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What can we learn about stars?
Light is split into spectral colours, corresponding to wavelength. Red light has long wavelengths,blue light has short wavelengths. Spectra from hot objects are continuous, like a rainbow ![]() atoms only emit light of specific colours, revealingtheir fingerprints as a line spectrum ![]() atoms in front of a hot object absorb light at these colours, giving an absorption spectrum ![]() | ||||||||||||
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