An ellipse is a geometric shape that looks like a stretched-out circle, with two focal points instead of one central point. The sum of the distances from any point on the ellipse to these two focal points is always constant. This unique property makes the ellipse distinctive and different from a circle.
In terms of an ellipse’s dimensions, the longest diameter is called the **major axis**, while the shortest diameter is the **minor axis**.
The semimajor axis, denoted by **a**, is half of the major axis, and the semiminor axis is half of the minor axis.
- An ellipse is symmetrical about both its major and minor axes.
- Its shape is determined by how much the minor axis differs from the major axis.
Ellipses appear in many real-world situations, such as planetary orbits and optics.
In polar coordinates, the equation for an ellipse takes a particular form: \[r=\frac{a(1-e^{2})}{1+e\cos \theta}\]
This formula links the polar angle \(\theta\) with the radial distance \(r\), showing how the ellipse extends out from its focal points.