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  GPS satellites

GPS satellites

 

Satellites sometimes hunt in packs, or constellations as they are sometimes called. A good example of this is the Global Positioning System (GPS) satellites, which are used for navigation. Using these satellites it is now possible to find out where you are to within just a few metres anywhere on Earth.

 

Image of all of the GPS satellites orbiting the Earth

 

Each GPS satellite sends radio signals down to Earth all the time. The GPS receivers on the ground pick up these signals. A computer in each receiver compares the arrival times of signals from different satellites. It can then calculate the position from this information.

 

This special navigation system is now being used in planes, boats and even cars.

 

The GPS orbits are arranged so that at least four satellites are visible at anytime from anywhere on Earth.

GPS comprises a constellation of 24 satellites. Each is in a 12 hour orbit at a height of 20,000 km above the ground.

 

 

Did you know? The GPS technology is now so advanced that it is like having every metre square of the Earth's surface numbered!

 

This animation shows the view of Earth which six GPS satellites had at one moment last year. All six satellites could see London and from their signals a GPS receiver in London could have worked out its precise location.

 

Centuries ago, how did sailors know where they were when they were out of sight of land? Often they didn't! It was not unusual to get lost and end up shipwrecked.

 

Latitude was easily measured using the position of the Sun or stars, but how did the sailors measure their longitude? It was a very difficult problem to solve. In 1714 a prize of 20,000 pounds (a lot of money in those days!) was offered to anyone who could provide an accurate way to measure longitude at sea.

 

Image of John Harrison and his timekeeperA very clever watchmaker called John Harrison eventually won the prize by making a clock which kept accurate time, even in stormy weather. With this clock, the sailors were able to keep track of the time at the place the ship sailed from. The difference between that clock time and the 'local noon' (when the Sun is highest in the sky) could be used to calculate their longitude.

 

 

John Harrison and his timekeeper.

 

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