential equations begun in the middle of the 1730’s with the study of separate kinds of firstorder equations, which he had encountered in certain problems of geometry (1740), the most important are the studies on secondorder linear equations—to which many problems of mathematical physics may be reduced. First was the problem of small plane vibrations of a string, the wave equation originally solved by d’Alembert with the socalled method of characteristics. Given a general solution expressible as a sum of two arbitrary functions, the initial conditions and the boundary conditions of the problem admitted of arriving at solutions in concrete cases (1749). Euler immediately tested this method of d’Alembert’s and further elaborated it, eliminating unnecessary restrictions imposed by d’Alembert upon the initial shape and velocity of the string (1749). As previously mentioned, the two mathematicians engaged in an argument which grew more involved when Daniel Bernoulli asserted that any solution of the wave equation might be expressed by a trigonometric series (1755). D’Alembert and Euler agreed that such a solution could not be sufficiently general. The discussion was joined by Lagrange, Laplace, and other mathematicians of great reputation and lasted for over half a century; not until Fourier (1807, 1822) was the way found to the correct formulation and solution of the problem. Euler later developed the method of characteristics more thoroughly (1766, 1767).
Euler encountered equations in other areas of what became mathematical physics: in hydrodynamics; in the problem of vibrations of membranes, which he reduced to the socalled Bessel equation and solved (1766) by means of the Bessel functions J_{n}(x); and in the problem of the motion of air in pipes (1772). Some classes of equations studied by Euler for velocities close to or surpassing the velocity of sound continue to figure in modern aerodynamics.
Calculus of Variations . Starting with several problems solved by Johann and Jakob Bernoulli, Euler was the first to formulate the principal problems of the calculus of variations and to create general methods for their solution. In Methodus inveniendi lineas curvas...^{13} he systematically developed his discoveries of the 1730’s (1739, 1741). The very title of the work shows that Euler widely employed geometric representations of functions as flat curves. Here he introduced, using different terminology, the concepts of function and variation and distinguished between problems of absolute extrema and relative extrema, showing how the latter are reduced to the former. The problem of the absolute extremum of the function of several independent variables, where F is the given and y(x) the desired minimizing or maximizing function, is treated as the limiting problem for the ordinary extremum of the function where x_{k} = a+k Δx, Δx =(b  a)/n, k = 0, 1,..., n (and→∞). Thus Euler deduced the differential equation named after him to which the function y(x) should correspond; this necessary condition was generalized for the case where F involves the derivatives y’, y“,..., y^{n}. In this way the solution of a problem in the calculus of variations might always be reduced to integration of a differential equation. A century and a half later the situation had changed. The direct method imagined by Euler, which he had employed only to obtain his differential equation, had (together with similar methods) acquired independent value for rigorous or approximate solution of variational problems and the corresponding differential equations.
In the mid1750’s, after Lagrange had created new algorithms and notations for the calculus of variations, Euler abandoned the former exposition and gave instead a detailed and lucid exposition of Lagrange’s method, considering it a new calculus—which he called variational (1766). He applied the calculus of variations to problems of extreme values of double integrals with constant limits in volume III of the Institutiones calculi integralis (1770); soon thereafter he suggested still another method of exposition of the calculus, one which became widely used.
Geometry . Most of Euler’s geometrical discoveries were made by application of the methods of algebra and analysis. He gave two different methods for an analytical exposition of the system of spherical trigonometry (1755, 1782). He showed how the trigonometry of spheroidal surfaces might be applied to higher geodesy (1755). In volume II of the Introductio he surpassed his contemporaries in giving a consistent algebraic development of the theory of secondorder curves, proceeding from their general equation (1748). He constituted the theory of thirdorder curves by analogy. But Euler’s main achievement was that for the first time he studied thoroughly the general equation of secondorder surfaces, applying Euler angles in corresponding transformations.
Euler’s studies of the geodesic lines on a surface are prominent in differential geometry; the problem was pointed out to him by Johann Bernoulli (1732, 1736, and later). But still more important were his pioneer investigations in the theory of surfaces, from which Monge and other geometers later proceeded. In 1763 Euler made the first substantial advance in the study of the curvature of surfaces; in particular, he expressed the curvature of an arbitrary normal section by principal curvatures (1767). He went on to study developable surfaces, introducing Gaussian coordinates (1772), which became widely used in the nineteenth century. In a note written about 1770 but not published until 1862 Euler discovered the necessary condition for applicability of surfaces that was independently established by Gauss (1828). In 1775 Euler successfully renewed elaboration of the general theory of space curves (1786), beginning where Clairaut had left off in 1731.
Euler was also the author of the first studies on topology. In 1735 he gave a solution to the problem of the seven bridges of Königsberg: the bridges, spanning several arms of a river, must all be crossed without recrossing any (1741). In a letter to Goldbach (1750), he cited (1758) a number of properties of polyhedra, among them the following: the number of vertices, S, edges, A, and sides, H, of a polyhedron are connected by an equality S  A + H = 2. A hundred years later it was discovered that the theorem had been known to Descartes. The Euler characteristic S  A + H and its generalization for multidimensional complexes as given by H. Poincaré is one of the principal invariants of modern topology.
Mechanics . In an introduction to the Mechanica (1736) Euler outlined a large program of studies embracing every branch of the science. The distinguishing feature of Euler’s investigations in mechanics as compared to those of his predecessors is the systematic and successful application of analysis. Previously the methods of mechanics had been mostly synthetic and geometrical; they demanded too individual an approach to separate problems. Euler was the first to appreciate the importance of introducing uniform analytic methods into mechanics, thus enabling its problems to be solved in a clear and direct way. Euler’s concept is manifest in both the introduction and the very title of the book, Mechanica sine motus scientia analytice exposita.
This first large work on mechanics was devoted to the kinematics and dynamics of a pointmass. The first volume deals with the free motion of a pointmass in a vacuum and in a resisting medium; the section on the motion of a pointmass under a force directed to a fixed center is a brilliant analytical reformulation of the corresponding section of Newton’s Principia; it was sort of an introduction to Euler’s further works on celestial mechanics. In the second volume, Euler studied the constrained motion of a pointmass; he obtained three equations of motion in space by projecting forces on the axes of a moving trihedral of a trajectory described by a moving point, i.e., on the tangent, principal normal, and binormal. Motion in the plane is considered analogously. In the chapter on the motion of a point on a given surface, Euler solved a number of problems of the differential geometry of surfaces and of the theory of geodesics.
The Theoria motus corporum solidorum^{19} published almost thirty years later (1765), is related to the Mechanica. In the introduction to this work, Euler gave a new exposition of punctual mechanics and followed Maclaurin’s example (1742) in projecting the forces onto the axes of a fixed orthogonal rectilinear system. Establishing that the instantaneous motion of a solid body might be regarded as composed of rectilinear translation and instant rotation, Euler devoted special attention to the study of rotatory motion. Thus, he gave formulas for projections of instantaneous angular velocity on the axes of coordinates (with application of Euler angles), and framed dynamical differential equations referred to the principal axes of inertia, which determine this motion. Special mention should be made of the problem of motion of a heavy solid body about a fixed point, which Euler solved for a case in which the center of gravity coincides with the fixed point. The law of motion in such a case is, generally speaking, expressed by means of elliptic integrals. Euler was led to this problem by the study of precession of the equinoxes and of the nutation of the terrestrial axis (175l).^{33} Other cases in which the differential equations of this problem can be integrated were discovered by Lagrange (1788) and S. V. Kovalevskaya (1888). Euler considered problems of the mechanics of solid bodies as early as the first St. Petersburg period.
In one of the two appendixes to the Methodus...^{13} Euler suggested a formulation of the principle of least action for the case of the motion of a point under a central force: the trajectory described by the point minimizes the integral f mu ds. Maupertuis had stated at nearly the same time the principle of least action in a much more particular form. Euler thus laid the mathematical foundation of the numerous studies on variational principles of mechanics and physics which are still being carried out.
In the other appendix to the Methodus, Euler, at the insistence of Daniel Bernoulli, applied the calculus of variations to some problems of the theory of elasticity, which he had been intensively elaborating since 1727. In this appendix, which was in fact the first general work on the mathematical theory of elasticity, Euler studied bending and vibrations of elastic bands (either homogeneous or nonhomogeneous) and of a plate under different conditions; considered nine types of elastic curves; and deduced the famous Euler buckling formula, or Euler critical load, used to determine the strength of columns.
Hydromechanics . Euler’s first large work on fluid mechanics was Scientia novalis. Volume I contains a general theory of equilibrium of floating bodies including an original elaboration of problems of stability and of small oscillations in the neighborhood of an equilibrium position. The second volume applies general theorems to the case of a ship.
