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Nuclear fusion lets sun burn


The way that the sun burns is called nuclear fusion. In the sun, intense gravity forces four atoms of hydrogen to fuse into one atom of helium. One helium weighs a good bit less than four hydrogens, so what happened to the missing mass? According to Einstein's famous equation, E=mc2, even a little mass (m) becomes a lot of energy (E). We observe this extra energy as the light and heat of our burning star, the sun. In fusion it is not the bonds between atoms that are changing but the atoms themselves.
Since the sun's burning occurs without oxygen and there is no oxygen in space, astronauts must carry it with them.
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