- Born:
- April 15, 1707, Basel, Switzerland
- Died:
- September 18, 1783, St. Petersburg, Russia (aged 76)
- Subjects Of Study:
- Moon
- calculus
- quadratic reciprocity law
- space motion
- three-body problem
Leonhard Euler
-
Who was Leonhard Euler?
Leonhard Euler (1707–1783) was a highly influential Swiss mathematician and physicist, considered a founder of pure mathematics. He made significant contributions to geometry, calculus, mechanics, and number theory, and applied mathematics to astronomy and technology.
Euler developed the concept of a function in mathematical analysis and advanced the use of infinitesimals. He is known for foundational concepts in geometry, such as the Euler line, and for treating trigonometric functions as numerical ratios. He also introduced many mathematical notations still in use today, including the symbols for summation ((\Sigma)), the base of natural logarithms ((e)), and the imaginary unit ((i)).
Euler's work on infinite series led to his formula relating the exponential function to trigonometric functions, published in his 1748 work Introductio in analysin infinitorum. Despite losing sight in his later years, his productivity remained high, demonstrating an exceptional memory and computational ability.
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Where and when was Euler born?
Leonhard Euler was born on April 15, 1707, in Basel, Switzerland. He was a Swiss mathematician and physicist who made significant contributions to various fields of mathematics and physics. Euler's work laid the foundation for many modern mathematical concepts and notations.
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What fields of math and science did Euler study?
Leonhard Euler, a prominent Swiss mathematician and physicist, made foundational contributions to numerous fields of mathematics and science. His work spanned geometry, calculus, mechanics, and number theory. He also developed methods applicable to observational astronomy and demonstrated practical uses of mathematics in technology and public affairs.
Euler's significant contributions include advancing integral calculus, developing theories for trigonometric and logarithmic functions, and simplifying analytical operations. He is also recognized for his work in analytic geometry, introducing the concept of a function as a central organizing principle in analysis. Furthermore, Euler explored number theory extensively, proving theorems and discovering new concepts. His research also touched upon mechanics, optics, acoustics, and physical astronomy.
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What are some famous mathematical ideas or formulas Euler created?
Leonhard Euler, a prolific Swiss mathematician, made foundational contributions to numerous mathematical fields. He is renowned for his work on the constant e, calculating it to 18 decimal places and expressing it as an infinite series. Euler also developed the famous Euler's identity, (e^{i\pi} + 1 = 0), which elegantly links fundamental mathematical constants. His work on the Königsberg bridge problem laid the groundwork for graph theory and topology. Euler also introduced many modern mathematical notations, including the symbol (\Sigma) for summation and f for functions.
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How did Euler continue to work even after losing his eyesight?
Leonhard Euler continued his prolific mathematical work even after losing his sight. Despite becoming totally blind in his remaining good eye during his later years, his productivity remained undiminished. This was due to his exceptional memory and remarkable ability in mental calculations. He was able to perform complex computations in his head, such as those for his second theory of lunar motion. His work during this period included clear expositions of fundamental principles in mechanics, optics, acoustics, and physical astronomy.
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How has Euler’s work influenced math and science today?
Leonhard Euler's extensive work significantly shaped modern mathematics and science. He made foundational contributions to geometry, calculus, mechanics, and number theory. Euler developed the concept of a mathematical function and advanced the use of infinitesimals and infinite quantities in analysis. He is credited with introducing many notations still in use today, such as (\Sigma) for summation and e for the base of natural logarithms. His work on number theory provided proofs for many of Fermat's assertions and established concepts like congruence. Furthermore, Euler's formula, (e^{ix} = \cos x + i \sin x), connects fundamental mathematical constants and functions. His systematic approach to calculus and his numerous publications laid the groundwork for future mathematical and scientific advancements.
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Leonhard Euler (born April 15, 1707, Basel, Switzerland—died September 18, 1783, St. Petersburg, Russia) was a Swiss mathematician and physicist, one of the founders of pure mathematics. He not only made decisive and formative contributions to the subjects of geometry, calculus, mechanics, and number theory but also developed methods for solving problems in observational astronomy and demonstrated useful applications of mathematics in technology and public affairs.