From 1753 to 1755 Euler elaborated in detail an analytical theory of fluid mechanics in three classic memoirs—“Principes généraux de l’état d’équilibre des fluides” “Principes généraux du mouvement des fluides”; and “Continuation des recherches sur la théorie du mouvement des fluides”—all published simultaneously (1757).^{34} Somewhat earlier (1752) the “Principia motus fluidorum” was written; it was not published, however, until 176l.^{35} Here a system of principal formulas of hydrostatics and hydrodynamics was for the first time created; it comprised the continuity equation for liquids with constant density; the velocitypotential equation (usually called after Laplace); and the general Euler equations for the motion of an incompressible liquid, gas, etc. As has generally been the case in mathematical physics, the main innovations were in the application of partial differential equations to the problems. At the beginning of the “Continuation des recherches” Euler emphasized that he had reduced the whole of the theory of liquids to two analytic equations and added:
However sublime are the researches on fluids which we owe to the Messrs. Bernoulli, Clairaut and d’Alembert, they flow so naturally from my two general formulae that one cannot sufficiently admire this accord of their profound meditations with the simplicity of the principles from which I have drawn my two equations, and to which I was led immediately by the first axioms of mechanics.^{36}
Euler also investigated a number of concrete problems on the motion of liquids and gases in pipes, on vibration of air in pipes, and on propagation of sound. Along with this, he worked on problems of hydrotechnology, discussed, in part, above. Especially remarkable were the improvements he introduced into the design of a hydraulic machine imagined by Segner in 1749 and the theory of hydraulic turbines, which he created in accordance with the principle of action and reaction (1752–1761).^{37}
Astronomy . Euler’s studies in astronomy embraced a great variety of problems: determination of the orbits of comets and planets by a few observations, methods of calculation of the parallax of the sun, the theory of refraction, considerations on the physical nature of comets, and the problem of retardation of planetary motions under the action of cosmic ether. His most outstanding works, for which he won many prizes from the Paris Académie des Sciences, are concerned with celestial mechanics, which especially attracted scientists at that time.
The observed motions of the planets, particularly of Jupiter and Saturn, as well as the moon, were evidently different from the calculated motions based on Newton’s theory of gravitation. Thus, the calculations of Clairaut and d’Alembert (1745) gave the value of eighteen years for the period of revolution of the lunar perigee, whereas observations showed this value to be nine years. This caused doubts about the validity of Newton’s system as a whole. For a long time Euler joined these scientists in thinking that the law of gravitation needed some corrections. In 1749 Clairaut established that the difference between theory and observation was due to the fact that he and others solving the corresponding differential equation had restricted themselves to the first approximation. When he calculated the second approximation, it was satisfactorily in accordance with the observed data. Euler did not at once agree. To put his doubts at rest, he advised the St. Petersburg Academy to announce a competition on the subject. Euler soon determined that Clairaut was right, and on Euler’s recommendation his composition received the prize of the Academy (1752). Euler was still not completely satisfied, however. In 1751 he had written his own Theoria motus lunae exhibens omnes ejus inaequalitates (published in 1753), in which he elaborated an original method of approximate solution to the threebody problem, the socalled first Euler lunar theory. In the appendix he described another method which was the earliest form of the general method of variation of elements. Euler’s numerical results also conformed to Newton’s theory of gravitation.
The first Euler lunar theory had an important practical consequence: T. Mayer, an astronomer from Göttingen, compiled, according to its formulas, lunar tables (1755) that enabled the calculation of the position of the moon and thus the longitude of a ship with an exactness previously unknown in navigation. The British Parliament had announced as early as 1714 a large cash prize for the method of determination of longitude at sea with error not to exceed half a degree, and smaller prizes for less exact methods. The prize was not awarded until 1765; £ 3,000 went to Mayer’s widow and £300 to Euler for his preliminary theoretical work. Simultaneously a large prize was awarded to J. Harrison for his construction of a more nearly perfect chronometer. Lunar tables were included in all nautical almanacs after 1767, and the method was used for about a century.
From 1770 to 1772 Euler elaborated his second theory of lunar motion, which he published in the Theoria motuum lunae, nova methodo pertractata (1772).^{24} For various reasons, the merits of the new method could be correctly appreciated only after G. W. Hill brilliantly developed the ideas of the composition in 18771888.
Euler devoted numerous works to the calculation of perturbations of planetary orbits caused by the mutual gravitation of Jupiter and Saturn (1749, 1769) as well as of the earth and the other planets (1771). He continued these studies almost to his death.
Physics . Euler’s principal contribution to physics consisted in mathematical elaboration of the problems discussed above. He touched upon various physical problems which would not yield to mathematical analysis at that time. He aspired to create a uniform picture of the physical world. He had been, as pointed out earlier, closer to Cartesian natural philosophy than to Newtonian, although he was not a direct representative of Cartesianism. Rejecting the notion of empty space and the possibility of action at a distance, he thought that the universe is filled up with ether—a thin elastic matter with extremely low density, like superrarified air. This ether contains material particles whose main property is impenetrability. Euler thought it possible to explain the diversity of the observed phenomena (including electricity, light, gravitation, and even the principle of least action) by the hypothetical mechanical properties of ether. He also had to introduce magnetic whirls into the doctrine of magnetism; these are even thinner and move more quickly than ether.
In physics Euler built up many artificial models and hypotheses which were shortlived. But his main concept of the unity of the forces of nature acting deterministically in some medium proved to be important for the development of physics, owing especially to Lettres à une princesse d’Allemagne. Thus, his views on the nature of electricity were the prototype of the theory of electric and magnetic fields of Faraday and Maxwell. His theory of ether influenced Riemann.
Euler’s works on optics were widely known and important in the physics of the eighteenth century. Rejecting the dominant corpuscular theory of light, he constructed his own theory in which he attributed the cause of light to peculiar oscillations of ether. His Nova theoria lucis et colorum(1746)^{38}explained some, but not all, phenomena. Proceeding from certain analogies that later proved incorrect, Euler concluded that the elimination of chromatic aberration of optic lenses was possible (1747); he conducted experiments with lenses filled with water to confirm the conclusion. This provoked objections by the English optician Dollond, who, following Newton, held that dispersion was inevitable. The result of this polemic, in which both parties were partly right and partly wrong, was the creation by Dollond of achromatic telescopes (1757), a turning point in optical technology. For his part, Euler, in his Dioptrica, laid the foundations of the calculation of optical systems.
NOTES
All works cited are listed in the BIBLIOGRAPHY. References to Euler’s Opera omnia(see [1] in BIBLIOGRAPHY) include series and volume number.
1. 20, p. 75
2. “Constructio linearum isochronarum in medio quocunque resistente,” in 1, 2nd ser., VI, p. 1.
3. “Methodus inveniendi traiectorias reciprocas algebraicas,” in 1, 1st ser., XXVII, p. 1.
4. To be published in 1, 2nd ser., XX.
5. 1, 3rd ser., 1p. 181.
6. 26, p. 51.
7. 13, II , p. 182.
8Einleitung zur RechenKunst zum Gebrauch des Gymnasii bey der Kayserlichen Academie der Wissenschafften in St. Petersburg (St. Petersburg, 17381740). See 1, 3rd ser., II, 1303.
9.Mechanica sine motus scientia analytice exposita, 2 vols. (St. Petersburg, 1736). See 1, 2nd ser., I and II.
10. 20, p. 77.
11.Neue Grudsätze der Artillerie aus dem Englischen des Herrn Benjamin Robins übersetzt und mit vielen Anmerkungen versehen (Berlin, 1745). See 1, 2nd ser., XIV.
12. See 1, 2nd ser., XIV, 468477.
13.Methodus inveniendi lineas curvas maximi minimive proprietate gaudentes (LausanneGeneva, 1744). See 1, 1st ser., XXIV.
14.Theoria motuum planetarum et cometarum (Berlin, 1744). See 1, 2nd ser., XXVIII, 105251.
15.Introductio in analysin infinitorum, 2 vols. (Lausanne, 1748). See 1, 1st ser., VIII and IX.
16.Scientia navalis, 2 vols. (St. Petersburg, 1749). See 1, 2nd ser., XVIII and XIX.
17.Theoria motus lunae(Berlin, 1753). See 1, 2nd ser., XXIII, 64336.
18.Institutiones calculi differentialis cum eius usu in analyst finitorum ac doctrina serierum(Berlin, 1755). See 1, 1st ser., X .
19.Theoria motus corporum solidorum seu rigidorum ex primis nostrae cognitionis principiis stabilita... (RostockGreifswald, 1765). See 1, 2nd ser., III and IV.
20. The work, which comprises 234 letters, was published at St. Petersburg in 3 vols. The first two vols. (letters 1154) appeared in 1768; vol. III appeared in 1772. See 1, 3rd ser., XI and XII.
