What Is Orbital Velocity?
Orbital velocity is the speed an object must travel to stay in a stable circular orbit around a more massive body, such as a satellite around Earth or a planet around the Sun. At this speed, the gravitational pull of the central body exactly supplies the centripetal force needed to keep the object curving around it. Too slow and it falls inward; too fast and it escapes.
The Formula
For a circular orbit, orbital velocity is given by
How to Use It
Enter the mass of the central body (for Earth, about 5.972 × 10^{24} kg) and the orbital radius. You can type scientific notation like 5.972e24. The calculator returns the velocity in m/s and km/s, plus the orbital period in seconds.
Worked Example
Consider a satellite orbiting at Earth's surface radius, r = 6.371 × 10^{6} m, with M = 5.972 × 10^{24} kg. Then
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