Hot solids, liquids and dense gases emit approximately continuous thermal spectra. As temperature rises, the peak shifts toward higher frequency or shorter wavelength and emitted intensity increases. A low-density excited atomic gas instead produces distinct emission lines. Their frequencies depend on that element’s allowed energy differences, so a line pattern can identify atoms.
A cooler gas in front of a continuous source absorbs selected frequencies, producing dark absorption lines. These correspond to allowed upward transitions and can be a subset of the element’s emission lines. A mixture can show lines from several elements. For fixed data questions, compare positions rather than overall brightness: intensity can depend on abundance, temperature and excitation. Spectral classification distinguishes evidence about atomic energy levels from the continuous radiation of an incandescent source.
Example 1
Element A emits at 430,520 and 610 nm; B at 450 and 590 nm. A sample has 430,450,520,590 and 610 nm lines. Identify it.
All listed lines match the union of A and B, so the data are consistent with a mixture of A and B.
Example 2
A glowing solid changes from dull red to white as it is heated. Classify its spectrum.
It emits a continuous thermal spectrum whose distribution moves toward shorter wavelengths and becomes more intense.
Watch out: Incandescent dense sources produce continuous spectra; isolated excited atoms produce characteristic line spectra.