21.Gedancken von den Elementen der Cörper, in welchen das LehrGebäude von den einfachen Dingen und Monaden geprüfet und das wahre Wesen der Cörper entdecket wird (Berlin, 1746). See 1, 3rd ser., II, 347366.
22. “Exposé concernant l’examen de la lettre de M. de Leibnitz, allégueé par M. le Professeur Koenig, dans le mois de mars 1751 des Actes de Leipzig, à l’occasion du principe de la moindre action.” See 1, 2nd ser., V, 6473.
23. The work was first published at St. Petersburg in Russian (vol. I, 1768; vol. II, 1769). It then appeared in a twovolume German edition (St. Petersburg, 1770). See 1, 1st ser., I.
24.Theoria motuum lunae, nova methodo pertractata (St. Petersburg, 1772). See 1, 2nd ser., XXII.
25. The work was published sequentially, in 3 vols., at St. Petersburg. Vol. I deals with principles of optics (1769); vol. II with construction of telescopes (1770); and vol. III with construction of microscopes (1771). See 1, 3rd ser., III and IV.
26. The work’s 3 vols. were published sequentially in St. Petersburg in 1768, 1769, and 1770. See 1, 1st ser., III and XIII.
27. To be published in 1, 2nd ser., XXI.
28. See 1, 3rd ser., VII, 200247.
29.Éclaircissemens sur les établissemens publics en faveur tant des veuves que des morts, avec la déscription d’une nouvelle espéce de tontine aussi favorable au public qu’utile à l’etat (St. Petersburg, 1776). See 1, 1st ser., VII, 181245.
30. See 17.
31. Condorcet’s éloge was first published in Histoire de l’Académie royale des sciences pour l’année 1783 (Paris, 1786), pp. 3768. It is reprinted in 1, 3rd ser., XII, 287310.
32. See 50, chs.12.
33. “Recherches sur la précession des équinoxes et sur la nutation de l’axe de la terre.” See 1, 2nd ser., XXIX, 92123.
34. See 1, 2nd ser., XII, 2132.
35. See 1, 2nd ser., XII, 133168.
36. See 1, 2nd ser., XII, 92, for the original French.
37. See 1, 2nd ser., XV, pt. 1, 139, 80104, 157218.
38. See 1, 3rd ser., V, 145.
BIBLIOGRAPHY
1. Original Works. Euler wrote and published more than any other mathematician. During his lifetime about 560 books and articles appeared, and he once remarked to Count Orlov that he would leave enough memories to fill the pages of publications of the St. Petersburg Academy for twenty years after his death. Actually the publication of his literary legacy lasted until 1862. N. Fuss published about 220 works, and then the work was carried on by V. Y. Buniakovsky, P. L. Chebyshev, and P.H. Fuss. Other works were found still later. The list compiled by Eneström (25) includes 856 titles and 31 works by J.A. Euler, all written under the supervision of his father.
Euler’s enormous correspondence (approximately 300 addressees), which he conducted from 1726 until his death, has been only partly published. For an almost complete description, with summaries and indexes, see (37) below. For his correspondence with Johann I Bernoulli, see (2) and (3); with Nikolaus I Bernoulli (2) and (4); with Daniel Bernoulli (2) and (3); with C. Goldbach (2) and (5); with J.N. Delisle (6); with Clairaut (7); with d’Alembert (3) and (8); with T. Mayer (9); with Lagrange (10); with J.H. Lambert (11); with M. V. Lomonosov (12); with G. F. Müller (13); with J. D. Schumacher (13); with King Stanislas II (14); and with various others (15).
Euler’s complete works are in the course of publication in a collection that has been destined from the outset to become one of the monuments of modern scholarship in the historiography of science: Leonhardi Euleri Opera omnia (BerlinGöttingenLeipzigHeidelberg, 1911). The Opera omnia is limited for the most part to republishing works that Euler himself prepared for the press. All texts appear in the original language of publication. Each volume is edited by a modern expert in the science it concerns, and many of the introductions constitute full histories of the relevant branch of science in the seventeenth and eighteenth centuries. Several volumes are in course of preparation. The work is organized in three series. The first series (Opera mathematica) comprises 29 vols. and is complete. The second series (Opera mechanica et astronomica) is to comprise 31 vols. and still lacks vols. XVI, XVII, XIX, XX, XXI, XXIV, XXVI, XXVII, and XXXI. The third series (Opera physica, Miscellanea, Epistolae) is to comprise 12 vols. and still lacks vols. IX and X. Euler’s correspondence is not included in this edition.
2. P.H. Fuss, ed., Correspondance mathématique et physique de quelques célèbres géomètres du XVIII^{e} siécle, 2 vols. (St. Petersburg, 1843). See vol. I for correspondence with Goldbach. For correspondence with Johann I Bernoulli, see II, 193; with Nikolaus I Bernoulli, II, 679713; and with Daniel Bernoulli, II, 407665.
3. G. Eneström, ed., Bibliotheca mathematica, 3rd ser., 4 (1903), 344388; 5 (1904), 248291; and 6 (1905), 1687; for correspondence with Johann I Bernoulli. For Euler’s correspondence with Daniel Bernoulli, see 7 (19061907); 126156. See 11 (1911), 223226, for correspondence with d’Alembert.
4. Opera postuma, I (St. Petersburg, 1862), 519549.
5. A.P. Youschkevitch and E. Winter, eds., Leonhard Euler und Christian Goldbach. Briefwechsel 1729–1764 (Berlin, 1965).
6. A. T. Grigorian, A. P. Youschkevitch, et. al., eds., Russkofrantsuskie nauchnye svyazi (Leningrad, 1968), pp. 119279.
7. G. Bigourdan, ed., “Lettres inédites d’Euler à Clairaut,” in Comptes rendus du Congrès des sociétés savantes, 1928 (Paris, 1930), pp. 2640.
8.Bullettino di bibliografia e di storia delle scienze matematiche e fisiche, 19 (1886), 136148.
9. Y. K. Kopelevich and E. Forbs, eds., Istorikoastronomicheskie issledovania, V (1959), 271444; X (1969), 285308.
10. J. L. Lagrange, Oeuvres, J. A. Serret and G. Darboux, eds., XIV (Paris, 1892), 135245.
11. K. Bopp, “Eulers und J.H. Lamberts Briefwechsel,” in Abhandlungen der Preussischen Akademie der Wissenschaften (1924), 737.
12. M. V. Lomonosov, Sochinenia, VIII (MoscowLeningrad, 1948); and Polnoe sobranie sochineny, X (MoscowLeningrad, 1957).
13. A. P. Youschkevitch, E. Winter, et. al., eds., Die Berliner und die Petersburger Akademie der Wissenschaften im Briefwechsel Leonhard Eulers, 2 vols. See vol. I (Berlin, 1959) for letters to G.F. Müller; vol. II (Berlin, 1961) for letters to Nartov, Schumacher, Teplov, and others.
14. T. K∤ado and R. W. Wo∤oszyński, eds., “Korrespondencja Stanis∤awa Augusta z Leonardem Eulerem...” in Studia i materia∤y z dziejów nauki polskiej, ser. C, no. 10 (Warsaw, 1965), pp. 341.
15. V.I. Smirnov et. al., eds., Leonard Euler. Pisma k uchenym (MoscowLeningrad, 1963). Contains letters to Bailly, Bülfinger, Bonnet, C. L. Ehler, C. Wolff, and others.
II. Secondary Literature.
16. J. W. Herzog, Adumbratio eruditorum basilensium meritis apud exteros olim hodieque celebrium (Basel, 1778), pp. 3260.
17. N. Fuss, Éloge de Monsieur Léonard Euler (St. Petersburg, 1783). A German trans. of this is in (1), 1st ser., I, xliiixcv.
18. Marquis de Condorcet, Éloge de M. Euler, in Histoire de l’Académie royale des sciences pour l’année 1783 (Paris, 1786), pp. 3768.
19. R. Wolf, Biographien zur Kulturgeschichte der Schweiz, IV (Zurich, 1862), 87134.
20. P. Pekarski, “Ekaterina II i Eyler,” in Zapiski imperatorskoi akademii nauk, 6 (1865), 5992.
21. P. Pekarski, Istoria imperatorskoi akademii nauk v Peterburge, 1 (1870), 247–308, See also index.
22. M. I. Sukhomlinov, ed., Materialy dlya istorii imperatorskoi akademii nauk, 17161760 10 vols. (St. Petersburg, 18851900). See indexes.
23. Protokoly zasedany konferentsii imperatorskoi akademii nauk s 1725 po 1803 god, 4 vols. (St. Petersburg, 18971911). See indexes.
