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After over a decade of planning, construction, and testing,
the IceCube Neutrino Observatory was completed on December 18, 2010. The $279
million dollar project involved constructing the observatory in ice on the
Antarctic plateau at the National Science Foundation's Amundsen-Scott South
Pole Station.
In the deep darkness of the Antarctic ice, the observatory
will record rare collisions of neutrinos, fundamental yet nearly-undetectable sub-atomic
particles. Neutrinos can come from the sun, from cosmic rays interacting with
the Earth's atmosphere, or through astronomical sources like exploding stars in
the Milky Way. Their appeal to astrophysicists is that they hold no charge, so
catching one on-the-move would allow it to be traced back to its point of
origin.
The IceCube observatory is made-up of 5,160 optical sensors
that are arranged in strings that have been lowered and frozen into 86 holes
that reach as far as 8,000 feet in some spots. The holes were bored into the
ice with a 4.8-megawatt hot water drill that was specially designed by The
University of Wisconsin-Madison. The sensor strings are spread over a half-mile
area on each side, which increases the chances a neutrino will hit a hydrogen
or oxygen atom.
From this research, scientists hope to gain insight on
things like dark matter and supersymmetric particles.
Sources: National
Science Foundation, Popular
Science
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