# Karl Friedrich Gauss

# Karl Friedrich Gauss

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 2^{2m} + 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) *x*^{2}/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 + 2*i*)(1 − 2*i*).

## 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. □

# Gauss, Karl Friedrich

# Karl Friedrich Gauss

**Born: April 30, 1777Brunswick, GermanyDied: February 23, 1855Göttingen, Germany**

*German mathematician*

The German mathematician Karl Friedrich Gauss made outstanding contributions to both pure (studied for its own sake) and applied (studied in order to solve specific problems) mathematics.

*Early life and education*

Karl Friedrich Gauss was born in Brunswick, Germany, on April 30, 1777. He was the son of Gebhard Dietrich Gauss, a gardener and bricklayer, and Dorothea Gauss, the daughter of a stonecutter. Karl was an extremely bright child, correcting his father's arithmetic when he was three years old. His intellectual abilities attracted the attention of the Duke of Brunswick, who sent him first to the Collegium Carolinum (1792–95) in Brunswick and then to the University of Göttingen (1795–98).

*Theory of numbers*

In 1801 Gauss published *Disquisitiones arithmeticae,* which is often regarded as the work that marked the beginning of the modern theory of numbers. It combined the work of past scientists with his own, and was presented in such an elegant and complete way that it rendered previous works on the subject obsolete (out of date and no longer needed).

Gauss made many outstanding contributions to the theory of numbers, including research on the division of a circle into equal parts. This solved a famous problem in Greek geometry (the study of points, lines, angles, and surfaces), namely, the inscription (drawing inside) of regular polygons (closed figures bounded by straight lines) in a circle. First, Gauss proved that a regular polygon with seventeen sides can be constructed with a ruler and compass; he then showed that any polygon with a prime number (able to be divided only by itself or the number 1) of sides can be constructed with these instruments.

Gauss also gave three proofs for the idea—conceived by others but never proved—that every equation in algebra has at least one root. Gauss was the first to adopt a strict approach to the treatment of infinite (never-ending) series of numbers. He also opened up a new line of research by updating the definition of a prime number.

*Astronomical calculations*

The discovery by Giuseppe Piazzi of the asteroid Ceres in 1801 increased Gauss's interest in astronomy, and upon the death of the Duke of Brunswick, Gauss was appointed director of the observatory (a building whose purpose is to observe stars and planets) in Göttingen, Germany, where he remained for the rest of his life. Gauss successfully determined the orbit of Ceres and was able to predict its correct 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 how to determine orbits from observed data.

In his calculation of the orbits of planets, Gauss used the method of least squares. This method is used to determine the most likely value of something from a number of available observations. In defense of the method, Gauss created the Gaussian law of error, which became known in studies of probability (chance) and statistics (the collection, study, and presentation of data) as the normal distribution.

*Non-Euclidean geometry*

Although he published nothing on the subject, Gauss was almost certainly the first to develop the idea of non-Euclidean geometry (disputing one of Euclid's [335 –270 b.c.e.] theories that through a given point not on a given line, there exists only one line parallel to the given line). As adviser to the government of Hanover, Gauss had to consider the problem of surveying (measuring and determining exact position of) hilly country. This led him to develop the idea that the measurements of a curved surface could be developed in terms of Gaussian coordinates (points). Instead of considering the surface as part of a three-dimensional (displaying depth) space, Gauss set up a network of coordinates 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 (lacking depth) non-Euclidean geometry.

Apart from his books Gauss published a number of memoirs (reports of his experiences), mainly in the journal of the Royal Society of Göttingen. In general, however, he was unwilling to publish anything that could be regarded as controversial (causing a dispute), and as a result 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 February 23, 1855.

*For More Information*

Buhler, W. K. *Gauss: A Biographical Study.* New York: Springer-Verlag, 1981.

Dunnington, G. Waldo. *Carl Friedrich Gauss, Titan of Science: A Study of His Life and Work.* New York: Exposition Press, 1955.

Schaaf, William L. *Carl Friedrich Gauss: Prince of Mathematicians.* New York: Watts, 1964.

# Gauss, Karl Friedrich

**Gauss, Karl Friedrich** (1777–1855) German mathematician. Gauss made many discoveries that were not credited to him, such as non-Euclidean geometry and quaternions. In 1801, he calculated the orbit of the asteroid Ceres. From 1821, he worked on the first worldwide survey of the Earth's magnetic field. In 1833, Gauss invented the electric telegraph. The unit of magnetic flux density is named after him.

# Gauss, Karl Friedrich

**Gauss, Karl Friedrich** (1777–1855) A German mathematician, Gauss developed the study of spherical geometry, which is essential to the theory of plate tectonics. His major work, Theoria Motus Corporum Coelestium (‘Theory of the Motion of Heavenly Bodies’) (1809), was on planetary movements. He also helped to initiate the international geomagnetic survey of 1834.

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