24. A. Harnack, Geschichte der königlichen preussischen Akademie der Wissenschaften, IIII (Berlin, 1900).
25. G. Eneström, “verzeichnis der Schriften Leonhard Eulers,” in Jahresbericht der Deutschen Mathematikervereinigung, Ergänzungsband 4 (Leipzig, 19101913). An important BIBLIOGRAPHY of Euler’s works in three parts, listed in order of date of publication, in order of date of composition, and by subject. The first part is reprinted in (35), I, 352386.
26. O. Spiess, Leonhard Euler. Ein Beitrag zur Geistesgeschichte des XVIII. Jahrhunderts (FrauenfeldLeipzig, 1929).
27. G. Du Pasquier, Léonard Euler et ses amis (Paris, 127)
28. W. Stieda, Die Übersiedlung Léonhard Eulers von Berlin nach Petersburg (Leipzing, 1931).
29. W. Stieda, J.A. Euler in seinen Briefen, 17661790 (Leipzig, 1932).
30. A. Speiser, Die Basler Mathematiker (Basel, 1939).
31. E. Fueter, Geschichte der exakten Wissenschaften in der Schweizerischen Aufklärung, 16801780 (Aarau, 1941).
32. Karl Euler, Das Geschlecht EulerSchölpi. Geschichte einer alien Familie (Giessen, 1955).
33. E. and M. Winter, eds., Die Registres der Berliner Akademie der Wissenschaften, 17461766. Dokumente für das Wirken Leonhard Eulers in Berlin (Berlin, 1957). With an intro. by E. Winter.
34. Istoria akademii nauk SSSR, I (MoscowLeningrad, 1958). See index.
35. Y.K. Kopelevich, M. V. Krutikova, G. M. Mikhailov, and N. M. Raskin, eds., Rukopisnye materialy Leonarda Eylera v arkhive akademii nauk SSR, 2 vols. (Moscow–Leningrad, 1962–1965). Vol. I contains an index of Euler’s scientific papers, an index of official and personal documents, summaries of proceedings of conferences of the Academy of Sciences of St. Petersburg with respect to Euler’s activities, an index of Euler’s correspondence, a reedited version of the first part of (24), and many valuable indexes. Vol. II contains 12 of Euler’s papers on mechanics published for the first time. See especially I, 120228.
36. G. K. Mikhailov, “K pereezdu Leonarda Eylera v Peterburg” “On Leonhard Euler’s Removal to St. Petersburg,” in Izvestiya Akademii nauk SSSR. Otdelenie tekhnicheskikh nauk, no. 3 (1957), 1038.
37. V.I. Smirnov and A. P. Youschkevitch, eds., Leonard Eyler. Perepiska. Annotirovannye ukazateli (Leningrad, 1967).
38. F. Dannemann, Die Naturwissenschaften in ihrer Entwicklung und in ihrem Zusammenhänge IIIII (Leipzig, 1921). See indexes.
39. R. Taton, ed., Histoire générale des sciences, II (Paris, 1958). See index.
40. I. Y. Timchenko, Osnovania teorii analiticheskikh funktsy. Chast I. Istoricheskie svedenia (Odessa, 1899).
41. M. Cantor, Vorlesungen über Geschichte der Mathematik, IIIIV (Leipzig, 18981908). See indexes.
42. H. Wieleitner, Geschichte der Mathematik, II (BerlinLeipzig, 19111921). See indexes.
43. D.J. Struik, A Concise History of Mathematics, 2 vols. (New York, 1948; 2nd ed., London, 1956).
44. J. E. Hofmann, Geschichte der Mathematik, pt. 3 (Berlin, 1957). See index.
45. A. P. Youschkevitch, Istoria matematika v Rossii do 1917 goda (Moscow, 1968). See index.
46. Carl B. Boyer, A History of Mathematics (New York, 1968).
47. L.E. Dickson, History of the Theory of Numbers, 3 vols. (Washington, 1919–1927; 2nd ed., 1934). See indexes.
48. D. J. Struik, “Outline of a History of Differential Geometry,” in Isis, 19 (1933), 92120; 20 (1933), 161191.
49. J. L. Coolidge, A History of Geometrical Methods (Oxford, 1940).
50. G. H. Hardy, Divergent Series (Oxford, 1949).
51. A. I. Markuschevitsch, Skizzen zur Geschichte der analytischen Funktionen (Berlin, 1955)
52. Carl B. Boyer, History of Analytic Geometry (New York, 1956). See index.
53. N. I. Simonov, Prikladnye metody analiza u Eylera (Moscow, 1957).
54. A. T. Grigorian, Ocherki istorii mekhaniki v Rossii (Moscow, 1961).
55. C. Truesdell, “The Rational Mechanics of Flexible or Elastic Bodies”, in (1), 2nd ser., XI, pt. 2.
57. A. P. Mandryka, Istoria ballistiki (MoscowLenigrad, 1964).
58. N.V. Bogolyubov, Istoria mekhaniki mashin (Kiev, 1964).
59. F. Rosenberger, Die Geschichte der Physik in Grundzügen II (Brunswick, 1884). See index.
60. V. F. Gnucheva, Geografichesky departament akademii nauk XVIII veka (MoscowLenigrad, 1946).
61. E. Hoppe, Die Philosophie Leonhard Eulers(Gotha, 1904).
62. A. Speiser, Leonhard Euler und die deutsche Philosophie (Zurich, 1934).
63. G. Kröber, L. Euler. Briefe an eine deutsche Prinzessin. Philosophische Auswahl (Leipzig, 1965), pp. 526. See also intro.
Many important essays on Euler’s life, activity, and work are in the following five memorial volumes.
64. Festschrift zur Feier 200. Geburtstages Leonhard Eulers (LeipzigBerlin, 1907), a publication of the Berliner Mathematische Gesellschaft.
65. A. M. Deborin, ed., Leonard Eyler, 1707–1783 (MoscowLeningrad, 1935).
66. E. Winter, et. al., eds., Die deutschrussische Begegnung und Leonhard Euler.... (Berlin, 1958).
67. M. A. Lavrentiev, A. P. Youschkevitch, and A. T. Grigorian, eds., Leonard Eyler. Sbornik statey (Moscow, 1958). See especially pp. 268375 and 377413 for articles on Euler’s work in astronomy and his physical concepts.
68. K. Schröder, ed., Sammelband der zu Ehren des 250. Geburtstages Leonhard Eulers... vorgelegten Abhandlungen (Berlin, 1959).
69. Istorikomatematicheskie issledovania (Moscow, 19491969). For articles on Euler, see II, VVII, X, XII, XIII, XVI, and XVII.
70. G. K. Mikhailov, “Leonard Eyler”, in Izvestiya akademii nauk SSSR. Otdelenie teknicheskikh nauk, no. 1 (1955), 326, with extensive BIBLIOGRAPHY.
A. P. Youschkevitch
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Euler, Leonhard
EULER, LEONHARD
(b. Basel, Switzerland, 15 April 1707;
d. St. Petersburg, Russia, 18 September 1783), mathematics, mechanics, astronomy, physics. For the original article on Euler see DSB, vol. 4.
Euler’s mathematics had its own characteristics and was based upon principles that distinguished it both from Leibnizian and Newtonian mathematics and nineteenthcentury mathematics. In the period from 1975 to 2005 the most interesting historical studies on Euler have tried to highlight these characteristics and to reconstruct the conceptual background to Euler’s mathematics and the reasons underlying his work.
Analysis and Geometry . Euler’s scientific work was crucial in the process of transformation of analysis into an autonomous field of mathematics. He thought that analysis and geometry were characterized by different methods. In geometry a part of the reasoning was unloaded onto figures in the sense that some steps of the deductive process were based on the intuitive inspection of a figure, without a verbal formulation. Instead analysis was understood as a conceptual system where deduction was merely linguistic and mediated: It proceeded from one proposition to another discursively, without inference derived from the immediate evidence of a diagram.
Even though this concept of analysis was the necessary premise for nineteenth and twentiethcentury concepts, Euler’s idea of mathematical theory was radically different from the modern one. In his opinion mathematics was not a free creation of the mind and was not constituted from a set of propositions syntactically derived from explicit axioms. Mathematics was viewed as a mirror of reality; its objects were idealizations derived from the physical world and had an intrinsic existence before and independent from their definition. Theorems were not merely hypothetical but concerned reality, and were true or false according to whether or not they corresponded to the facts. This led to a lack of distinction between syntactical and semantic aspects of mathematical theories (see Ferraro, 2001).
Quantity, Function, and Formal Methodology . The transformation of analysis into an exclusively linguistic deductive system was based on the notions of general quantity and function. A general quantity was what all geometrical quantities had in common, namely, it was an abstract entity characterized by the capacity of being increased or decreased in a continuous way (see Panza, 1996). A general quantity was measured by numbers and could have any numerical value; however, it was a mathematical object different from the set of real numbers.
