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Carl Friedrich Gauss

 
Statistics Dictionary: Johann Carl Friedrich Gauss

(1777–1855; b. Brunswick, Germany; d. Göttingen, Germany) German mathematician and astronomer. Gauss was responsible, in a paper published in 1809, for developing the statistical theory underlying the method of least squares. He was educated at U Göttingen and U Helmstedt, obtaining his doctorate from the latter in 1799. His work on least squares, which was a consequence of his appointment as director of the observatory at Göttingen in 1807, also entailed his deriving an appropriate error distribution — the distribution now called the normal or Gaussian distribution. He was elected FRS in 1804 and awarded the Society's Copley Medal in 1838. He was elected FRSE in 1820. A lunar crater is named after him.



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Britannica Concise Encyclopedia: Carl Friedrich Gauss
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(born April 30, 1777, Brunswick, Duchy of Brunswick — died Feb. 23, 1855, Göttingen, Hanover) German mathematician, astronomer, and physicist. Born to poor parents, he was a prodigy of astounding depth. By his early teens he had already performed astonishing proofs. He published over 150 works and made such important contributions as the fundamental theorem of algebra (in his doctoral dissertation), the least squares method, Gauss-Jordan elimination (for solving matrix equations), and the bell curve, or Gaussian error curve (see normal distribution). Gauss made important contributions to physics and astronomy and pioneered the application of mathematics to gravitation, electricity, and magnetism. He also developed the fields of potential theory and real analysis. With Archimedes and Newton, he is one of the greatest mathematicians of all time.

For more information on Carl Friedrich Gauss, visit Britannica.com.

Scientist: Gauss, (Johann) Karl Friedrich
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(Johann) Karl Friedrich Gauss
Library of Congress

[b. Braunschweig, Germany, April 30, 1777, d. Göttingen, Germany, February 23 1855]

Gauss is ranked with Archimedes and Newton as the greatest of mathematicians. At age 19 he constructed a regular polygon with 17 sides, the first major new construction since Greek times. In 1799 he provided the first proof that all equations formed by setting a polynomial equal to zero have a solution, the fundamental theorem of algebra. In 1801 he completely restructured number theory. An interest in surveying led to his 1827 theory that mathematically describes properties of surfaces. The asteroid Ceres was discovered in 1801, but astronomers soon lost the location of the dim body. Gauss invented a way to calculate the path of a planet from a few observations. When Ceres was found exactly where he predicted, his fame was ensured.

Gauss was the first to establish a non-Euclidean geometry but he did not publish it. Other mathematicians soon rediscovered it. Gauss similarly discovered much of advanced calculus but failed to publish his results. It is said that his discoveries would have advanced mathematics by 50 years if announced when made. Gauss also studied Earth's magnetic field. He and a collaborator built a working telegraph more than a decade earlier than the 1843 system of Samuel F.B. Morse.


Biography: Karl Friedrich Gauss
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The German mathematician Karl Friedrich Gauss (1777-1855) made outstanding contributions to both pure and applied mathematics.

Karl Friedrich Gauss was born in Brunswick on April 30, 1777. At an early age his intellectual abilities attracted the attention of the Duke of Brunswick, who secured his education first at the Collegium Carolinum (1792-1795) in his native city and then at the University of Göttingen (1795-1798). In 1801 Gauss published Disquisitiones arithmeticae, a work of such originality that it is often regarded as marking the beginning of the modern theory of numbers. The discovery by Giuseppe Piazzi of the asteroid Ceres in 1801 stimulated Gauss's interest in astronomy, and upon the death of his patron, the Duke of Brunswick, Gauss was appointed director of the observatory in Göttingen, where he remained for the rest of his life. In 1831 he collaborated with Wilhelm Weber in the establishment of a geomagnetic survey in Göttingen.

Apart from his books Gauss published a number of memoirs, mainly in the journal of the Royal Society of Göttingen. Generally, however, he was reluctant to publish anything that could be regarded as controversial, so that some of his most brilliant work was found only after his death.

Gauss married twice, but both wives died young. Of his six children, his youngest daughter remained to take care of him until his death on Feb. 23, 1855.

