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  • At this exact wavelength range, the light we see is mainly from objects at around room temperature (300K) to less than a few thousand Kelvin. (This is due to blackbody emission, a concept which you should look up if you are interested or ask me!) By looking at light in the infra-red we can study objects such as big dust and gas clouds, cool dwarf stars, exo-planets, asteroids & comets.
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