Each of these 3,000- to 4,000-pound solar-powered satellites circles the globe at about 12,000 miles (19,300 km), making two complete rotations every day. The orbits be arranged so that at any time, anywhere on Earth, there are at least four satellites visible in the sky.
A GPS receivers job is to locate four or more of these satellites, epitome out the distance to each, and use this information to deduce its birth location. This operation is based on a simple numeral principle called trilateration.

2-D Trilateration:
Imagine you are somewhere in the India and you are TOTALLY lost -- for whatever reason, you have absolutely no clue where you are. You find a friendly local and ask, Where am I? He says, You are 2600 Km from Delhi. This is a nice, disfranchised fact, but it is not particularly useful by itself. You could be anywhere on a circle around Delhi that has a radius of 2600 Km, like this:
You ask somebody else where you are, and she says, You are 2650 Km from Lucknow. Now youre getting somewhere. If you combine this information with the Delhi information, you have two circles that intersect. You now know that you must be at one
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