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Satellites, Science of
Many of our modern global communication systems depend on satellite technology. In the most general sense, a satellite is any object that orbits another object in space. Hence the Earth is a satellite of the sun, and the moon is a satellite of the Earth. However, when thinking about satellites today, most human-made satellites in orbit around the Earth come to mind. These are critical to any number of modern technological systems. They enable communication across continents but also monitor the Earth's weather, look for evidence of climate change, help us create accurate maps, and track everything from the movements of arms and armies to the delivery of packages.
Any object in orbit is actually a satellite, from a dropped wrench used by an astronaut to the International Space Station (ISS). There are more than 500 human-made operational satellites in orbit as of 2009, and over 8,000 separate human-made objects larger than 10 centimeters (baseball sized) tracked by the Space Surveillance Network (SSN), mostly items referred to as “space junk.” The SSN has tracked over 24,500 objects in space since 1957, the year that the Sputnik, created by the Union of Soviet Socialist Republics (USSR), became the first-ever human-made satellite.
Every human-made satellite goes through different stages in its life. First it must be designed, built, and tested. Then it must be launched into a specific orbit. It must be properly deployed and activated. Then it has a normal operational life span as it completes many orbits, doing whatever tasks it is meant to. When the satellite reaches the end of its useful life span, it is disposed of. At any point in this general timeline, there are many opportunities for things to go wrong.
Design
Depending on its type and size, a satellite may have one function or many. The ISS is the largest object currently in orbit. It would weigh roughly 670,000 pounds on Earth and is 240 feet long. Up to six people can live onboard and conduct many different kinds of experiments in the weightless (micro-gravity) environment. As there is no single rocket that can lift an object that large, it has been constructed in space one module at a time, starting with the Zarya and Unity modules in 1998. On the other end of the spectrum are “picosatellites” weighing less than two pounds. Because every ounce sent into orbit costs a significant amount of money (the heavier the satellite, the harder and more expensive it is to launch), mass is usually the primary constraint on the design of satellites.
The other key aspect of satellite design is its purpose. For each task that the satellite will need to do (relaying communications, astronomy, weather observation), it will need specific instruments on board (transmitters and receivers, a telescope, and perhaps a thermal imaging camera, respectively). These instruments are often called the “payload” of the satellite. Again, cost is the key constraint here. All the instruments, plus the batteries or solar arrays needed to power them and the electronics needed to control them, need to be as small and light as possible to reduce overall cost. Various subsystems will need to be designed, such as attitude determination and control (AD&C), communications, command and data handling (C&DH), power, thermal, and guidance and navigation (G&C).
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