Coordinate system
See Cartesian coordinate system or Coordinates (elementary mathematics) for a more elementary introduction to this topic
In mathematics as applied to geometry, physics or engineering, a coordinate system is a system for assigning a tuple of scalars to each point in an n-dimensional space. "Scalars" in many cases means real numbers, but, depending on context, can mean complex numbers or elements of some other field. More generally, co-ordinates may sometimes be taken from rings or other ring-like algebraic structures.
Although any specific coordinate system is useful for numerical calculations in a given space, the space itself is considered to exist independently of any particular choice of coordinates.
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2 Transformations 3 Systems commonly used 4 Astronomical systems 5 External links |
An example of a coordinate system is to describe a point P in the Euclidean space Rn by an n-tuple
If a subset S of a Euclidean space is mapped continuously onto another topological space, this defines coordinates in the image of S. That can be called a parametrization of the image, since it assigns numbers to points. That correspondence is unique only if the mapping is bijective.
The system of assigning longitude and latitude to geographical locations is a coordinate system. In this case the parametrization fails to be unique at the north and south poles.
A coordinate transformation is a conversion from one system to another, to describe the same space.
Some choices of coordinate systems may lead to paradoxes, for example, close to a black hole, but can be understood by changing the choice of coordinate system. At an actual mathematical singularity the coordinate system breaks down.
Some coordinate systems are the following:
Examples
of real numbers
These numbers r1,...,rn are called the coordinates of the point P.Transformations
Systems commonly used
Astronomical systems
External links