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The wavelength of the light produced by collisions depends on the speed of the colliding atoms, and the structure of the atom, which varies from one element to the next. Room-temperature collisions typically produce infrared light, higher speed collisions produce optical and ultraviolet light, and collisions typical of multimillion degree gases produce X-rays.
A supernova remnant contains huge quantities of elements such as oxygen, neon, silicon, sulfur, calcium and iron that were made inside the star and expelled into space. It has been estimated that the Cas A supernova remnant contains enough calcium to make several nonillion (a million trillion trillion) glasses of milk.