From St. Petersburg to Berlin
Euler’s mathematical ability earned him the esteem of Johann Bernoulli, one of the first mathematicians in Europe at that time, and of his sons Daniel and Nicolas. In 1727 he moved to St. Petersburg, where he became an associate of the St. Petersburg Academy of Sciences and in 1733 succeeded Daniel Bernoulli to the chair of mathematics. By means of his numerous books and memoirs that he submitted to the academy, Euler carried integral calculus to a higher degree of perfection, developed the theory of trigonometric and logarithmic functions, reduced analytical operations to a greater simplicity, and threw new light on nearly all parts of pure mathematics. Overtaxing himself, Euler in 1735 lost the sight of one eye. Then, invited by Frederick the Great in 1741, he became a member of the Berlin Academy, where for 25 years he produced a steady stream of publications, many of which he contributed to the St. Petersburg Academy, which granted him a pension.
Foundational works and new concepts
In 1748, in his Introductio in analysin infinitorum, he developed the concept of function in mathematical analysis, through which variables are related to each other and in which he advanced the use of infinitesimals and infinite quantities. He did for modern analytic geometry and trigonometry what the Elements of Euclid had done for ancient geometry, and the resulting tendency to render mathematics and physics in arithmetical terms has continued ever since. He is known for familiar results in elementary geometry—for example, the Euler line through the orthocentre (the intersection of the altitudes in a triangle), the circumcentre (the centre of the circumscribed circle of a triangle), and the barycentre (the “centre of gravity,” or centroid) of a triangle. He was responsible for treating trigonometric functions—i.e., the relationship of an angle to two sides of a triangle—as numerical ratios rather than as lengths of geometric lines and for relating them, through the so-called Euler identity (eiθ = cos θ + i sin θ), with complex numbers (e.g., 3 + 2Square root of√−1). He discovered the imaginary logarithms of negative numbers and showed that each complex number has an infinite number of logarithms.
Euler’s textbooks in calculus, Institutiones calculi differentialis in 1755 and Institutiones calculi integralis in 1768–70, have served as prototypes to the present because they contain formulas of differentiation and numerous methods of indefinite integration, many of which he invented himself, for determining the work done by a force and for solving geometric problems, and he made advances in the theory of linear differential equations, which are useful in solving problems in physics. Thus, he enriched mathematics with substantial new concepts and techniques. He introduced many current notations, such as Σ for the sum; the symbol e for the base of natural logarithms; a, b and c for the sides of a triangle and A, B, and C for the opposite angles; the letter f and parentheses for a function; and i for Square root of√−1. He also popularized the use of the symbol π (devised by British mathematician William Jones) for the ratio of circumference to diameter in a circle.
Later years
After Frederick the Great became less cordial toward him, Euler in 1766 accepted the invitation of Catherine II to return to Russia. Soon after his arrival at St. Petersburg, a cataract formed in his remaining good eye, and he spent the last years of his life in total blindness. Despite this tragedy, his productivity continued undiminished, sustained by an uncommon memory and a remarkable facility in mental computations. His interests were broad, and his Lettres à une princesse d’Allemagne in 1768–72 were an admirably clear exposition of the basic principles of mechanics, optics, acoustics, and physical astronomy. Not a classroom teacher, Euler nevertheless had a more pervasive pedagogical influence than any modern mathematician. He had few disciples, but he helped to establish mathematical education in Russia.
Euler devoted considerable attention to developing a more perfect theory of lunar motion, which was particularly troublesome, since it involved the so-called three-body problem—the interactions of Sun, Moon, and Earth. (The problem is still unsolved.) His partial solution, published in 1753, assisted the British Admiralty in calculating lunar tables, of importance then in attempting to determine longitude at sea. One of the feats of his blind years was to perform all the elaborate calculations in his head for his second theory of lunar motion in 1772. Throughout his life Euler was much absorbed by problems dealing with the theory of numbers, which treats of the properties and relationships of integers, or whole numbers (0, ±1, ±2, etc.); in this, his greatest discovery, in 1783, was the law of quadratic reciprocity, which has become an essential part of modern number theory.
Legacy
In his effort to replace synthetic methods by analytic ones, Euler was succeeded by Joseph-Louis Lagrange. But, where Euler had delighted in special concrete cases, Lagrange sought for abstract generality, and, while Euler incautiously manipulated divergent series, Lagrange attempted to establish infinite processes upon a sound basis. Thus it is that Euler and Lagrange together are regarded as the greatest mathematicians of the 18th century, but Euler has never been excelled either in productivity or in the skillful and imaginative use of algorithmic devices (i.e., computational procedures) for solving problems.
Since 1993 the U.S.-based Institute of Combinatorics and its Applications has awarded a medal named for Euler that recognizes lifetime achievement in combinatorics.
