Here's a breakdown:

* Continuous Spectrum: This means that the light from the sun contains all wavelengths of visible light (and beyond), making it appear white. This is due to the sun's hot, dense core emitting a broad range of electromagnetic radiation.

* Absorption Lines: Superimposed on this continuous spectrum are dark lines, called Fraunhofer lines. These lines are created when specific wavelengths of light are absorbed by elements in the sun's cooler outer layers and in the Earth's atmosphere.

The presence of these absorption lines allows us to identify the elements present in the sun's atmosphere. This is because each element absorbs specific wavelengths of light, resulting in unique "fingerprints" in the solar spectrum.

Therefore, the light from the sun produces a continuous spectrum with absorption lines.