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Classical Mechanics

Orbital Velocity

The speed required for a body to maintain a stable circular orbit around a primary gravitational mass at a given radius.

Governing formula v_orb = √(G M / r)
SI unit m/s

In depth

Orbital velocity balances centripetal acceleration with gravitational force (m v² / r = G M m / r²). Low Earth Orbit velocity is approximately 7.8 km/s (17,500 mph).

Examples in the real world

The International Space Station orbiting Earth at approximately 7.66 km/s at an altitude of 400 km.