Theory of Numbers

Gauss always strove for perfection of form in his writings. Consequently his finest work, Disquisitiones arithmeticae, in which he integrated the work of his predecessors with his own, by its elegance and completeness rendered previous works on the subject superfluous. Quadratic residues, which led to the law of quadratic reciprocity that Gauss had discovered before he was 18, and indeed power residues in general, are treated extensively. Gauss made three more outstanding contributions to the theory of numbers: the theory of congruences, the theory of quadratic forms, and researches on the division of the circle into equal parts. Gauss also introduced the notation a b (mod c) for congruences; he developed the theory of congruences of the first and second degrees and showed that all problems of indeterminate analysis can be expressed in terms of congruences. Also he investigated the representation of integers by binary and ternary quadratic forms. However, neither the work on quadratic forms nor that on second-degree congruences had any impact until the importance of these contributions was later recognized by K. G. J. Jacobi.

On the other hand, Gauss's results on the division of the circle were received with enthusiasm, for these were immediately recognizable as the solution of a famous problem in Greek geometry, namely, the inscription of regular polygons in a circle. First, Gauss proved that a regular polygon with 17 sides can be constructed with ruler and compasses; he then generalized the result by showing that any polygon with a prime number of sides of the form 22m + 1 can be constructed with these instruments.

Algebra and Analysis

Albert Girard was the first to surmise in 1629, but was unable to prove, that every algebraic equation has at least one root. Gauss gave three proofs for this: the first of these, given in his thesis, assumes that a continuous function which takes positive and negative values is necessarily zero for some value of the variable.

It is clear from Gauss's notebooks that he recognized the double periodicity of the elliptic functions; however, the work was unpublished, and discovery of the property is credited to N. H. Abel, a later mathematician who gave the first published account. Gauss was the first to adopt a rigorous approach to the treatment of infinite series, as illustrated by his treatment of the hypergeometric series. This series, 1 + ab/c x + a(a + 1)b(b + 1)/c(c + 1) x2/2! + …, had been introduced earlier by Leonhard Euler, but it was Gauss who devised a test to establish the conditions for the convergence of this series. He also brought to light the important property that nearly all the functions then known could be expressed as hypergeometric series.

The theory of biquadratic residues was developed by Gauss in two memoirs which he presented to the Royal Society of Göttingen in 1825 and 1831. These investigations, an extension of his earlier work on quadratic residues, involved the use of complex numbers. Gauss recognized that all numbers are of the form a + ib and represented such numbers by points in a plane. Besides deriving the law of biquadratic reciprocity with the help of complex numbers, Gauss opened up a new line of research by modifying the definition of a prime number. According to the new definition, the number 3, for example, remains a prime, while the number 5 becomes composite, since it can be expressed as a product of complex factor (1 + 2i)(1 − 2i).

Astronomical Calculations

After the discovery of Ceres in 1801, the body was lost to observers, but from Piazzi's observations before it disappeared, Gauss successfully determined the orbit of this asteroid and was able to predict accurately its position. Gauss's success in these calculations encouraged him to develop his methods further, and in 1809 his Theoria motus corporum coelestium appeared. In it Gauss discussed the determination of orbits from observational data and also presented an analysis of perturbations.

In his calculation of planetary orbits Gauss used the method of least squares. This method enables all the data to be used when more observations are available than the minimum needed to satisfy the equations. In attempting to justify the method, Gauss derived the Gaussian law of error, familiar to students of probability and statistics as the normal distribution.

Non-Euclidean Geometry

Since the time of the Greeks many attempts had been made to prove Euclid's postulate concerning parallels; the postulate is equivalent to the supposition that the sum of the angles of a triangle is two right angles. In 1733 an attempt to prove the postulate was made by Girolamo Saccheri, who, in fact, invented two non-Euclidean geometries only to reject them for unsound reasons. Gauss envisaged the possibility of developing a geometry without the parallel postulate and on one occasion even measured the angles of a triangle formed by three mountains, finding the sum to be two right angles within the limits of experimental error. Although he published nothing on the subject, Gauss was almost certainly the first to develop the idea of non-Euclidean geometry.

