In mathematics, the Euclidean distance between two points in Euclidean space is a number, the length of a line segment between the two points. It can be calculated from the Cartesian coordinates of the points using the Pythagorean theorem, and is occasionally called the Pythagorean distance. These names come from the ancient Greek mathematicians Euclid and Pythagoras, but Euclid did not represent distances as numbers, and the connection from the Pythagorean theorem to distance calculation was not made until the 17th century.
The distance between two objects that are not points is usually defined to be the smallest distance between any two points from the two objects. Formulas are known for computing distances between different types of objects, such as the distance from a point to a line. In advanced mathematics, the concept of distance has been generalized to abstract metric spaces, and other distances than Euclidean have been studied. The square of the Euclidean distance is not a metric, but is convenient for many applications in statistics and optimization.
The distance between any two points on the real line is the absolute value of the numerical difference of their coordinates. Thus if and are two points on the real line, then the distance between them is given by:
A more complicated formula, giving the same value, but generalizing more readily to higher dimensions, is:
This can be seen by applying the Pythagorean theorem to a right triangle with horizontal and vertical sides, having the line segment from to as its hypotenuse. The two squared formulas inside the square root give the areas of squares on the horizontal and vertical sides, and the outer square root converts the area of the square on the hypotenuse into the length of the hypotenuse.
In general, for points given by Cartesian coordinates in -dimensional Euclidean space, the distance is
Other objects than points
For pairs of objects that are not both points, the distance can most simply be defined as the smallest distance between any two points from the two objects, although more complicated generalizations from points to sets such as Hausdorff distance are also commonly used. Formulas for computing distances between different types of objects include:
- The distance from a point to a line, in the Euclidean plane
- The distance from a point to a plane in three-dimensional Euclidean space
- The distance between two lines in three-dimensional Euclidean space
Squared Euclidean distance
In many applications, and in particular when comparing distances, it may be more convenient to omit the final square root in the calculation of Euclidean distances. The value resulting from this omission is the square of the Euclidean distance, and is called the squared Euclidean distance. As an equation:
Beyond its application to distance comparison, squared Euclidean distance is of central importance in statistics, where it is used in the method of least squares, a standard method of fitting statistical estimates to data by minimizing the average of the squared distances between observed and estimated values. The addition of squared distances to each other, as is done in least squares fitting, corresponds to an operation on (unsquared) distances called Pythagorean addition. In cluster analysis, squared distances can be used to strengthen the effect of longer distances.
Squared Euclidean distance is not a metric, as it does not satisfy the triangle inequality. However it is a smooth, strictly convex function of the two points, unlike the distance, which is non-smooth for equal points and convex but not strictly convex. The squared distance is thus preferred in optimization theory, since it allows convex analysis to be used. Since squaring is a monotonic function of non-negative values, minimizing squared distance is equivalent to minimizing the Euclidean distance, so the optimization problem is equivalent in terms of either, but easier to solve using squared distance.
The collection of all squared distances between pairs of points from a finite set may be stored in a Euclidean distance matrix. In rational trigonometry, squared Euclidean distance is used because (unlike the Euclidean distance itself) the squared distance between points with rational number coordinates is always rational; in this context it is also called "quadrance".
In more advanced areas of mathematics, Euclidean space and its distance provides a standard example of a metric space, called the Euclidean metric. Euclidean distance geometry studies properties of Euclidean geometry in terms of its distances, and properties of sets of distances that can be used to determine whether they come from the Euclidean metric. When viewing Euclidean space as a vector space, its distance is associated with a norm called the Euclidean norm, defined as the distance of each vector from the origin. One of the important properties of this norm, relative to other norms, is that it remains unchanged under arbitrary rotations of space around the origin. By Dvoretzky's theorem, every finite-dimensional normed vector space has a high-dimensional subspace on which the norm is approximately Euclidean; the Euclidean norm is the only norm with this property. It can be extended to infinite-dimensional vector spaces as the L2 norm or L2 distance.
Other common distances on Euclidean spaces and low-dimensional vector spaces include:
- Chebyshev distance, which measures distance assuming only the most significant dimension is relevant.
- Manhattan distance, which measures distance following only axis-aligned directions.
- Minkowski distance, a generalization that unifies Euclidean distance, Manhattan distance, and Chebyshev distance.
For points on surfaces in three dimensions, the Euclidean distance should be distinguished from the geodesic distance, the length of a shortest curve that belongs to the surface. In particular, for measuring great-circle distances on the earth or other near-spherical surfaces, distances that have been used include the Haversine distance giving great-circle distances between two points on a sphere from their longitudes and latitudes, and Vincenty's formulae also known as "Vincent distance" for distance on a spheroid.
Euclidean distance is the distance in Euclidean space; both concepts are named after ancient Greek mathematician Euclid, whose Elements became a standard textbook in geometry for many centuries. Concepts of length and distance are widespread across cultures, can be dated to the earliest surviving "protoliterate" bureaucratic documents from Sumer in the fourth millenium BC (far before Euclid), and have been hypothesized to develop in children earlier than the related concepts of speed and time. But the notion of a distance, as a number defined from two points, does not actually appear in Euclid's Elements. Instead, Euclid approaches this concept implicitly, through the congruence of line segments, through the comparison of lengths of line segments, and through the concept of proportionality.
The Pythagorean theorem is also ancient, but it only took its central role in the measurement of distances with the invention of Cartesian coordinates by René Descartes in 1637. Because of this connection, Euclidean distance is also sometimes called Pythagorean distance. Although accurate measurements of long distances on the earth's surface, which are not Euclidean, had again been studied in many cultures since ancient times (see history of geodesy), the idea that Euclidean distance might not be the only way of measuring distances between points in mathematical spaces came even later, with the 19th-century formulation of non-Euclidean geometry. The definition of the Euclidean norm and Euclidean distance for geometries of more than three dimensions also first appeared in the 19th century, in the work of Augustin-Louis Cauchy.
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