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Distance is a numerical description of how far apart objects are. In physics or everyday discussion, distance may refer to a physical length, a period of time, or an estimation based on other criteria (e.g. "two counties over"). In mathematics, distance must meet more rigorous criteria.

In most cases there is symmetry and "distance from A to B" is interchangeable with "distance between B and A".

In analytic geometry, the distance between two points of the xy-plane can be found using the distance formula. The distance between (x_{1}, y_{1}) and (x_{2}, y_{2}) is given by

- $d=sqrt\{(Delta\; x)^2+(Delta\; y)^2\}=sqrt\{(x\_2-x\_1)^2+(y\_2-y\_1)^2\}.,$

Similarly, given points (x_{1}, y_{1}, z_{1}) and (x_{2}, y_{2}, z_{2}) in three-space, the distance between them is

- $d=sqrt\{(Delta\; x)^2+(Delta\; y)^2+(Delta\; z)^2\}=sqrt\{(x\_2-x\_1)^2+(y\_2-y\_1)^2+(z\_2-z\_1)^2\}.$

In the study of complicated geometries, we call this (most common) type of distance Euclidean distance, as it is derived from the Pythagorean theorem, which does not hold in Non-Euclidean geometries. This distance formula can also be expanded into the arc-length formula.

In the Euclidean space R^{n}, the distance between two points is usually given by the Euclidean distance (2-norm distance). Other distances, based on other norms, are sometimes used instead.

For a point (x_{1}, x_{2}, ...,x_{n}) and a point (y_{1}, y_{2}, ...,y_{n}), the Minkowski distance of order p (p-norm distance) is defined as:

1-norm distance | = sum_{i=1}^n left> x_i - y_i right| |

2-norm distance | = left(sum_{i=1}^n left> x_i - y_i right|^2 right)^{1/2} |

p-norm distance | = left(sum_{i=1}^n left> x_i - y_i right|^p right)^{1/p} |

infinity norm distance | = lim_{p to infty} left(sum_{i=1}^n left> x_i - y_i right|^p right)^{1/p} |

= max left(>x_1 - y_1|, |x_2 - y_2|, ldots, |x_n - y_n| right). |

p need not be an integer, but it cannot be less than 1, because otherwise the triangle inequality does not hold.

The 2-norm distance is the Euclidean distance, a generalization of the Pythagorean theorem to more than two coordinates. It is what would be obtained if the distance between two points were measured with a ruler: the "intuitive" idea of distance.

The 1-norm distance is more colourfully called the taxicab norm or Manhattan distance, because it is the distance a car would drive in a city laid out in square blocks (if there are no one-way streets).

The infinity norm distance is also called Chebyshev distance. In 2D it represents the distance kings must travel between two squares on a chessboard.

The p-norm is rarely used for values of p other than 1, 2, and infinity, but see; super ellipse.

In physical space the Euclidean distance is in a way the most natural one, because in this case the length of a rigid body does not change with rotation.

- d(x,y) ≥ 0, and d(x,y) = 0 if and only if x = y. (Distance is positive between two different points, and is zero precisely from a point to itself.)
- It is symmetric: d(x,y) = d(y,x). (The distance between x and y is the same in either direction.)
- It satisfies the triangle inequality: d(x,z) ≤ d(x,y) + d(y,z). (The distance between two points is the shortest distance along any path).

Such a distance function is known as a metric. Together with the set, it makes up a metric space.

For example, the usual definition of distance between two real numbers x and y is: d(x,y) = |x − y|. This definition satisfies the three conditions above, and corresponds to the standard topology of the real line. But distance on a given set is a definitional choice. Another possible choice is to define: d(x,y) = 0 if x = y, and 1 otherwise. This also defines a metric, but gives a completely different topology, the "discrete topology"; with this definition numbers cannot be arbitrarily close.

