This document provides an overview of polar coordinates. It defines polar coordinates as using distance from a fixed point called the pole and an angle from a fixed ray. Points are identified by an ordered pair (r,θ) where r is the distance from the pole and θ is the angle from the horizontal ray. There are multiple representations of a point as (r, θ + 2kπ) or (r, θ + (2k+1)π) for any integer k. Polar equations are written in the form r=f(θ). The distance formula for points in the polar plane is √(r1^2 + r2^2 - 2r1r2cos(θ1-θ2)).