Orbital Velocity Calculator
Enter an orbital radius or altitude to compute circular orbit velocity, orbital period, and gravitational acceleration at that orbit.
Use the Orbital Velocity Calculator
Orbit Parameters
Must be ≥ 6,371 km (Earth's mean surface radius).
Common Orbit Presets
Orbital Results
Orbital Period
—
Grav. Acceleration
—
Orbital Radius
—
from Earth's center
Altitude AGL
—
above sea level
Orbit Regime Reference
| Region | Altitude | Approx. Speed |
|---|---|---|
| LEO | 160 – 2,000 km | 7.8 – 6.9 km/s |
| MEO | 2,000 – 35,786 km | 6.9 – 3.07 km/s |
| GEO | 35,786 km | 3.07 km/s |
| HEO / GTO | > 35,786 km | < 3.07 km/s |
| Moon orbit | ~384,400 km | ~1.02 km/s |
Summary
This calculator applies Newton's law of gravitation and the vis-viva equation to find the velocity required to maintain a stable circular orbit at any altitude above Earth. For a circular orbit at radius r from Earth's center, the orbital speed is v = √(GM/r), the period is T = 2π√(r³/GM), and gravitational acceleration is g = GM/r². Enter either the orbital radius measured from Earth's center, or the altitude above sea level, and the tool converts between them automatically.
How it works
- Enter the orbital radius from Earth's center, or switch to altitude mode and enter height above sea level.
- The calculator derives the complementary value using Earth's mean radius (6,371 km).
- Orbital velocity is computed with v = √(GM/r), where GM = 3.986 × 10¹⁴ m³/s².
- Orbital period follows from T = 2π√(r³/GM), converted to hours and minutes.
- Gravitational acceleration at that orbit uses g = GM/r².
- Results update live; use the preset buttons to jump to common orbits instantly.
Use cases
- Estimate the speed and period of a satellite at any target altitude.
- Verify delta-v requirements when designing a transfer orbit maneuver.
- Compare LEO, MEO, and GEO parameters side by side.
- Understand why geostationary satellites orbit at exactly 35,786 km altitude.
- Calculate gravitational acceleration in orbit for microgravity mission planning.
- Teach orbital mechanics and Kepler's third law in classroom settings.
- Cross-check simulation outputs from orbital mechanics software.
- Explore how orbital velocity drops as altitude increases.