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Cartesian Coordinates -- from Wolfram MathWorld

Algebra Applied Mathematics Calculus and Analysis Discrete Mathematics Foundations of Mathematics Geometry History and Terminology Number Theory Probability and Statistics Recreational Mathematics Topology Alphabetical Index New in MathWorld Cartesian Coordinates

Cartesian coordinates are rectilinear two- or three-dimensional coordinates (and therefore a special case of curvilinear coordinates) which are also called rectangular coordinates. The two axes of two-dimensional Cartesian coordinates, conventionally denoted the x- and y-axes (a notation due to Descartes), are chosen to be linear and mutually perpendicular. Typically, the -axis is thought of as the "left and right" or horizontal axis while the -axis is thought of as the "up and down" or vertical axis. In two dimensions, the coordinates and may lie anywhere in the interval , and an ordered pair in two-dimensional Cartesian coordinates is often called a point or a 2-vector.

The three-dimensional Cartesian coordinate system is a natural extension of the two-dimensional version formed by the addition of a third "in and out" axis mutually perpendicular to the - and -axes defined above. This new axis is conventionally referred to as the z-axis and the coordinate may lie anywhere in the interval . An ordered triple in three-dimensional Cartesian coordinates is often called a point or a 3-vector.

In René Descartes' original treatise (1637), which introduced the use of coordinates for describing plane curves, the axes were omitted, and only positive values of the - and the -coordinates were considered, since they were defined as distances between points. For an ellipse this meant that, instead of the full picture which we would plot nowadays (left figure), Descartes drew only the upper half (right figure).

The inversion of three-dimensional Cartesian coordinates is called 6-sphere coordinates.

The scale factors of Cartesian coordinates are all unity, . The line element is given by

(1)

and the volume element by

(2)

The gradient has a particularly simple form,

(3)

as does the Laplacian

(4)

The vector Laplacian is

The divergence is

(7)

and the curl is

The gradient of the divergence is

Laplace's equation is separable in Cartesian coordinates.

See also6-Sphere Coordinates

,

Cartesian Geometry

,

Coordinates

,

Helmholtz Differential Equation--Cartesian Coordinates Explore this topic in the MathWorld classroom

Portions of this entry contributed by Christopher Stover

Explore with Wolfram|Alpha ReferencesArfken, G. "Special Coordinate Systems--Rectangular Cartesian Coordinates." §2.3 in Mathematical Methods for Physicists, 3rd ed. Orlando, FL: Academic Press, pp. 94-95, 1985.Moon, P. and Spencer, D. E. "Rectangular Coordinates ." Table 1.01 in Field Theory Handbook, Including Coordinate Systems, Differential Equations, and Their Solutions, 2nd ed. New York: Springer-Verlag, pp. 9-11, 1988.Morse, P. M. and Feshbach, H. Methods of Theoretical Physics, Part I. New York: McGraw-Hill, p. 656, 1953. Referenced on Wolfram|AlphaCartesian Coordinates Cite this as:

Stover, Christopher and Weisstein, Eric W. "Cartesian Coordinates." From MathWorld--A Wolfram Resource. https://mathworld.wolfram.com/CartesianCoordinates.html

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