The elliptical paths of planets in our solar system result from gravitational forces, primarily from the Sun, and the influence of other celestial bodies. For a planet to maintain a circular orbit, its velocity must be precisely balanced with the Sun's gravitational pull, which is rarely the case, leading to elliptical orbits. The planets' orbits are nearly circular due to their formation from a swirling solar nebula, where those on non-circular paths would have collided or been ejected. The center of mass of the solar system lies at one focus of the elliptical orbits, maintaining equilibrium among the planets. This distribution of mass and gravitational interactions ultimately shapes the orbits of the planets around the Sun.