
The curved path of an object around a star or planet, determined by gravity.An orbit is the curved path an object takes around a star, planet, or other massive body, governed by the pull of gravity. In essence, it is a perpetual falling: the object is constantly drawn toward the central body, but its sideways motion keeps it from ever hitting it. Orbits are not just circles — they can be ellipses, and in complex gravitational environments, they can wobble, tilt, or even reverse direction relative to the host star's spin.
Johannes Kepler first described planetary orbits as ellipses in the early 1600s, based on Tycho Brahe's precise observations. Isaac Newton later explained why they take that shape, showing that gravity alone could produce such paths.
The shape and orientation of an orbit are set by the balance between the object's velocity and the gravitational pull of the central mass. If the object moves fast enough, it escapes; if too slow, it spirals inward. In multi-body systems, like planetary systems with several planets, gravitational interactions can slowly alter orbits over time, causing shifts in tilt, eccentricity, or even flipping them entirely.
Orbital mechanics is used to design satellite trajectories, plan interplanetary missions, and predict the motion of asteroids or comets that might threaten Earth.
Some planets orbit their stars in the opposite direction of the star's rotation, a phenomenon called a retrograde orbit, which likely results from a violent gravitational encounter early in the system's history.






