Polar equations are a way to describe curves using a relationship between the distance from a fixed point (called the pole or origin) and an angle. Instead of the usual x and y coordinates we use in Cartesian equations, polar equations make use of a radial coordinate, denoted as \( r \), and an angular coordinate, \( \theta \).
- \( r \) represents the radius or the distance from the origin.
- \( \theta \) represents the angle measured from the positive x-axis.
Polar equations are particularly useful for describing shapes that have clear radial symmetry, such as circles and spirals. A typical polar equation like \( r = f(\theta) \) directly relates these polar coordinates. In our example, we have \( r \sin \theta = 1 \), which forms a horizontal line in Cartesian coordinates when transformed, illustrating how polar equations can represent curves in a different yet insightful manner.