About this Simulation

This simulation models planetary orbits and gravitational interactions, allowing learners to visualize elliptical paths, adjust orbital parameters, and observe how eccentricity and energy affect motion. Students can explore the relationship between orbital speed, distance, and the forces governing celestial bodies in space.

Learning objectives: Understand Kepler's three laws of planetary motion and their mathematical relationships | Investigate how eccentricity and orbital energy determine planetary trajectories | Analyze the role of gravitational force in maintaining stable orbits