Tiny variations in the temperature of the cosmic microwave background show variations in the density of the early universe. What mechanism is believed to have made some regions denser and others more rarefied?
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A surface explosion on a white dwarf, produced by falling matter from the atmosphere of its binary companion, produces what sort of object?
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The cosmic background is usually characterized as having a temperature of 2.725 Kelvin - that's 2.725 degrees Celsius above absolute zero. What does it mean to say that these photons have a temperature?
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It's a challenge to determine the best placement for a satellite observatory; you need stable positioning, a clear field of view, and a nice line of sight back to Earth. For deep-sky observations like probes into the cosmic microwave background, it's also
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As the cosmic microwave background is made up of light waves, we can use well-known techniques of wave analysis to examine it. One useful tool includes looking at the angular sizes of variations in the CMB. It turns out that the largest variations in the
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Very nearly uniform in every direction, the cosmic microwave background shows an early universe in thermal equilibrium -- but maybe it's a little too uniform. Its uniformity was originally rather awkward for astrophysicists to explain because it gives ris
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If the Earth were to be compressed down in size until it became a black hole, its Schwarzschild radius would be
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The headline for the March 15, 2010 edition of "Scientific American" read "Star set to collide with solar system". The orange dwarf star called Gliese 710 is considered 86% likely to collide with what part of our solar system within the next million and a
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Given how hard astrophysicists have struggled to make precise measurements of the cosmic microwave background, you might be forgiven for thinking that it's an extremely arcane phenomenon, well out of reach for mere mortals. However, you can see it for you
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Temperature maps of the cosmic microwave background exhibit a remarkable characteristic. Over the entire field of view, one side of the sky appears a bit colder and the other side appears a bit warmer; the difference is about seven-thousandths of a degree
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