Orbital Velocity Calculator
Calculate the precise speed needed to maintain a stable orbit around any celestial body. From satellites around Earth to planets around the Sun.
Orbital velocity is the speed needed to maintain a stable circular orbit around a celestial body.
Formula: v = √(GM/r)
Where G is the gravitational constant, M is the mass of the central body, and r is the orbital radius.
The Science of Orbital Motion
Orbital velocity is the speed an object needs to maintain a stable circular orbit around a larger body. This velocity creates a perfect balance where the gravitational pull inward equals the centrifugal force outward, keeping the orbiting object at a constant distance.
Understanding orbital velocity is crucial for space missions, satellite deployment, and comprehending how natural celestial bodies like moons and planets maintain their orbits. The closer to the central body, the faster the orbital velocity required!