In Euler’s opinion the proposition “y is a function of x” meant that there was a particular relationship between general quantities x and y and that this relationship could be expressed by an appropriate analytical expression. A function therefore was not a mere analytical expression: It was a pair that consisted of a relationship between general quantities and the analytical expression of this relationship. This twofold aspect of the notion of a function gave rise to a tension that also appears in the apparently different definitions found in Introductio in analysin infinitorum (1748) and in Institutiones calculi differentialis(1755)(see Ferraro, 2000a, pp. 113–114).
The importance of the analytical expression in the concept of a function was due to the fact that only the relationships that were analytically expressed by means of certain determined analytical expressions were accepted as functions. More precisely, an explicit function was given by one analytical expression constructed from variables in a finite number of steps using exponential, logarithmic, and trigonometric functions, algebraic operations, and composition of functions (see Fraser, 1989, p. 325). A function could also be given in an implicit form f(x,y) = 0, where f is an analytical expression in the above sense.
Euler realized that elementary functions were not sufficient to the development of analysis. He also investigated certain relations between quantities that could not be expressed using elementary functions and sometimes termed them “functions.” However, the knowledge of these transcendental nonelementary functions was considered incomplete and unsatisfactory, and Euler did not put these functions and elementary ones on the same plane. In his opinion a function was an entirely known object, to such a degree that it could be accepted as the final solution to a problem. During the eighteenth century only elementary functions were thought to be known objects to the point that they could be accepted as the final solution to a problem: For this reason, only elementary functions were considered as functions in the proper sense of the term. Nonelementary transcendental functions were objects to be investigated and made known, rather than effectively given functions. Euler believed that they could be accepted as functions (in the proper sense) when their knowledge was improved (on Euler’s concept of a function see Fraser, 1989; Panza, 1996; and Ferraro, 2000a).
Euler’s notion of function was characterized in an essential way by the use of a formal methodology that made it possible to operate upon analytical expressions independently of their meaning. This formal methodology was based upon two closely connected analogical principles:
 (Principle of the generality of algebra.) If formulas or equations were derived by using the rules of analysis and were valid over an interval I_{x} of values of variables, then it was thought to be valid in general.
 (Principle of extension of rules and procedures from the finite to the infinite.) If a rule R was valid for finite expressions or if a procedure P depended on a finite number n of steps S_{1,}, S_{2,}, S_{3,}, ... , S_{n,}, then it was legitimate to apply the rule R and the procedure P to infinite expressions and in an unending number of steps S_{1,}, S_{2,}, S_{3,} ...
Infinite Series . Infinite series were not themselves regarded as functions. They were conceived as the development of functions or other quantities and served to represent them (see Fraser, 1989, p. 322). The procedures for developing a function into a series were based upon principle 2. Following the pioneer of series theory, Euler initially thought that a series represented a quantity only if it converged to it. Principle 2, however, posed the problem of the relationship between formal manipulation and convergence. The eighteenthcentury accepted solution consisted
in assuming that the usual procedures of development transformed a given function f(x) into a series converging to f(x) at least over an intervaln of values of the variable x. The actual determination of the interval of convergence was an a posteriori question, which occurred only when, in dealing with numerical, geometric, and mechanical problems, it was necessary to compute the values of f(x) by means of its series expansion (on Euler’s theory of series see Ferraro, 2000b, and Ferraro and Panza, 2003).
This way of treating series worked well enough as concerns the ordinary power series deriving from elementary functions and did not involve the consideration of the sum of divergent series. However, formal manipulation led Euler to consider asymptotic series and series with the radius of convergence equal to zero. He also came to regard certain power series only from a combinatorial viewpoint. This yielded an aware shift to a more formal concept and led to Euler’s notion of the sum of a series as the function that generated the series. The latter notion solved some complications in series theory and had significant developments during the second part of the eighteenth century (for instance, Laplace’s theory of generating functions) but prevented Euler from achieving a real understanding of trigonometric functions and from using series to investigate special functions appropriately.
Differential and Integration . In Institutiones calculi differentialisEuler stated that the true object of the calculus was not the differentialdyof a function y = y(x)but the differential ratio However,this idea was not sufficiently developed, and Euler’s calculus continued to be based on the use of differentials. These were thought of as fictitious quantities, namely as symbols that represented quantities tending to zero and that were manipulated in the same way as numbers (on Euler ’s notion of number and infinitesimal, see Ferraro, 2003).
The fact that a function was a relationship between general quantities involved some implicit assumptions. General quantities (and consequently functions) were thought to possess properties such as continuity, differentiability, and Taylor expansion (in the modern sense of the terms), which corresponded to the usual properties of a “nice” curve, lack of jumps, presence of the tangent, curvature radius, and so on. This was due to the fact that general quantities were abstractions from geometrical objects. Thus, even if Euler’s analysis dispensed with figures, it retained a remarkably geometric characterization.
Euler’s approach to the calculus was global; namely, he did not considered a certain property of a function f(x), such as differentiability, as a local property valid in a neighborhood of given values x_{o} of the variable. He rather considered them as global properties valid for every value of the variable quantity x (see Fraser, 1989, pp. 328–329). If a certain property failed at a value x_{o} of x, this was not considered significant. The generality of algebra was the basis of this approach.
Euler did not appreciate the difference between complex and real variables and, therefore, between complex and real analysis. Even if he obtained some results, which can be interpreted a posteriori as being related to the functions of complex variables, complex functions were not an autonomous object of study (see Fraser, 1989, pp. 327–328).
Euler defined integration as the inverse operation of differentiation or derivation, namely the integral ∫ f(x)dx of the function f(x) was defined as a function F(x) such that dF = f(x)dx. He was aware that many simple functions could not be integrated by means of elementary functions and that this concept of integration posed the problem of nonelementarily integrable functions. However, the problem of establishing a priori the existence of the integral or of the solution of a differential equation was not tackled. Euler limited himself to comparing integration with inverse arithmetical operations. In his opinion integration led to new transcendental “quantities” in the same manner as the operations of subtraction, division, and extracting a root led to negative, rational, and irrational numbers. Even if Euler devoted many pages to the investigation of new transcendental quantities, such as
his concept of a function prevented him from giving them adequate treatment.
Calculus of Variations and Applied Mathematics . Although Euler was a student of Johann Bernoulli, Euler’s calculus of variations was much influenced by Jacob Bernoulli and Brook Taylor, in particular, “the essential analytical innovations that distinguished Euler’s approach from the Bernoullis were provided by Taylor” (Fraser, 1994, pp. 138–139). Taylor was not the only English mathematician to influence Euler. For instance, Euler’s theory of series was rooted in Isaac Newton’s method of series and in Abraham de Moivre’s work on recurrent series.
Euler did not employ limiting processes or finite approximations in order to minimize and maximize an integral
where F is a function of x, y, and He rather considered the integral
as an infinite sum of the form ...+Z_{/}ddx+Zdx+Z^{/}dx+... , where dx is an infinitesimal and Z_{/}, Z, Z^{/} are the values of Z at ...,xdx, x, x+dx, ... (Fraser, 1999, p. 359). In his Methodus inveniendi lineas curvas maximi minimive proprietate gaudentes (1744) Euler treated the calculus of variations geometrically; however, his reasonings were very general and did not depend on the particular geometrical representation. He also called for the development of a simple method or an algorithm to obtain variational equation. This algorithm was developed by Lagrange, who recognized the dual usage of the symbol dy in Euler’s paper, where it denoted both the differential dy of y with respect to x and the variation of the curve y(x) (on Euler’s calculus of variation see Fraser, 1992, 1994, and 1997).
Euler strongly developed analytical methods in applied mathematics. He thought that while analysis considered general quantities, applied mathematics concerned the specific types of quantities, such as areas, lengths, and force. His concept of mechanics had wide success and paved the way for analytical mechanics (Euler’s mechanics as discussed here refer to Fraser, 1991; Maltese, 2000; Panza, 1995; and Cordoso and Penha, 1999, in particular for the relationship between mathematical technique and physical conception, for the notion of a motion, and for his conception of the principle of least action). Euler also investigated the theory of music. In his Tentamen novae theoriae musicae(1739), he tried to make music part of mathematics and calculated the degrees of order associated with chords and sequences of chords.
BIBLIOGRAPHY
WORKS BY EULER
Leonhardi Euleri Opera omnia. Berlin, Leipzig, Heidelberg, Zurich, and Basel: 1911– .The plan of Euler’s Opera omnia originally involved three series, containing the works that Euler personally prepared for publication. Between 1911 and 2006 seventy volumes of series 1, 2, and 3 were published. Volumes 26 and 27 of series 2 were expected to be published in 2010. The publication of series 4 began in 1985. It is devoted to Euler’s correspondence (series 4A) and manuscripts (series 4B). Series 4A was planned to consist of ten volumes (four volumes were published by 2006). Series 4B was anticpated to contain Euler’s hitherto unpublished manuscripts, notebooks, and diaries.