As adviser on geodesy to the Hanoverian government, Gauss had to consider the problem of surveying hilly country. This led him to study differential geometry, and he developed the concepts of curvilinear coordinates and line-element and parametric representations. In 1827 he published a memoir in which the geometry of a curved surface was developed in terms of intrinsic, or Gaussian, coordinates. Instead of considering the surface as embedded in a three-dimensional space, Gauss set up a coordinate network on the surface itself, showing that the geometry of the surface can be described completely in terms of measurements in this network. Defining a straight line as the shortest distance between two points, measured along the surface, the geometry of a curved surface can be regarded as a two-dimensional non-Euclidean geometry. The Gaussian coordinates thus provided an instrument for the analytical development of non-Euclidean geometries.

Further Reading

An extract from Gauss's memoir on magnetic measurements is given in William Francis Magie, A Source Book in Physics (1955). The best book on Gauss is G. Waldo Dunnington, Carl Friedrich Gauss, Titan of Science: A Study of His Life and Work (1955). A good account of Gauss's life and work is William L. Schaaf, Carl Friedrich Gauss: Prince of Mathematicians (1964). A simple introduction to the application of non-Euclidean geometry in relativity theory is in Max Born, Einstein's Theory of Relativity (trans. 1922; rev. ed. 1962).

Additional Sources

Beuhler, W. K. (Walter Kaufmann), Gauss, Berlin; New York: Springer, 1986.

Beuhler, W. K. (Walter Kaufmann), Gauss: a biographical study, Berlin; New York: Springer-Verlag, 1981.

Reich, Karin, Carl Friedrich Gauss: 1777/1977, Meunchen: Moos, 1977.

Reich, Karin, Carl Friedrich Gauss: 1777-1977, Bonn-Bad Godesberg: Inter Nationes, 1977.

Spotlight: Carl Friedrich Gauss
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From our Archives: Today's Highlights, April 30, 2005

Johann Karl Friedrich Gauss, one of the greatest mathematicians of all time, was born on this date in 1777. The first to prove the fundamental theorem of algebra, Gauss also made important contributions to statistics, physics and astronomy, including the Gaussian gravitational constant and the Gauss-Markov theorem.
 
Columbia Encyclopedia: Carl Friedrich Gauss
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Gauss, Carl Friedrich (kärl frē'drĭkh gous), born Johann Friederich Carl Gauss, 1777-1855, German mathematician, physicist, and astronomer. Gauss was educated at the Caroline College, Brunswick, and the Univ. of Göttingen, his education and early research being financed by the Duke of Brunswick. Following the death of the duke in 1806, Gauss became director (1807) of the astronomical observatory at Göttingen, a post he held until his death. Considered the greatest mathematician of his time and as the equal of Archimedes and Newton, Gauss showed his genius early and made many of his important discoveries before he was twenty. His greatest work was done in the area of higher arithmetic and number theory; his Disquisitiones Arithmeticae (completed in 1798 but not published until 1801) is one of the masterpieces of mathematical literature.

Gauss was extremely careful and rigorous in all his work, insisting on a complete proof of any result before he would publish it. As a consequence, he made many discoveries that were not credited to him and had to be remade by others later; for example, he anticipated Bolyai and Lobachevsky in non-Euclidean geometry, Jacobi in the double periodicity of elliptic functions, Cauchy in the theory of functions of a complex variable, and Hamilton in quaternions. However, his published works were enough to establish his reputation as one of the greatest mathematicians of all time. Gauss early discovered the law of quadratic reciprocity and, independently of Legendre, the method of least squares. He showed that a regular polygon of n sides can be constructed using only compass and straight edge only if n is of the form 2p(2q+1)(2r+1) … , where 2q + 1, 2r + 1, … are prime numbers.

In 1801, following the discovery of the asteroid Ceres by Piazzi, Gauss calculated its orbit on the basis of very few accurate observations, and it was rediscovered the following year in the precise location he had predicted for it. He tested his method again successfully on the orbits of other asteroids discovered over the next few years and finally presented in his Theoria motus corporum celestium (1809) a complete treatment of the calculation of the orbits of planets and comets from observational data. From 1821, Gauss was engaged by the governments of Hanover and Denmark in connection with geodetic survey work. This led to his extensive investigations in the theory of space curves and surfaces and his important contributions to differential geometry as well as to such practical results as his invention of the heliotrope, a device used to measure distances by means of reflected sunlight.

