| Radiotelephones and Radio Waves | |||||||||||||||||||||||||
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| Cosmic Background radiation travels in the form of microwaves (not the ovens), which are basically high-frequency radio waves. See the link to Radiation below for more information on the electromagnetic spectrum This picture shows images of CMB taken from when it was first discovered to the present. Although it is quite constant ( at 2.7 degrees K) scientists have found that there are slight fluctuations in this temperature. This information suggests that the universe was quite "smooth" at its creation, meaning that with a few minor exceptions, most of matter was pretty much the same. |
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| Radiation | |||||||||||||||||||||||||
| Pictures Found at: http://imagine.gsfc.nasa.gov/docs/science/.html | |||||||||||||||||||||||||
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| Picture from: http://map.gsfc.nasa.gov/m_uni/uni_101bbtest1.html | |||||||||||||||||||||||||
| Hubble�s Experiments In the early 1920�s, the idea that the universe was growing larger was ludicrous. Although Albert Einstein�s Theory of Relativity actually supported this idea, he added the �Cosmological Concept� to his theory in order eliminate the apparent support for an expanding universe. Aleksandr Friedmann was the first to suggest that Einstein�s concept was true without the correction, but he was unable to prove this. Hubble was able to prove the accuracy of Einstein�s initial theory however, by observing distant galaxies and recording data that confirmed the notion that the farther a galaxy was from any point in the universe, the faster away it was moving from that point. |
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| Aleksander: Close, but no cigar | |||||||||||||||||||||||||
| Picture from: http://bubba.ucdavis.edu/~mchu/graphics/Friedmann.jpeg | |||||||||||||||||||||||||