The Sun contains a lot of hot gas,so why do we observe an absorption spectrum rather than an emission spectrum from it?

Question

Quizplus · Accepted Answer

The Sun's photosphere is the outermost layer visible to us, and it has a temperature of around 5,500 degrees Celsius. However, the layers below it, such as the chromosphere and the corona, are hotter. This leads to a situation where the photosphere acts as a cooler "lid" over the hotter layers beneath it. The hot gas in the layers below emits a continuous spectrum, but as it passes through the cooler photosphere, some of the light is absorbed, creating an absorption spectrum.

The Sun Contains a Lot of Hot Gas,so Why Do