The Euler Archive. Available from http://math.dartmouth.edu/~euler An online resource for Leonhard Euler’s original works and modern Euler scholarship.
OTHER SOURCES
Bailhache, Patrice. “Deux mathématiciens musiciens: Euler et d’Alembert.” Physis Rivista Internazionale Storia Scienza (N.S.) 32 (1995): 1–35.
Calinger Ronald. “Leonhard Euler: The First St. Petersburg Years (1727–1741).” Historia Mathematica 23 (1996): 121–166.
Cardoso Dias, Maria Penha. “Euler’s ‘Harmony’ between thePrinciples of ‘Rest’ and ‘Least Action’: The Conceptual Making of Analytical Mechanics.” Archive for History of Exact Sciences 54 (1999): 67–86.
Engelsman, Steven B. Families of Curves and the Origins of Partial Differentiation. Amsterdam: NorthHolland, 1984.
Ferraro, Giovanni. “Some Aspects of Euler’s Theory of Series: Inexplicable Functions and the EulerMaclaurin Summation Formula.” Historia Mathematica 25 (1998): 290–317
. ———.“Functions, Functional Relations, and the Laws of Continuity in Euler.” Historia Mathematica 27 (2000a): 107–132.
———. “The Value of an Infinite Sum: Some Observations on the Eulerian Theory of Series.” Sciences et Techniques en Perspective 4 (2000b): 73–113.
———. “Analytical Symbols and Geometrical Figures: EighteenthCentury Analysis as Nonfigural Geometry.” Studies in History and Philosophy of Science 32 (2001): 535–555.
———. “Differentials and Differential Coefficients in the Eulerian Foundations of the Calculus.” Historia Mathematica31 (2004): 34–61.
Ferraro, Giovanni, and Marco Panza. “Developing into Series and Returning from Series: A Note on the Foundations of EighteenthCentury Analysis.” Historia Mathematica 30 (2003): 17–46.
Fraser, Craig G. “The Calculus as Algebraic Analysis: Some Observations on Mathematical Analysis in the 18th Century.” Archive for History of Exact Sciences 39 (1989): 317–335. A crucial essay that clarifies the conceptual foundation of analysis in the eighteenth century.
———. “Mathematical Technique and Physical Conception in Euler’s Investigation of the Elastica.” Centaurus 34, no. 3 (1991): 211–246.
———. “Isoperimetric Problems in the Variational Calculus of Euler and Lagrange. Historia Mathematica 19 (1992): 4–23.
———. “The Origins of Euler’s Variational Calculus.” Archive for History of Exact Sciences 47 (1994): 103–141.
———. “The Concept of Elastic Stress in EighteenthCentury Mechanics: Some Examples from Euler.” In Hamiltonian Dynamical Systems: History, Theory, and Applications, edited by H. Scott Dumas, Kenneth R. Meyer, and Dieter S. Schmidt. Heidelberg: SpringerVerlag, 1995.
———. “The Background to and Early Emergence of Euler’s Analysis.” In Analysis and Synthesis in Mathematics: History and Philosophy, edited by Michael Otte and Marco Panza. Dordrecht, Boston, and London: Kluwer, 1997.
———. “The Calculus of Variations: A Historical Survey.” In A History of Analysis, edited by Hans Niels Jahnke. Providence, RI: American Mathematical Society, 2003.
Golland, Louise Ahrndt, and Ronald William Golland. “Euler’s Troublesome Series: An Early Example of the Use of Trigonometric Series.” Historia Mathematica 20 (1993): 54–67.
Maltese, Giulio. “On the Relativity of Motion in Leonhard Euler’s Science.” Archive for History of Exact Sciences 54 (2000): 319–348.
Panza, Marco. La forma della quantità. Analisi algebrica e analisi superiore: Il problema dell’unità della matematica nel secolo dell’illuminismo. Vols. 38–39 of the Cahiers d’historie et de philosophie des sciences. Nantes, France: 1992. A wide investigation (almost eight hundred pages) of eighteenthcentury mathematics. Several aspects of Euler’s work are dealt with (Italian).
———. “Concept of Function, between Quantity and Form, in the Eighteenth Century.” In History of Mathematics and Education: Ideas and Experiences, edited by Hans Niels Jahnke, Norbert Knoche, and Michael Otte. Göttingen, Germany: Vandenhoeck & Ruprecht, 1996.
———. “De la nature épargnante aux forces généreuses: Le principe de moindre action entre mathématiques et métaphysique Maupertuis et Euler, 1740–1751.” Revue d’Histoire des Sciences4 (1995): 435–520.
Steele, Brett D. “Muskets and Pendulums: Benjamin Robins, Leonhard Euler, and the Ballistics Revolution.” Technology and Culture 35 (1994): 348–382.
Wilson, Curtis. “D’Alembert versus Euler on the Precession of the Equinoxes and the Mechanics of Rigid Bodies.” Archive for History of Exact Sciences 37 (1987): 233–273.
Giovanni Ferraro
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Mayer, Johann Tobias
MAYER, JOHANN TOBIAS
(b. Marbach, near Stuttgart, Germany, 17 February 1723; d. Göttingen, Germany, 20 February 1762).
cartography, astronomy.
Mayer was the son of a cartwright, also named Johann Tobias Mayer, and his second wife, Maria Catherina Finken. In 1723 the father left his trade and went to work as the foreman of a welldigging crew in the nearby town of Esslingen, where his family joined him the Following year. After his father’s death in 1737 Mayer was taken into the tocal orphanage, while his mother found employment in St. Katharine’s Hospital, where she remained until her death in 1737. It was probably through her occupation that Mayer found the opportunity to make architectural drawings of the hospital, as he did when he was barely fourteen years old. There is some evidence to indicate that he was encouraged in his draftmanship by Gottlieb David Kandler, a shoemaker who was subsequently responsible for the education of orphans in Esslingen.
Mayer’s skill in architectural drawings also brought him to the attention of a certain Geiger, a noncommissioned officer in the Swabian district artillery, which was then garrisoned in Esslingen. Under Geiger’s instruction, Mayer, in early 1739, prepared a book of plans and drawings of military fortifications. Later in the same year he drew a map of Esslingen and its surroundings (the oldest still extant), which was reproduced as a copper engraving by Gabriel Bodenehr of Augsburg in 1741.
Mayer’s first book, written on the occasion of his eighteenth birthday, was published at about this same time. It was devoted to the application of analytic methods to the solution of geometrical problems, and m its preface Mayer acknowledged his debt to Christian son Woff’s AnfangsGrünlc aller mathematischen hen Wisscnschatften, through which he had taught himself mathematics, a subject not included in the curriculum of the Esslingen Latin school, which he attended. The influence of Wolff’s compendium is again apparent in the arrangement and content of Mayer’s Mathematischer Atlas of 1745; the sixty plates of the latter work duplicate Wolff’s choice of subjects—arithmetic, geometry, trigonometry, and anal v sis, as applied to mechanics, optics, astronomy, geography, chronotogy, gnomonics, pyrotechnics, and military and civil architecture. This atlas, published in Augsburg by the firm of Johann Andreas Pfeffel for which Mayer worked during his brief stay there (from 1744 to 1746), provides a good index to the extent of his scientific and technical knowledge at that period. It was probably in Augsburg that he acquired much of his knowledge of French, Italian, and English. He also became acquainted with a tocal mechanic and optician, G. F. Brander.
Mayer left Augsburg to take up a post with the Homann Cartographic Bureau in Nuremberg. He spent live years there, which he devoted primarily to improving the state of cartography. To this end he collated geographical and astronomical data from the numerous printed and manuscript records to which the Homann office permitted him access. He also made personal observations of lunar occul unions and other astronomical eclipse phenomena, using a ninefootfocus telescope and a glass micrometer of his own design. Of more than thirty maps that he drew, the “mappa critica” of Germany is generally considered to be the most significant, since it established a new standard for the rigorous handling of geographical source materials and for the application of accurate astronomical methods in finding terrestrial latitude and longitude.
In order to facilitate the lunar eclipse method of longitude determination, Mayer in 1747 and 1748 made a large number of micrometric measurements of the angular diameter of the moon and of the times of its meridian transits, In his determinations of the selenographic coordinates of eightynine prominent lunar markings, he took account of the irregularity of the orbital and libratory motions of the moon and of the effect of its variable parallax. In addition his analysis correctly—although fortuitously—reduced twentyseven conditional equations to three “normal” ones, a procedure that had never before been attempted, and one for which a theory had still be developed.
