Polar coordinates are a way of representing points in a plane using a distance from a fixed point (the pole or origin) and an angle from a fixed direction (the polar axis or positive x-axis).
A point in polar coordinates is represented as (r, θ), where r is the distance from the origin to the point, and θ is the angle measured in radians from the polar axis to the line segment connecting the origin and the point.
To convert from polar coordinates to rectangular coordinates, you can use the following equations:
x = r * cos(θ)
y = r * sin(θ)
where (x, y) are the rectangular coordinates and (r, θ) are the polar coordinates.
To convert from rectangular coordinates to polar coordinates, you can use the following equations:
r = √(x^2 + y^2)
θ = arctan(y / x)
where (x, y) are the rectangular coordinates and (r, θ) are the polar coordinates.
Equations in polar coordinates often involve the use of θ. For example, the equation r = a represents a circle centered at the origin with radius a, and the equation θ = k represents a line at angle k from the polar axis.
Here are some key points to remember when working with polar coordinates: