Orbital Mechanics

Orbital mechanics is a branch of classical mechanics that deals with the motion of objects in space under the influence of gravitational forces. It primarily focuses on the trajectories, forces, and orbits of celestial bodies, such as planets, moons, and satellites, as they move through gravitational fields. Key concepts in orbital mechanics include Kepler’s laws of planetary motion, which describe the orbits of planets around the sun, and Newton’s law of universal gravitation, which explains the gravitational interactions between objects. Orbital mechanics is essential for space navigation, satellite deployment, and understanding the dynamics of various celestial phenomena. It applies mathematical modeling and analysis to predict and optimize the paths of objects in space, facilitating missions that require precise maneuvers and timing.