Earth Orbit Calculator
Calculate circular-orbit period, orbital speed, local escape velocity, and gravitational force for a satellite above Earth.
About Earth orbit calculations
Earth orbit examples
| Altitude and mass | Approximate results | Orbit class |
|---|---|---|
| 400 km; 1,000 kg | Period 5,545 s; speed 7,673 m/s | Representative low Earth orbit near the altitude of a crewed space station. |
| 35,786 km; 500 kg | Period 86,142 s; speed 3,075 m/s | Near geosynchronous altitude, though inclination and longitude behavior require more conditions. |
| 20,200 km; 2,000 kg | Period 43,078 s; speed 3,873 m/s | Representative medium Earth orbit used by navigation satellite constellations. |
How to calculate an Earth orbit
- Enter the circular orbital altitude above Earth's mean surface in kilometers.
- Enter satellite mass in kilograms to calculate gravitational force.
- Select Calculate orbit to evaluate radius-based speed, period, and escape velocity.
- Use the results as ideal two-body estimates and account separately for drag and perturbations.
Earth orbit FAQ
Why does satellite mass not change orbital speed?
Both gravitational force and inertia scale with satellite mass, so mass cancels from the orbital-motion equation. Mass still changes the force shown by the calculator.
Is 35,786 kilometers always geostationary?
That altitude gives approximately the required period. A truly geostationary orbit must also be circular, equatorial, and move eastward.
Does escape velocity mean required delta-v?
No. It is the total local speed for an ideal escape trajectory, while required delta-v depends on the spacecraft's existing velocity and planned maneuver.
Does the calculator include atmospheric drag?
No. It assumes empty space and a spherical Earth, so low-orbit spacecraft will experience real decay not represented here.
Can I use this for an elliptical orbit?
Not directly. Elliptical orbits need semimajor axis and current radius, plus the vis-viva equation for speed at a particular point.