Which type of spectrum, emission or absorption, can be viewed when the light from a hot gas is viewed through a prism (or diffraction grating)?
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Studying the line spectra produced by hot gases and absorbed by cooler gases allows us to identify the elements in stars. When matter is very hot it emits light. This light, when seen through a prism or diffraction grating , shows all wavelengths of visible light. This is called a continuous emission spectrum .
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