Orbital Velocity
Worked example: ISS: Earth mass, r = 6.771e6 m → v = 7.672 km/s. Press Try an example to run it live, then adjust anything.
Enter your known values, leave one input blank, and solves for the missing one. Tap a variable’s symbol to see what it means, with a typical value. Change any unit and the answer follows.
Where Orbital Velocity fits
- Gravitation and orbital mechanics8 formulas
See also
Escape Velocity: Both use central mass and orbital radius.Gravitational Field Strength: Both use central mass and orbital radius.Gravitational Potential Energy (Orbital): Both use central mass and orbital radius.Orbital Period: Both use central mass and orbital radius.Falling around the Earth →
Grade 12Grade 12 Physics
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Orbital Velocity explained
A satellite stays in a circular orbit when gravity supplies exactly the centripetal force it needs: setting GMm/r² equal to mv²/r and cancelling the satellite's mass gives v = √(GM/r). The cancellation is the famous part: orbital speed depends only on the central body's mass and the orbit's radius, never on what is orbiting. The International Space Station, circling Earth (M ≈ 5.97 × 10²⁴ kg) at r ≈ 6.79 × 10⁶ m, moves at √(6.674 × 10⁻¹¹ × 5.97 × 10²⁴ / 6.79 × 10⁶) ≈ 7 660 m/s: about 7.7 km/s, one lap of the planet every 92 minutes.
The inverse square root also explains a counter-intuitive fact: higher orbits are slower. GPS satellites at r ≈ 26 600 km amble along at 3.9 km/s, half the ISS's speed. Astronomers run the formula in reverse constantly: measure a moon's or a star's orbital speed and radius, and M = v²r/G weighs the central body, which is how we know the mass of everything from Jupiter to the black hole at the centre of the Milky Way.
Orbital Velocity formula
- = Orbital velocity (m/s)
- = Central mass (kg)
- = Orbital radius (m)
Cite this page
formula.expert. (2026, October 16). Orbital Velocity Formula & Calculator. https://formula.expert/solvers/orbital-velocity