In our solar system, all planets orbit the Sun in elliptical paths, following Kepler’s laws of planetary motion. This heliocentric model, established by Copernicus and refined by Kepler, replaced the geocentric view, placing the Sun at the center. Each planet, including Earth, travels in its distinct orbit, influenced by gravitational forces. The inner planets, like Mercury and Venus, have shorter orbital periods, while outer planets, such as Jupiter and Saturn, take longer to complete their orbits. This synchronized dance of celestial bodies around the Sun illustrates the harmonious gravitational interplay that defines our solar system.