Orbital Velocity Calculator Formula

Understand the math behind the orbital velocity calculator. Each variable explained with a worked example.

Formulas Used

Orbital Velocity

orbital_vel = sqrt(6.6743e-11 * mass_body / orbital_radius)

Orbital Period

orbital_period = 2 * pi * orbital_radius / sqrt(6.6743e-11 * mass_body / orbital_radius)

Variables

VariableDescriptionDefault
mass_bodyMass of Central Body(kg)5.972e+24
orbital_radiusOrbital Radius(m)6771000

How It Works

Orbital Velocity

For a circular orbit, gravitational force provides the centripetal force.

Derivation

Setting G*M*m/r² = m*v²/r and solving:

v = sqrt(G * M / r)

The orbital period is T = 2*pi*r / v.

Worked Example

Low Earth orbit at 400 km altitude (r = 6,371 + 400 = 6,771 km).

mass_body = 5.972e+24orbital_radius = 6771000
  1. 01v = sqrt(G * M / r)
  2. 02v = sqrt(6.6743e-11 * 5.972e24 / 6.771e6)
  3. 03v = sqrt(5.888e7)
  4. 04v ≈ 7,674 m/s
  5. 05T = 2*pi*r / v ≈ 5,541 s ≈ 92.3 minutes

Frequently Asked Questions

How is orbital velocity related to escape velocity?

Escape velocity is sqrt(2) times orbital velocity at the same radius: v_escape = sqrt(2) * v_orbital.

Does a satellite in orbit need fuel to stay in orbit?

In an ideal vacuum, no. In low Earth orbit, atmospheric drag gradually slows the satellite, requiring periodic boosts.

What happens if an orbiting object speeds up?

It moves to a higher orbit. If it reaches escape velocity, it leaves the gravitational field entirely.

Ready to run the numbers?

Open Orbital Velocity Calculator