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I. Multiple Choice Questions · Q10

Q.Fraunhofer lines are an example of _______ spectrum.

(a) line emission
(b) line absorption
(c) band emission
(d) band absorption
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Step 1. Fraunhofer lines are the large number of dark lines observed when the Sun's spectrum is examined closely.

Step 2. These dark lines arise because light from the Sun's hot interior passes outward through its cooler outer atmosphere, where specific elements absorb light at their own characteristic wavelengths, leaving those wavelengths missing (dark) against the otherwise continuous background.

Step 3. Since the dark features are individual sharp lines (not broad bands), and they arise from absorption (not emission), this is by definition a line absorption spectrum. …

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