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.
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)
| Symbol | Meaning | Unit |
|---|---|---|
| r | radial distance from the origin (pole) | length units |
| θ | angular coordinate measured counterclockwise from positive x-axis | radians or degrees |
| x | Cartesian horizontal coordinate | length units |
| y | Cartesian vertical coordinate | length units |
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).
| Curve Name | Polar Equation | Shape | Application |
|---|---|---|---|
| Circle (centred at origin) | r = a | Perfect circle, radius a | Antenna coverage patterns |
| Archimedean Spiral | r = aθ | Outward spiral | Watch spring, vinyl grooves |
| Rose Curve (4 petals) | r = a·cos(2θ) | Four-petal flower | Antenna radiation patterns |
| Limaçon | r = a + b·cos(θ) | Teardrop or dimpled loop | Gear and cam design |
| Lemniscate | r² = a²·cos(2θ) | Figure-eight shape | Complex analysis |
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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).
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.
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.