Gauss was also interested in electric and magnetic phenomena and after about 1830 was involved in research in collaboration with Wilhelm Weber. In 1833 he invented the electric telegraph. He also made studies of terrestrial magnetism and electromagnetic theory. During the last years of his life Gauss was concerned with topics now falling under the general heading of topology, which had not yet been developed at that time, and he correctly predicted that this subject would become of great importance in mathematics.

Bibliography

See biography by T. Hall (tr. 1970).

Wikipedia: Carl Friedrich Gauss
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Carl Friedrich Gauss

Johann Carl Friedrich Gauss (1777–1855), painted by Christian Albrecht Jensen
Born 30 April 1777(1777-04-30)
Braunschweig, Electorate of Brunswick-Lüneburg, Holy Roman Empire
Died 23 February 1855 (aged 77)
Göttingen, Kingdom of Hanover
Residence Kingdom of Hanover
Nationality German
Fields Mathematician and physicist
Institutions University of Göttingen
Alma mater University of Helmstedt
Doctoral advisor Johann Friedrich Pfaff
Other academic advisors Johann Christian Martin Bartels
Doctoral students Friedrich Bessel
Christoph Gudermann
Christian Ludwig Gerling
Richard Dedekind
Johann Encke
Johann Listing
Bernhard Riemann
Christian Peters
Moritz Cantor
Other notable students August Ferdinand Möbius
Julius Weisbach
L. C. Schnürlein
Known for See full list
Influenced Sophie Germain
Notable awards Copley Medal (1838)
Religious stance Lutheran
Signature

Johann Carl Friedrich Gauss (pronounced /ˈɡaʊs/; German: Gauß De-carlfriedrichgauss.ogg listen , Latin: Carolus Fridericus Gauss) (30 April 1777 – 23 February 1855) was a German mathematician and scientist who contributed significantly to many fields, including number theory, statistics, analysis, differential geometry, geodesy, geophysics, electrostatics, astronomy and optics. Sometimes known as the Princeps mathematicorum[1] (Latin, "the Prince of Mathematicians" or "the foremost of mathematicians") and "greatest mathematician since antiquity", Gauss had a remarkable influence in many fields of mathematics and science and is ranked as one of history's most influential mathematicians.[2] He referred to mathematics as "the queen of sciences."[3]

Gauss was a child prodigy. There are many anecdotes pertaining to his precocity while a toddler, and he made his first ground-breaking mathematical discoveries while still a teenager. He completed Disquisitiones Arithmeticae, his magnum opus, in 1798 at the age of 21, though it would not be published until 1801. This work was fundamental in consolidating number theory as a discipline and has shaped the field to the present day.

Contents

Early years (1777–1798)

Statue of Gauss at his birthplace, Braunschweig

Carl Friedrich Gauss was born on April 30, 1777 in Braunschweig, in the Electorate of Brunswick-Lüneburg, now part of Lower Saxony, Germany, as the second son of poor working-class parents.[4] He was christened and confirmed in a Catholic church near the school he had attended as a child.[5] There are several stories of his early genius. According to one, his gifts became very apparent at the age of three when he corrected, mentally and without fault in his calculations, an error his father had made on paper while calculating finances.

Another famous story has it that in primary school his teacher, J.G. Büttner, tried to occupy pupils by making them add a list of integers in arithmetic progression; as the story is most often told, these were the numbers from 1 to 100. The young Gauss reputedly produced the correct answer within seconds, to the astonishment of his teacher and his assistant Martin Bartels. Gauss's presumed method was to realize that pairwise addition of terms from opposite ends of the list yielded identical intermediate sums: 1 + 100 = 101, 2 + 99 = 101, 3 + 98 = 101, and so on, for a total sum of 50 × 101 = 5050. However, the details of the story are at best uncertain (see [6] for discussion of the original Wolfgang Sartorius von Waltershausen source and the changes in other versions); some authors, such as Joseph Rotman in his book A first course in Abstract Algebra, question whether it ever happened.

