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Polar coordinates

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For an extension to three dimensions, see spherical polar coordinates.
Two dimensional polar coordinates r and θ of vector
Two dimensional polar coordinates r and θ of vector \scriptstyle \vec{\mathbf{r}}

In mathematics and physics, polar coordinates are two numbers—a distance and an angle—that specify the position of a point on a plane.

In their classical ("pre-vector") definition polar coordinates give the position of a point P with respect to a given point O (the pole) and a given line (the polar axis) through O. One real number (r ) gives the distance of P to O and another number (θ) gives the angle of the line OP with the polar axis. Given r and θ, one determines P by constructing a circle of radius r with O as origin, and a line with angle θ measured counterclockwise from the polar axis. The point P is on the intersection of the circle and the line.

In modern vector language one identifies the plane with a real Euclidean space \scriptstyle \mathbb{R}^2 that has a Cartesian coordinate system. The crossing of the Cartesian axes is on the pole, that is, O is the origin of the Cartesian system and the polar axis is identified with the x-axis of the Cartesian system. The line OP is generated by the vector

 
\overrightarrow{OP} \equiv \vec{\mathbf{r}}.

Hence we obtain the figure on the right where \scriptstyle \vec{\mathbf{r}} is the position vector of the point P.

Algebraic definition

The polar coordinates r and θ are related to the Cartesian coordinates x and y through


\begin{align}
r  &=  \sqrt{x^2+y^2} \\
x &= r\cos\theta \\
y &= r \sin\theta, \\
\end{align}

so that for r ≠ 0,


\theta = 
\begin{cases}
\arccos(x/r)         & \hbox{ if } y \ge 0 \\
360^0 - \arccos(x/r) & \hbox{ if } y < 0 .\\
\end{cases}

Bounds on the coordinates are: r ≥ 0 and 0 ≤ θ < 3600. Coordinate lines are: the circle (fixed r, all θ) and a half-line from the origin (fixed direction θ all r). The slope of the half-line is tanθ = y/x.

Surface element

The infinitesimal surface element in polar coordinates is


dA = J\, dr\,d\theta.

The Jacobian J is the determinant


J= \frac{\partial(x,y)}{\partial(r,\theta)} = 
\begin{vmatrix}
\cos\theta &  -r\sin\theta \\
\sin\theta &  r\cos\theta \\
\end{vmatrix} = r \cos^2\theta + r\sin^2\theta 
= r .

Example: the area A of a circle of radius R is given by


A = \int_{0}^{2\pi}  \int_{0}^R r\, dr\, d\theta = \pi R^2 .
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