He needed to find the best explanations for the motions of Mars. There were many theories of how the planets orbited, mostly in a circular motion, but the data didn’t support them. Instead, Kepler found that another shape, the ellipse, worked a lot better. In his book, Kepler states that Mars travels in an elliptical orbit around the sun. He, later, explained the same with other planets, demonstrating that this shape fit the available observations. The further apart both foci are, the longer and skinnier the ellipse. The skinniness parameter is called eccentricity. In our solar system, the orbit of the planets are not very eccentric at all and very close to circular. With his first law of planetary motion, Kepler rejected these circular orbits, and explained the rotational motion of Mars as an