As his father wanted him to follow in his footsteps and become a pastor, he was not supportive of Gauss's schooling in mathematics and science. Gauss was primarily supported by his mother in this effort and by the Duke of Braunschweig,[2] who awarded Gauss a fellowship to the Collegium Carolinum (now Technische Universität Braunschweig), which he attended from 1792 to 1795, and subsequently he moved to the University of Göttingen from 1795 to 1798. While in university, Gauss independently rediscovered several important theorems;[citation needed] his breakthrough occurred in 1796 when he was able to show that any regular polygon with a number of sides which is a Fermat prime (and, consequently, those polygons with any number of sides which is the product of distinct Fermat primes and a power of 2) can be constructed by compass and straightedge. This was a major discovery in an important field of mathematics; construction problems had occupied mathematicians since the days of the Ancient Greeks, and the discovery ultimately led Gauss to choose mathematics instead of philology as a career. Gauss was so pleased by this result that he requested that a regular heptadecagon be inscribed on his tombstone. The stonemason declined, stating that the difficult construction would essentially look like a circle.[7]

The year 1796 was most productive for both Gauss and number theory. He discovered a construction of the heptadecagon on March 30.[8] He invented modular arithmetic, greatly simplifying manipulations in number theory.[citation needed] He became the first to prove the quadratic reciprocity law on 8 April. This remarkably general law allows mathematicians to determine the solvability of any quadratic equation in modular arithmetic. The prime number theorem, conjectured on 31 May, gives a good understanding of how the prime numbers are distributed among the integers. Gauss also discovered that every positive integer is representable as a sum of at most three triangular numbers on 10 July and then jotted down in his diary the famous words, "Heureka! num = Δ + Δ + Δ." On October 1 he published a result on the number of solutions of polynomials with coefficients in finite fields, which ultimately led to the Weil conjectures 150 years later.

Middle years (1799–1830)

In his 1799 doctorate in absentia, A new proof of the theorem that every integral rational algebraic function of one variable can be resolved into real factors of the first or second degree, Gauss proved the fundamental theorem of algebra which states that every non-constant single-variable polynomial over the complex numbers has at least one root. Mathematicians including Jean le Rond d'Alembert had produced false proofs before him, and Gauss's dissertation contains a critique of d'Alembert's work. Ironically, by today's standard, Gauss's own attempt is not acceptable, owing to implicit use of the Jordan curve theorem. However, he subsequently produced three other proofs, the last one in 1849 being generally rigorous. His attempts clarified the concept of complex numbers considerably along the way.

Gauss also made important contributions to number theory with his 1801 book Disquisitiones Arithmeticae (Latin, Arithmetical Investigations), which contained a clean presentation of modular arithmetic and the first proof of the law of quadratic reciprocity.

Title page of Gauss's Disquisitiones Arithmeticae

In that same year, Italian astronomer Giuseppe Piazzi discovered the dwarf planet Ceres, but could only watch it for a few days. Gauss predicted correctly the position at which it could be found again, and it was rediscovered by Franz Xaver von Zach on 31 December 1801 in Gotha, and one day later by Heinrich Olbers in Bremen. Zach noted that "without the intelligent work and calculations of Doctor Gauss we might not have found Ceres again." Though Gauss had been up to that point supported by the stipend from the Duke, he doubted the security of this arrangement, and also did not believe pure mathematics to be important enough to deserve support. Thus he sought a position in astronomy, and in 1807 was appointed Professor of Astronomy and Director of the astronomical observatory in Göttingen, a post he held for the remainder of his life.

The discovery of Ceres by Piazzi on 1 January 1801 led Gauss to his work on a theory of the motion of planetoids disturbed by large planets, eventually published in 1809 under the name Theoria motus corporum coelestium in sectionibus conicis solem ambientum (theory of motion of the celestial bodies moving in conic sections around the sun). Piazzi had only been able to track Ceres for a couple of months, following it for three degrees across the night sky. Then it disappeared temporarily behind the glare of the Sun. Several months later, when Ceres should have reappeared, Piazzi could not locate it: the mathematical tools of the time were not able to extrapolate a position from such a scant amount of data—three degrees represent less than 1% of the total orbit.

