Space Academy · Contents · Chapter 2 · §2.1 · Nederlandse versie

§2.1 How an orbit works

A satellite is constantly falling towards the Earth — but moves sideways so fast that it keeps missing it.

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In plain terms

Throw a ball hard enough and it lands further away. Throw it so hard that the Earth curves away beneath it as it falls, and it never comes down: that is an orbit. The higher up, the slower a satellite needs to go — and the longer a lap takes.

In practice

The ISS at ± 400 km races round the Earth in an hour and a half and is visible to an observer on the ground for only a few minutes. A communications satellite at 35,786 km takes exactly one day and therefore seems to hang still: a dish can stay fixed on it.

Three quantities are tied together: altitude, speed and orbital period. Choose the altitude and the other two are fixed (for a circular orbit). Lower means faster and a shorter lap; higher means slower and a longer one.

AltitudeSpeedPeriodExample
400 km± 7.7 km/s± 92 minISS
550 km± 7.6 km/s± 95 minStarlink
800 km± 7.5 km/s± 101 minEarth observation (sun-synchronous)
20,200 km± 3.9 km/s± 12 hoursGPS
35,786 km± 3.1 km/s23 h 56 minGeostationary (GEO)

Besides altitude, the inclination — the angle between the orbital plane and the equator — determines which part of the Earth a satellite passes over. An orbit inclined at 53° never goes above 53° north or south; a polar orbit (± 90°) goes everywhere. An elliptical orbit has a lowest point (perigee) and a highest point (apogee); near apogee the satellite moves slowest and dwells over the same area for a long time.

Try it yourself: pick an orbit or slide the altitude, and see what happens to speed, period, the visible part of the Earth and the delay of a signal.