In physics, astronomy, and engineering, ellipses are prevalent. For example, each planet’s orbit in the Solar System is roughly an ellipse, with the Sun at one focus point (more accurately, the Sun–planet pair’s barycenter). Moons orbiting planets and all other systems of two astronomical bodies are the same. Ellipsoids are widely used to describe the forms of planets and stars. When viewed from a side angle, a circle seems to be an ellipse: the ellipse is the image of a circle projected in parallel or perspective projection. The ellipse is also the simplest Lissajous figure, generated when horizontal and vertical motions have the same frequency: elliptical polarization of light is caused by a similar process.
In terms of locus, an ellipse is the set of all points on an XY plane whose distance from two fixed points (known as foci) equals a constant value. When a plane slices the cone at an angle with the base, the ellipse is one of the conic sections that results. A circle is formed when the cone is intersected by a plane parallel to the base.
The eccentricity of the ellipse is defined as the ratio of distances from the centre of the ellipse to either focus to the semi-major axis of the ellipse.
e = c/a is the eccentricity of an ellipse.
The focal length is c, while the length of the semi-major axis is a.
A plane forms an ellipse when it crosses a cone at an angle with respect to the base. It's a curve with two focal points on either side. Ellipse is a collection of points whose distances from two foci are equal.
The ellipse's primary axis runs parallel to the x-axis and has the greatest width. It measures 2a in length. The vertices of the main axis, with coordinates (ha, k), are the endpoints. The minor axis runs parallel to the y-axis and has the shortest width. It measures 2b in length. The vertices of the minor axis with coordinates (h, kb) are the endpoints.