Earth Orbit Calculator

Calculate circular-orbit period, orbital speed, local escape velocity, and gravitational force for a satellite above Earth.

Calculate satellite orbit parameters
Enter altitude above mean Earth radius and satellite mass for an ideal circular two-body orbit.

About Earth orbit calculations

An Earth orbit is a continuous free fall in which a spacecraft moves sideways quickly enough that Earth's curved surface falls away beneath it. For an ideal circular orbit, altitude determines orbital radius, speed, and period. This calculator adds the entered altitude to a mean Earth radius of 6,371 kilometers and applies the standard gravitational parameter for Earth, 3.986004418 × 10^14 cubic meters per second squared. Circular orbital velocity is the square root of Earth's gravitational parameter divided by orbital radius. A lower orbit requires a higher speed because gravity is stronger closer to Earth. Orbital period follows Kepler's third law: two pi multiplied by the square root of radius cubed divided by the gravitational parameter. Period increases rapidly with altitude, from roughly ninety minutes in low Earth orbit to nearly one sidereal day near geosynchronous altitude. Local escape velocity is the minimum ideal instantaneous speed needed to depart from the current radius without further propulsion, ignoring the atmosphere and other bodies. It equals the circular speed multiplied by the square root of two. A satellite already in circular orbit would need a velocity change to reach escape speed; the displayed number is the total local speed, not the required engine delta-v. Gravitational force depends on satellite mass as well as radius. The calculator multiplies satellite mass by Earth's gravitational parameter and divides by radius squared. Mass does not affect orbital speed or period in this two-body approximation because inertial and gravitational mass cancel, but doubling satellite mass doubles the gravitational force. The corresponding acceleration remains the same. Real missions require more detailed models. Earth is oblate, its atmosphere creates drag in low orbit, the Moon and Sun perturb trajectories, and spacecraft often travel on elliptical rather than circular paths. Altitude also varies over uneven terrain, whereas this calculator references a mean spherical radius. Use these outputs for education, preliminary estimates, and consistency checks. Mission design and operational navigation require validated ephemerides, perturbation models, coordinate systems, and safety margins.

Earth orbit examples

Altitude and massApproximate resultsOrbit class
400 km; 1,000 kgPeriod 5,545 s; speed 7,673 m/sRepresentative low Earth orbit near the altitude of a crewed space station.
35,786 km; 500 kgPeriod 86,142 s; speed 3,075 m/sNear geosynchronous altitude, though inclination and longitude behavior require more conditions.
20,200 km; 2,000 kgPeriod 43,078 s; speed 3,873 m/sRepresentative medium Earth orbit used by navigation satellite constellations.

How to calculate an Earth orbit

  1. Enter the circular orbital altitude above Earth's mean surface in kilometers.
  2. Enter satellite mass in kilograms to calculate gravitational force.
  3. Select Calculate orbit to evaluate radius-based speed, period, and escape velocity.
  4. 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.