Mayer was the editor of the Kosmographische Nachrichten und Sammlungen auf das Jahr 1748, which was published in Nuremberg in 1750, under the auspices of the newly established Cosmographical Society. The work contains Mayer’s own description of his glass micrometer, his observations of the solar eclipse of 25 July 1748 and the occultations of a number of bright stars, his long treatise on the libration of the moon, and his argument as to why the moon cannot possess an atmosphere. The Cosmographical Society itself, founded by Johann Michael Franz, director of the Homann firm, was crucial in determining the nature, scope, and, to some degree, motivation of Mayer’s subsequent scientific research. The aims of the mathematical class of the society, to which Mayer betonged, as set out by Franz in the preface to the HomannischHaseschen Gesellschafts Atlas (Nuremberg, 1747), define much of Mayer’s later work.
In November 1750 Mayer was called to a professorship at the GeorgAugust Academy in Göttingen, a post that he took up after Faster of the Following year. Shortly before he left Nuremberg he married Maria Victoria Gnüge; of their eight children, two. Johann Tobias and Georg Moritz lived to maturity. Mayer’s academic title, professor of economy, was purely nominal, since his actual duties were assigned, in his letter of appointment, as the teaching of practical (that is, applied) mathematics and research. His reputation as a cartographer and practical astronomer had preceded him, and was indeed the basis for his selection as professor.
Mayer’s chief scientific concerns at this time were the investigation of astronomical refraction and lunar theory. In 1752 he drew up new lunar and solar tables, in which he attained an accuracy of ±,’an achievement attributable to his skillful use of observational data, rather than to the originality of his theory or the superiority of his instruments, Mayer subsequently undertook an investigation of the celestial positions of the moon at conjunction and opposition; he compared the values that he obtained with those derivable from a systematic study of all lunar and solar eclipses reported since the invention of the astronomical telescope and the pendulum clock. His results led him to recognize that the discrepancies of up to ±5’ that he and his contemporaries had found were due largely to errors in the determination of star places and to the poor quality of their instruments.
Mayer’s further astronomical researches consequently included the problem of the elimination of errors from a sixfootradius mural quadrant made in 1755 by John Bird for installation in Mayer’s newly completed observatory in Göttingen; the invention of a simple and accurate method for computing solar eclipses; the compilation of a catalogue of zodiacal stars; and the investigation of stellar proper motions. He wrote treatises on each of these topics that were published posthumously in Georg Christoph Lichtenberg’s Opera inedita Tobiae Mayeri (Göttingen, 1775). This work also contains a treatise on the problem of accurately defining thermometric changes (an extension of Mayer’s research on astronomical refraction) and another on a mathematical theory of color mixing (a topic that Mayer may have taken up in response to the need of the Homann firm, part of which had been transferred to Göttingen in 1755, to train unskilled workers in the accurate reproduction of maps). Appended to Lichtenberg’s book, in accordance with one of Mayer’s last wishes, is a copper engraving of Mayer’s map of the moon; the original map and the forty detailed drawings from which it was constructed were also reproduced by photolithography more than a century later.
Others of Mayer’s treatises, lecture notes, and correspondence have been neglected since their deposit, shortly after his death, in the Göttingen observatory archives, although abstracts of some of his lectures to the Göttingen Scientific Society were printed in the Göttingische Anzeigen von gelehrten Sachen between 1752 and 1762. His researches during these years included his efforts to improve the art of land measurement, for which purpose he invented a new goniometer and explored the application of the repeating principle of angle measurement, developed a new projective method for finding the areas of irregularly shaped fields, and transformed the common astrolabe into a precision instrument. He further applied the repeating principle to an instrument of his own invention, the repeating circle, which proved to be of use not only for the sea navigation for which it had been designed but also for making standard trigonometrical land surveys. (The instrument used by Delambre and Méchain in their determination of the standard meter was a variant, designed by Borda, of the Mayer circle.)
Mayer also undertook to devise a method for finding geographical coordinates independently of astronomical observations. In so doing he arrived at a new theory of the magnet, based, like his lunar theory, on the principles of Newtonian mechanics. This theory represented a convincing demonstration of the validity of the inversesquare law of magnetic attraction and repulsion, and antedated Coulomb’s wellknown verification of that law by some twenty five years. Mayer’s manuscripts on this theory and on its application to the calculation of the variation and dip of a magnetic needle are among those that went virtually unnoticed after his death.
In 1763 Mayer’s widow, acting upon another of his last requests, submitted to the British admiralty his Theoria lunae juxta systema Newtonianum, which contained the derivations of the equations upon which his lunar theory was based, and his Tabulae motuum solis et lunae novae et correctae, which were published in London in 1767 and 1770, respectively. The tables were edited by Maskelyne, and printed under his direct supervision; they were used to compute the lunar and solar ephemerides for the early editions of the Nautical Almanac. (They were superseded a decade later by tables employing essentially the same principles, but based upon the newer and more accurate observational data that were gradually being assembled at the Royal Observatory at Greenwich.) In 1765 the British parliament authorized Maria Mayer to receive an award of £3,000, in recognition of her husband’s claim, lodged ten years before, for one of the prizes offered to “any Person or Persons as shall Discover the Longitude at Sea.”
BIBLIOGRAPHY
A comprehensive list of Mayer’s publications is given in Poggendoriff, II, 91, the sole omission being his article “Versuch einer Erklärung des Erdbebens,” in Hannoverischen nüzlichen Sammlungen (1756), 290–296.
Mayer’s scientific work is discussed by his official biographer, Siegmund Günther, in Allgemeine deutsche Biographie, XXI (1885), 109–116. His correspondence with Euler between 1751 and 1755, a valuable primary source of information about the former’s contributions to the lunar theory, is in E. G. Forbes, ed., The EulerMayer Correspondence (1751–1755) (London, 1971).
The bulk of MS material relating to Mayer is preserved in Göttingen. The official classification of these papers is contained in the Verzeichniss der Handschriften im Preussischen Staate I Hannover 3 Göttingen, III (Berlin, 1894), 154–158. The title “Tobias Mayer’s Nachlass, aufbewahrt in der K. Sternwarte” no longer applies, since the 70 items catalogued in this index were transferred to the Niedersächsische Staats und UniversitätsBibliothek, Gä’ttingen, during the summer of 1965. In this same repository there is a booklet entitled “Briefe von und an J. Tobias Mayer,” Cod. MS philos. 159. Cod. MS philos. 157 and Cod. MS Michaelis 320 are two other items worth consulting. Personalakte Tobias Mayer 4│Vb 18, and 4│Vf│1–4 are preserved in the Dekanate und UniversitäteArchiv, Göttingen. Some additional items of minor importance are also in the archives of the Göttingen Akademie der Wissenschaften.
The only significant MS collection outside Göttingen is “Betreffend der von Seiten des Prof. Tobias Mayer in Göttingen gelöste englische Preisfrage üher die Bestimmung der Longitudo maris. 1754–1765,” Hannover Des. 92 xxxiv no. II, 4, á, Staatsarchiv, Hannover, A few document relating to the payment of the parliamentary award to Mayer’s widow are in vol. I of the Board of Longitude papers at the Royal Greenwich Observatory (P.R.O. Ref. 529, pp. 143–155).
E. G. Forbes, ed., The Unpublished Writings of Tobias Mayer, 3 vols. (Göttingen, 1972), contains Mayer’s writings on astronomy and geography, his lecture notes on artillery and mechanics, and his theory of the magnet and its application to terrestrial magnetism.
Mayer’s role in the development of navigation and his dealings with the British Admiralty and Board of Longitude are discussed in E. G. Forbes, The Birth of Scientific Navigation (London, 1973).
Eric G. Forbes
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Euler, Leonhard (1707–1783)
EULER, LEONHARD (1707–1783)
EULER, LEONHARD (1707–1783), the most prominent and productive mathematician of the Enlightenment, who laid the foundations for numerous new fields. Born in Basel to a Protestant minister and the daughter of another, Euler was destined for the clergy. His propensity for mathematics appeared early, however, and when he entered the University of Basel at the age of thirteen, he studied under the noted mathematician Johann I Bernoulli (1667–1748). He received his master's degree in philosophy in 1723 and joined the department of theology.
From the beginning, however, Euler worked hard to secure a position as a professional mathematician. His close association with the Bernoulli clan of mathematicians, which was to last throughout his life, proved invaluable in this. In 1727 he followed Johann I's two sons, Nikolaus II and Daniel, to the newly established St. Petersburg Academy of Sciences. Although initially invited to serve as professor of physiology, Euler ultimately succeeded Daniel Bernoulli as the academy's professor of mathematics in 1733. In the same year he married Katrina Gsell, daughter of a Swiss painter residing in St. Petersburg. During his years in St. Petersburg, Euler set the pattern for his subsequent career with a prodigious output of articles, treatises, and books on all aspects of mathematics. He was also active in various practical duties of the academy, including the mapping of Russian territories and studies of shipbuilding and navigation.