Various distance definitions are possible between objects. For example, between celestial bodies one should not confuse the surface-to-surface distance and the center-to-center distance. If the former is much less than the latter, as for a LEO, the first tends to be quoted (altitude), otherwise, e.g. for the Earth-Moon distance, the latter.

There are two common definitions for the distance between two non-empty subsets of a given set:

- One version of distance between two non-empty sets is the infimum of the distances between any two of their respective points, which is the every-day meaning of the word. This is a symmetric prametric. On a collection of sets of which some touch or overlap each other, it is not "separating", because the distance between two different but touching or overlapping sets is zero. Also it is not hemimetric, i.e., the triangle inequality does not hold, except in special cases. Therefore only in special cases this distance makes a collection of sets a metric space.
- The Hausdorff distance is the larger of two values, one being the supremum, for a point ranging over one set, of the infimum, for a second point ranging over the other set, of the distance between the points, and the other value being likewise defined but with the roles of the two sets swapped. This distance makes the set of non-empty compact subsets of a metric space itself a metric space.

The is the infimum of the distances between the point and those in the set. This corresponds to the distance, according to the first-mentioned definition above of the distance between sets, from the set containing only this point to the other set.

In terms of this, the definition of the Hausdorff distance can be simplified: it is the larger of two values, one being the supremum, for a point ranging over one set, of the distance between the point and the set, and the other value being likewise defined but with the roles of the two sets swapped.

Distance cannot be negative. Distance is a scalar quantity, containing only a magnitude, whereas a displacement vector are vector quantities characterized by both magnitude and direction.

The distance covered by a vehicle (often recorded by an odometer), person, animal, or object along a curved path from a point A to a point B should be distinguished from the respective displacement (the distance along a straight line from A to B). For instance, the distance covered during a round trip from A to B and back to A may be very long, while the displacement is always zero (because starting and ending points coincide).

Directed distances are distances with a direction or sense. They can be determined along straight lines and along curved lines. A directed distance along a straight line from A to B is a vector joining any two points in a n-dimensional Euclidean vector space. A directed distance along a curved line is not a vector and is represented by a segment of that curved line defined by endpoints A and B, with some specific information indicating the sense (or direction) of an ideal or real motion from one endpoint of the segment to the other (see figure). For instance, just labelling the two endpoints as A and B can indicate the sense, if the ordered sequence (A, B) is assumed, which implies that A is the starting point.

A displacement (see above) is a special kind of directed distance defined in mechanics. A directed distance is called displacement when it is the distance along a straight line (minimum distance) from A and B, and when A and B are positions occupied by the same particle at two different instants of time. This implies motion of the particle.

Another kind of directed distance is that between two different particles or point masses at a given time. For instance, the distance from the center of gravity of the Earth A and the center of gravity of the Moon B (which does not strictly imply motion from A to B).

- Mahalanobis distance is used in statistics.
- Hamming distance and Lee distance are used in coding theory.
- Levenshtein distance
- Chebyshev distance

- Taxicab geometry
- astronomical units of length
- cosmic distance ladder
- comoving distance
- distance geometry
- distance (graph theory)
- Distance in military affairs
- Dijkstra's algorithm
- distance-based road exit numbers
- Distance Measuring Equipment (DME)
- great-circle distance
- length
- milestone
- Metric (mathematics)
- Metric space
- orders of magnitude (length)
- Proper length
- distance matrix
- Hamming distance
- Free Euclidian Distance
- Lee distance
- proxemics - physical distance between people

- E. Deza, M.M. Deza, Dictionary of Distances, Elsevier (2006) ISBN 0-444-52087-2

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Last updated on Tuesday September 30, 2008 at 10:27:53 PDT (GMT -0700)

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This article is licensed under the GNU Free Documentation License.

Last updated on Tuesday September 30, 2008 at 10:27:53 PDT (GMT -0700)

View this article at Wikipedia.org - Edit this article at Wikipedia.org - Donate to the Wikimedia Foundation

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