Polar equations are a way to represent curves using the polar coordinate system. This system is different from the regular Cartesian coordinate system you might be more familiar with. Instead of using x and y to describe a point on a plane, polar coordinates use two values: the radius \( r \) and the angle \( \theta \). The radius is the distance from the origin to the point, while the angle is measured from the positive x-axis.
In the context of conics, polar equations can represent different types of shapes like ellipses, parabolas, and hyperbolas, depending on the eccentricity. The standard form of a polar equation for a conic section with a focus at the origin is:
- If the directrix is horizontal: \( r = \frac{ed}{1 \, \pm \, e \sin \theta} \)
- If the directrix is vertical: \( r = \frac{ed}{1 \, \pm \, e \cos \theta} \)
In these equations, \( e \) is the eccentricity, \( d \) is the distance of the directrix from the origin, and \( \theta \) is the angle in polar coordinates. Using these formulas, you can rewrite given Cartesian equations in polar form, gaining insight into the nature of the conic section.