Gauss, who was 23 at the time, heard about the problem and tackled it. After three months of intense work, he predicted a position for Ceres in December 1801—just about a year after its first sighting—and this turned out to be accurate within a half-degree. In the process, he so streamlined the cumbersome mathematics of 18th century orbital prediction that his work—published a few years later as Theory of Celestial Movement—remains a cornerstone of astronomical computation.[citation needed] It introduced the Gaussian gravitational constant, and contained an influential treatment of the method of least squares, a procedure used in all sciences to this day to minimize the impact of measurement error. Gauss was able to prove the method in 1809 under the assumption of normally distributed errors (see Gauss–Markov theorem; see also Gaussian). The method had been described earlier by Adrien-Marie Legendre in 1805, but Gauss claimed that he had been using it since 1795.[citation needed]

Gauss' portrait published in Astronomische Nachrichten 1828

Gauss was a prodigious mental calculator. Reputedly, when asked how he had been able to predict the trajectory of Ceres with such accuracy he replied, "I used logarithms." The questioner then wanted to know how he had been able to look up so many numbers from the tables so quickly. "Look them up?" Gauss responded. "Who needs to look them up? I just calculate them in my head!"[citation needed]

In 1818 Gauss, putting his calculation skills to practical use, carried out a geodesic survey of the state of Hanover, linking up with previous Danish surveys. To aid in the survey, Gauss invented the heliotrope, an instrument that uses a mirror to reflect sunlight over great distances, to measure positions.

Gauss also claimed to have discovered the possibility of non-Euclidean geometries but never published it. This discovery was a major paradigm shift in mathematics, as it freed mathematicians from the mistaken belief that Euclid's axioms were the only way to make geometry consistent and non-contradictory. Research on these geometries led to, among other things, Einstein's theory of general relativity, which describes the universe as non-Euclidean. His friend Farkas Wolfgang Bolyai with whom Gauss had sworn "brotherhood and the banner of truth" as a student had tried in vain for many years to prove the parallel postulate from Euclid's other axioms of geometry. Bolyai's son, János Bolyai, discovered non-Euclidean geometry in 1829; his work was published in 1832. After seeing it, Gauss wrote to Farkas Bolyai: "To praise it would amount to praising myself. For the entire content of the work... coincides almost exactly with my own meditations which have occupied my mind for the past thirty or thirty-five years."

This unproved statement put a strain on his relationship with János Bolyai (who thought that Gauss was "stealing" his idea), but it is now generally taken at face value.[citation needed] Letters by Gauss years before 1829 reveal him obscurely discussing the problem of parallel lines. Waldo Dunnington, a life-long student of Gauss, successfully proves in Gauss, Titan of Science that Gauss was in fact in full possession of non-Euclidian geometry long before it was published by János, but that he refused to publish any of it because of his fear of controversy.

The survey of Hanover fueled Gauss's interest in differential geometry, a field of mathematics dealing with curves and surfaces. Among other things he came up with the notion of Gaussian curvature. This led in 1828 to an important theorem, the Theorema Egregium (remarkable theorem in Latin), establishing an important property of the notion of curvature. Informally, the theorem says that the curvature of a surface can be determined entirely by measuring angles and distances on the surface. That is, curvature does not depend on how the surface might be embedded in 3-dimensional space or 2-dimensional space.

In 1821, he was made a foreign member of the Royal Swedish Academy of Sciences.

Later years and death (1831–1855)

Grave of Gauss at Albanifriedhof in Göttingen, Germany.

In 1831 Gauss developed a fruitful collaboration with the physics professor Wilhelm Weber, leading to new knowledge in magnetism (including finding a representation for the unit of magnetism in terms of mass, length and time) and the discovery of Kirchhoff's circuit laws in electricity. They constructed the first electromagnetic telegraph in 1833, which connected the observatory with the institute for physics in Göttingen. Gauss ordered a magnetic observatory to be built in the garden of the observatory, and with Weber founded the magnetischer Verein (magnetic club in German), which supported measurements of earth's magnetic field in many regions of the world. He developed a method of measuring the horizontal intensity of the magnetic field which has been in use well into the second half of the 20th century and worked out the mathematical theory for separating the inner (core and crust) and outer (magnetospheric) sources of Earth's magnetic field.

