MathematicsTrigonometryMedium

Polar Coordinates

Also known as:polar systemradial coordinatesplane polar coordinates

Polar coordinates are a two-dimensional coordinate system in which each point in the plane is specified by a radial distance r from a fixed origin (pole) and an angle θ measured from a fixed reference direction (polar axis), written as the ordered pair (r, θ). Unlike Cartesian coordinates that use perpendicular axes, polar coordinates are natural for describing curves with rotational symmetry such as circles, spirals, roses, and limaçons. They are widely used in physics (orbital mechanics, wave interference), engineering (antenna patterns), and complex number representation.

Key Formula

x = r·cos(θ), y = r·sin(θ); r = √(x² + y²), θ = arctan(y/x)

LaTeX: x = r\cos\theta,\quad y = r\sin\theta,\quad r = \sqrt{x^2 + y^2},\quad \theta = \arctan\!\left(\frac{y}{x}\right)

SymbolMeaningUnit
rradial distance from the origin (pole)length units
θangular coordinate measured counterclockwise from positive x-axisradians or degrees
xCartesian horizontal coordinatelength units
yCartesian vertical coordinatelength units

Worked Example

Problem

Convert the Cartesian point (3, −3) to polar coordinates, and convert the polar point (4, 2π/3) to Cartesian coordinates.

Solution

Part 1 — Cartesian to Polar: r = √(3² + (−3)²) = √(9 + 9) = √18 = 3√2 ≈ 4.243. θ = arctan(−3/3) = arctan(−1) = −45° = −π/4. Since point is in quadrant IV, θ = −π/4 (or equivalently 7π/4). Polar form: (3√2, −π/4). Part 2 — Polar to Cartesian: x = 4·cos(2π/3) = 4 × (−1/2) = −2. y = 4·sin(2π/3) = 4 × (√3/2) = 2√3 ≈ 3.464. Cartesian form: (−2, 2√3).

Answer

Part 1: (3√2, −π/4) ≈ (4.24, −45°). Part 2: (−2, 2√3) ≈ (−2, 3.46).

Common Polar Curves and Their Equations

Curve NamePolar EquationShapeApplication
Circle (centred at origin)r = aPerfect circle, radius aAntenna coverage patterns
Archimedean Spiralr = aθOutward spiralWatch spring, vinyl grooves
Rose Curve (4 petals)r = a·cos(2θ)Four-petal flowerAntenna radiation patterns
Limaçonr = a + b·cos(θ)Teardrop or dimpled loopGear and cam design
Lemniscater² = a²·cos(2θ)Figure-eight shapeComplex analysis

Interactive Tools

Desmos Graphing Calculator

Switch to polar mode and plot polar equations such as r = a·cos(nθ) interactively.

Open Tool

GeoGebra

Construct and convert between polar and Cartesian coordinate systems dynamically.

Open Tool

Wolfram Alpha

Plot polar curves, convert coordinates, and compute areas enclosed by polar curves.

Open Tool
Polar coordinate grid showing radial lines and concentric circles with angle labels

Wikimedia Commons, CC BY-SA

Related Terms

Mathematics

Radian

A radian is the SI unit of angular measure defined as the angle subtended at the centre of a circle by an arc whose length equals the radius of the circle. Since the full circumference is 2πr, one complete revolution equals 2π radians, giving the exact conversion 180° = π radians. Radians are the natural unit for trigonometry and calculus because they make derivative formulas for trigonometric functions simple (d/dθ sin θ = cos θ holds only when θ is in radians).

Mathematics

Sine Function

The sine function is a fundamental trigonometric function defined for an angle θ in a right triangle as the ratio of the length of the side opposite the angle to the length of the hypotenuse, extended to all real numbers via the unit circle. It is a periodic function with period 2π, amplitude 1, and range [−1, 1], producing a smooth oscillating wave. Sine is essential in modelling wave phenomena including sound, light, alternating current, and simple harmonic motion.

Mathematics

Spherical Geometry

Spherical geometry is the study of figures on the surface of a sphere, where the analogue of a straight line is a great circle (the intersection of the sphere with a plane through its centre). Unlike Euclidean geometry, the angles of a spherical triangle sum to more than 180°, parallel lines do not exist, and the shortest path between two points is along a great-circle arc. It is essential in navigation (great-circle routes), astronomy (celestial coordinates), geodesy (Earth's shape and GPS calculations), and general relativity.

The polar coordinate system was formalised by Isaac Newton in his Methodus Fluxionum (written c. 1671, published 1736) and independently by Jacob Bernoulli in 1691. The term "polar" derives from the Latin polus ("pivot, pole"), itself from Greek polos ("axis, pivot"). Newton used the pole and radius vector (now called r) as primary descriptors.

polar-coordinatestrigonometrycoordinate-systemcomplex-numbersspiralgeometry