The trajectory of Earth around the Sun can be derived as an ellipse using principles such as the force of attraction between masses and conservation laws. While Kepler initially observed that planets follow elliptical orbits, Newton later proved that this behavior results from gravity's inverse square law. The seasons on Earth are primarily due to the axial tilt, not the elliptical shape of the orbit, as evidenced by the opposite seasons in the northern and southern hemispheres despite the Earth's distance from the Sun. Calculus can simplify the derivation, but it is also achievable through geometric methods as demonstrated by Newton. An experimental idea involving measuring rain circles over time was proposed to observe changes related to Earth's elliptical orbit, though its effectiveness was questioned.