Gauss died in Göttingen, Hannover (now part of Lower Saxony, Germany) in 1855 and is interred in the cemetery Albanifriedhof there. Two individuals gave eulogies at his funeral, Gauss's son-in-law Heinrich Ewald and Wolfgang Sartorius von Waltershausen, who was Gauss's close friend and biographer. His brain was preserved and was studied by Rudolf Wagner who found its mass to be 1,492 grams and the cerebral area equal to 219,588 square millimeters[9] (340.362 square inches). Highly developed convolutions were also found, which in the early 20th century was suggested as the explanation of his genius.[10]

Family

Gauss' daughter Therese (1816—1864)

Gauss's personal life was overshadowed by the early death of his first wife, Johanna Osthoff, in 1809, soon followed by the death of one child, Louis. Gauss plunged into a depression from which he never fully recovered. He married again, to Johanna's best friend named Friederica Wilhelmine Waldeck but commonly known as Minna. When his second wife died in 1831 after a long illness,[11] one of his daughters, Therese, took over the household and cared for Gauss until the end of his life. His mother lived in his house from 1817 until her death in 1839.[2]

Gauss had six children. With Johanna (1780–1809), his children were Joseph (1806–1873), Wilhelmina (1808–1846) and Louis (1809–1810). Of all of Gauss's children, Wilhelmina was said to have come closest to his talent, but she died young. With Minna Waldeck he also had three children: Eugene (1811–1896), Wilhelm (1813–1879) and Therese (1816–1864). Eugene emigrated to the United States about 1832 after a falling out with his father.[citation needed] Wilhelm also settled in Missouri, starting as a farmer and later becoming wealthy in the shoe business in St. Louis. Therese kept house for Gauss until his death, after which she married.

Gauss eventually had conflicts with his sons, two of whom migrated to the United States. He did not want any of his sons to enter mathematics or science for "fear of sullying the family name".[citation needed] Gauss wanted Eugene to become a lawyer, but Eugene wanted to study languages. They had an argument over a party Eugene held, which Gauss refused to pay for. The son left in anger and emigrated to the United States, where he was quite successful. It took many years for Eugene's success to counteract his reputation among Gauss's friends and colleagues. See also the letter from Robert Gauss to Felix Klein on 3 September 1912.

Personality

Gauss was an ardent perfectionist and a hard worker. According to Isaac Asimov, Gauss was once interrupted in the middle of a problem and told that his wife was dying. He is purported to have said, "Tell her to wait a moment till I'm done."[12] This anecdote is briefly discussed in G. Waldo Dunnington's Gauss, Titan of Science where it is suggested that it is an apocryphal story.

He was never a prolific writer, refusing to publish works which he did not consider complete and above criticism. This was in keeping with his personal motto pauca sed matura ("few, but ripe"). His personal diaries indicate that he had made several important mathematical discoveries years or decades before his contemporaries published them. Mathematical historian Eric Temple Bell estimated that had Gauss timely published all of his discoveries, Gauss would have advanced mathematics by fifty years.[13]

Though he did take in a few students, Gauss was known to dislike teaching. It is said that he attended only a single scientific conference, which was in Berlin in 1828. However, several of his students became influential mathematicians, among them Richard Dedekind, Bernhard Riemann, and Friedrich Bessel. Before she died, Sophie Germain was recommended by Gauss to receive her honorary degree.

Gauss usually declined to present the intuition behind his often very elegant proofs—he preferred them to appear "out of thin air" and erased all traces of how he discovered them.[citation needed] This is justified, if unsatisfactorily, by Gauss in his "Disquisitiones Arithmeticae", where he states that all analysis (i.e. the paths one travelled to reach the solution of a problem) must be suppressed for sake of brevity.

Gauss supported monarchy and opposed Napoleon, whom he saw as an outgrowth of revolution.

