Mechanics

Orbital Velocity

v=GMrv = \sqrt{\frac{GM}{r}}

Velocity for circular orbit at radius r.

Variables

v
Orbital velocity
Circular orbit speed
m/s
G
Gravitational constant
6.674×10⁻¹¹
In SI units: m³/(kg·s²)
Allowed values: greater than 0
N·m²/kg²
M
Central mass
Mass being orbited
Allowed values: greater than 0
kg
r
Orbital radius
Distance from center
Allowed values: greater than 0
m

Derivation

Set gravitational force = centripetal force: GMm/r² = mv²/r.

Your notes

0/5000

Constants in this formula

G
6.674 30 × 10⁻¹¹ ± 0.000 15 × 10⁻¹¹. Measured (CODATA 2018).
N·m²/kg²

Check value

Round inputs run through this page's calculator, with each constant at its tabulated value. Use it to test your own working or a rearranged form. It is a test case, not a real-world example.

  • G = 6.674 30 × 10⁻¹¹ N·m²/kg² (Gravitational constant)
  • M = 2 kg (Central mass)
  • r = 3 m (Orbital radius)

Result: v = 6.670482 × 10⁻⁶ m/s

Other mechanics formulas with the same quantities

Where this formula is listed

Common questions

What is the Orbital Velocity formula?

Orbital Velocity is written v = √(GM/r). Velocity for circular orbit at radius r. It belongs to Mechanics, under Gravitation.

What are the units in v = √(GM/r)?

In SI units, v is orbital velocity, measured in m/s; G is gravitational constant, measured in m³/(kg·s²); M is central mass, measured in kg; r is orbital radius, measured in m.

How is the Orbital Velocity formula derived?

Set gravitational force = centripetal force: GMm/r² = mv²/r. The result is v = √(GM/r).