In our Sun, the spectral lines of hydrogen are weak, compared to their appearance in hotterstars.

Name: In our Sun, the spectral lines of hydrogen are weak, compared to their appearance in hotterstars.
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This is because in hotter stars, hydrogen atoms have more energy and are excited to higher energy levels, causing them to emit stronger spectral lines. The spectral lines of hydrogen become stronger and more prominent in hotter stars, but in our Sun, they are relatively weak.

In Our Sun, the Spectral Lines of Hydrogen Are Weak