Commemorations

A 10 Deutsche Mark banknote from Germany 1993 (discontinued) showing Gauss
Gauss on an East-German stamp produced in 1977

From 1989 until the end of 2001, his portrait and a normal distribution curve as well as some prominent buildings of Göttingen were featured on the German ten-mark banknote. The other side of the note features the heliotrope and a triangulation approach for Hannover. Germany has issued three stamps honouring Gauss, as well. A righteous stamp (no. 725), was issued in 1955 on the hundredth anniversary of his death; two other stamps, no. 1246 and 1811, were issued in 1977, the 200th anniversary of his birth.

Daniel Kehlmann's 2005 novel Die Vermessung der Welt, translated into English as Measuring the World: a Novel in 2006, explores Gauss's life and work through a lens of historical fiction, contrasting it with the German explorer Alexander von Humboldt.

In 2007, his bust was introduced to the Walhalla temple.[14]

Things named in honour of Gauss include:

Writings

See also

Notes

  1. ^ Zeidler, Eberhard (2004). Oxford User's Guide to Mathematics. Oxford, UK: Oxford University Press. p. 1188. ISBN 0198507631. 
  2. ^ a b c Dunnington, G. Waldo. (May, 1927). "The Sesquicentennial of the Birth of Gauss". Scientific Monthly XXIV: 402–414. Retrieved on 29 June 2005. Comprehensive biographical article.
  3. ^ Smith, S. A., et al. 2001. Algebra 1: California Edition. Prentice Hall, New Jersey. ISBN 0130442631
  4. ^ "Carl Friedrich Gauss". Wichita State University. http://www.math.wichita.edu/history/men/gauss.html. 
  5. ^ Susan Chambless. "Author — Date". Homepages.rootsweb.ancestry.com. http://homepages.rootsweb.ancestry.com/~schmblss/home/Letters/Gauss/1911-07-26b.htm. Retrieved 2009-07-19. 
  6. ^ http://www.americanscientist.org/issues/pub/gausss-day-of-reckoning/2
  7. ^ Pappas, Theoni: Mathematical Snippets, Page 42. Pgw 2008
  8. ^ Carl Friedrich Gauss §§365–366 in Disquisitiones Arithmeticae. Leipzig, Germany, 1801. New Haven, CT: Yale University Press, 1965.
  9. ^ This reference from 1891 ( - {{cite journal - |last=Donaldson - |first=Henry H. - |authorlink= - |coauthors= - |title=Anatomical Observations on the Brain and Several Sense-Organs of the Blind Deaf-Mute, Laura Dewey Bridgman - |journal=The American Journal of Psychology - |volume=4 - |issue=2 - |pages=248–294 - |publisher=E. C. Sanford - |location= - |year=1891 - |url= - |doi=10.2307/1411270 - |id= - |accessdate=}}) says: "Gauss, 1492 grm. 957 grm. 219588. sq. mm. ", i.e the unit is square mm. In the later reference: Dunnington (1927), the unit is erroneously reported as square cm, which gives an unreasonably large area, the 1891 reference is more reliable. -
  10. ^ Dunnington, 1927
  11. ^ "Gauss biography". Groups.dcs.st-and.ac.uk. http://www-groups.dcs.st-and.ac.uk/~history/Biographies/Gauss.html. Retrieved 2008-09-01. 
  12. ^ Asimov, I. (1972). Biographical Encyclopedia of Science and Technology; the Lives and Achievements of 1195 Great Scientists from Ancient Times to the Present, Chronologically Arranged.. New York: Doubleday. 
  13. ^ Bell, E. T. (2009). "Ch. 14: The Prince of Mathematicians: Gauss". Men of Mathematics: The Lives and Achievements of the Great Mathematicians from Zeno to Poincaré. New York: Simon and Schuster. pp. 218–269. ISBN 0-671-46400-0. 
  14. ^ "Bayerisches Staatsministerium für Wissenschaft, Forschung und Kunst: Startseite". Stmwfk.bayern.de. http://www.stmwfk.bayern.de/downloads/aviso/2004_1_aviso_48-49.pdf. Retrieved 2009-07-19. 
  15. ^ Andersson, L. E.; Whitaker, E. A., (1982). NASA Catalogue of Lunar Nomenclature. NASA RP-1097.

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Awards and achievements
Preceded by
Antoine César Becquerel and John Frederic Daniell
Copley Medal
1838
jointly with Michael Faraday
Succeeded by
Robert Brown


 
 

 

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