In geometry, a position or position vector, also known as location vector or radius vector, is a Euclidean vector that represents a point P in space. Its length represents the distance in relation to an arbitrary reference origin O, and its direction represents the angular orientation with respect to given reference axes. Usually denoted x, r, or s, it corresponds to the straight line segment from O to P. In other words, it is the displacement or translation that maps the origin to P:
r = O P → . {\displaystyle \mathbf {r} ={\overrightarrow {OP}}.}
The term position vector is used mostly in the fields of differential geometry, mechanics and occasionally vector calculus. Frequently this is used in two-dimensional or three-dimensional space, but can be easily generalized to Euclidean spaces and affine spaces of any dimension.
Relative position The relative position of a point Q with respect to point P is the Euclidean vector resulting from the subtraction of the two absolute position vectors (each with respect to the origin):
Δ r = s − r = P Q → , {\displaystyle \Delta \mathbf {r} =\mathbf {s} -\mathbf {r} ={\overrightarrow {PQ}},}
where s = O Q → {\displaystyle \mathbf {s} ={\overrightarrow {OQ}}} . The direction between two points is their relative position normalized as a unit vector.
Definition and representation
Three dimensions
In three dimensions, any set of three-dimensional coordinates and their corresponding basis vectors can be used to define the location of a point in space—whichever is the simplest for the task at hand may be used. Commonly, one uses the familiar Cartesian coordinate system, or sometimes spherical polar coordinates, or cylindrical coordinates:
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