Q. What is Dark Matter, really?
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A. It's all sorts of planets and other smaller bodies lying outside solar systems.
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Q. Why is it called Dark?
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A. Because it's too cold to give out its own light, and too distant from any star to be visible by reflected light.
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Q. Then how do we know about it?
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A. It includes a lot of mass -- perhaps 90% of a galaxy's mass. This affects the rotation of galaxies, which can be detected.
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Q. Can it be detected directly?
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A. Yes, even very cold bodies radiate, but with Dark Matter this radiation is of long wavelength, in the microwave band.
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Q. So why hasn't it been studied?
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A. It has, but this radiation, called CMBR (Cosmic Microwave Background Radiation), has been wrongly assumed to come from the Big Bang. This has greatly limited what could be deduced.
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Q. Where can more be found about all this?
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