In 1741 Euler accepted the invitation of Frederick II of Prussia to join the newly reorganized Berlin Academy of Sciences. His twentyfive years in Berlin were marked by his close association with the academy's president, PierreLouis Moreau de Maupertuis (1698–1759), as well by his active participation in several controversies that rocked the "Republic of Letters." Most celebrated among these were a dispute on Leibnizian monads, which Euler vehemently opposed; a controversy about Maupertuis's "Principle of Least Action," in which Euler supported his colleague against Johann Samuel König and Voltaire; and a prolonged debate with d'Alembert and Daniel Bernoulli on the equations describing vibrating strings, which drew in all the leading mathematicians in Europe.
After Maupertuis's death in 1759 Euler became the de facto leader and administrator of the Berlin Academy, but without the official title of president. His strained relations with Frederick II led him to accept an invitation from Catherine the Great to rejoin the St. Petersburg Academy. He returned to St. Petersburg in 1766 and remained there until his death in 1783.
Euler's mathematical output was prodigious, and his collected works include no less than 856 separate works, both published and unpublished. His contributions span all mathematical fields known in his time, as well as several that he founded himself. Euler wrote three textbooks on the differential and integral calculus, which included extensive discussions of differential equations and means to their solution: Introductio in Analysin Infinitorum (1748), Institutiones Calculi Differentialis (1755), and Institutiones Calculi Integralis (1768–1770). In these works Euler insists that the calculus is essentially a relationship between algebraic functions and is not based on geometry. He has no place for the traditional interpretation of differentials and integrals as determining the tangent of a curve or the area beneath it, and his calculus textbooks include none of those familiar graphics. The notion of "function" was a novel one at this time, and he defined it as any algebraic expression including variables and constants.
In the Introductio Euler presents the differential calculus as a special case of the calculus of finite differences when the difference reaches zero. At that point, the ratio between the difference in the value of the function f(x) and the difference in the value of the variable x is 0/0. Whereas most mathematicians considered this expression to be more or less meaningless, according to Euler, it is the basis of the calculus and can take on any value whatsoever. The calculus, he argued, was a procedure to determine the specific value taken on by this ratio in each particular case.
Euler, along with JosephLouis Lagrange, founded the calculus of variations, which deals with the extremum characteristics of functions as a whole, rather than the point characteristics dealt with by the differential calculus. His work in this field played a crucial role in supporting Maupertuis during the controversy over his principle of least action. Using the calculus of variations, Euler demonstrated that the fundamental laws of motion were those that demonstrated the least amount of "action," as defined by Maupertuis. Maupertuis viewed this result as a clear manifestation of God's infinite wisdom in designing the world. Although Euler himself did not present his work explicitly in such metaphysical terms, he remained Maupertuis's most important and loyal supporter throughout the controversy.
Euler was a principal founder of complex analysis, and the field's fundamental relationship, eiθ = cosθ + isinθ, is known today as "Euler's formula." He contributed extensively to mathematical notation, introducing "f(x)" for a function, "e" for the base of natural logarithms, "i" for the square root of–1, and "Σ" for a sum. He worked extensively on number theory and many aspects of mathematical physics, including hydrodynamics and astronomy. Euler was a true polymath, and his deep mark on mathematics is evidenced today by the very numerous "Euler theorems" interspersed in a remarkably wide range of mathematical fields.
See also Alembert, Jean Le Rond d' ; Catherine II (Russia) ; Frederick II (Prussia) ; Lagrange, JosephLouis ; Mathematics ; Republic of Letters ; Voltaire .
BIBLIOGRAPHY
Primary Sources
Euler, Leonhard. Foundations of Differential Calculus. Translated by John D. Blanton. New York, 2000. Translation of first nine chapters of Institutiones Calculi Differentialis (1755).
——. Introduction to Analysis of the Infinite. 2 vols. Translated by John D. Blanton. New York, 1988, 1990. Translation of Introductio in Analysin Infinitorum (1748).
Secondary Sources
Boyer, Carl B. "The Age of Euler." In History of Mathematics, revised by Uta C. Merzbach, Ch. 21, pp. 439–465. New York, 1991.
Youschkevitch, Adolph P. "Euler, Leonhard." In The Dictionary of Scientific Biography, edited by Charles C. Gillispie, 16 vols. New York, 1970–1980.
Amir Alexander
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Euler, Leonhard
Euler, Leonhard
Swiss Geometer and Number Theorist 1707–1783
Leonhard Euler is a name well known in many academic fields: philosophy, hydrodynamics , astronomy, optics, and physics. His true fame comes, however, through his prolific work in pure mathematics. He produced more scholarly work in mathematics than have most other mathematicians. His abilities were so great that his contemporaries called him "Analysis Incarnate."
Euler (pronounced "oiler") was born in Switzerland in 1707. He had originally intended to follow the career path of his father, who was a Calvinist clergyman. Euler studied theology and Hebrew at the University of Basel.
Johann Bernoulli, however, tutored Euler in mathematics on the side. Euler's facility in the subject was so great that his father, an amateur mathematician himself, soon favored the decision of his son to pursue mathematics rather than join the clergy.
Euler first taught at the Academy of Sciences in St. Petersburg, Russia, in 1727. He married and eventually became the father of thirteen children. His children provided him with great joy, and children were often playing in the room or sitting on his lap while Euler worked. It was in Russia that he lost sight in one eye after working for three days to solve a mathematics problem that Academy members urgently needed but had predicted would take months to solve.
Euler was a very productive writer, completing five hundred books and papers in his lifetime and having four hundred more published posthumously. The Swiss edition of his complete works is contained in seventyfour volumes. He wrote Introductio in Analysin Infinitorum in 1748. This book introduces much of the material that is found in modern algebra and trigonometry textbooks.
Euler wrote the first treatment of differential calculus in 1755 in Institutiones Calculi Differentialis and in 1770 explored determinate and indeterminate algebra in Anleitung zur Algebra. Threedimensional surfaces and conic sections were also extensively treated in his writings.
Euler introduced many of the important mathematical symbols that are now in standard usage, such as Σ (for summation), π (the ratio of the circumference of a circle to its diameter), f (x ) (function notation), e (the base of a natural logarithm), and i (square root of negative one). He was the first to develop the calculus of variations. One of the more notable equations that he developed was cosθ + i sinθ = e^{iθ}, which shows that exponential and trigonometric functions are related. Another important equation he developed establishes a relationship among five of the most significant numbers, e^{πi} + 1 = 0.
All of Euler's work was not strictly academic, however. He enjoyed solving practical problems such as the famous "seven bridges of Königsberg" problem that led to Euler circuits and paths. He even performed calculations simply for their own sake.
Euler later went to Berlin to become the director of Mathematics at the Academy of Science under Frederick the Great and to enjoy a more free political climate. However, Euler was viewed as being rather unsophisticated, and Frederick referred to him as a "mathematical Cyclops." He returned to Russia when a more liberal leader, Catherine the Great, came to rule.
By 1766, Euler was completely blind but continued to dictate his work to his secretary and his children. His last words, uttered as he suffered a fatal stroke in 1783, imitated his work in eloquence and simplicity: "I die."
see also Bernoulli Family; Nets.
Laura Snyder
Bibliography
Ball, W. W. Rouse. A Short Account of the History of Mathematics, 4th ed. New York: Dover Publications, 1960.
Bell, E. T. Men of Mathematics. New York: Simon and Schuster, 1986.
Benson, Donald C. The Moment of Proof: Mathematical Epiphanies. New York: Oxford University Press, 1999.
Hollington, Stuart. Makers of Mathematics. London: Penguin Books, 1994.
Motz, Lloyd, and Jefferson Hane Weaver. The Story of Mathematics. New York: Avon Books, Inc., 1993.
Parkinson, Claire L. Breakthroughs: A Chronology of Great Achievements in Science and Mathematics. Boston: G. K. Hall & Co., 1985.
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Mayer, Johann Tobias
Johann Tobias Mayer (yō´hän tōbē´äs mī´ər), 1723–62, German mathematician and astronomer. In 1751 he became professor of economics and mathematics at the Univ. of Göttingen, and in 1754 director of the observatory there. He is especially noted for his lunar tables (1752), which were important in precisely determining longitude at sea. Mayer is remembered also for his improvements in mapmaking and for the invention of the repeating circle, later used in measuring the arc of the meridian. A collection of his memoirs was published in 1775; a revision of his catalog of 998 zodiacal stars, newly computed, appeared in 1894.
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