Would you expect to see hydrogen Balmer lines in the spectra of stars with temperatures of 3200 K?

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Quizplus · Accepted Answer

Stars with temperatures around 3200 K are relatively cool, meaning that most of the hydrogen atoms in their atmospheres have their electrons in the lowest energy level, or ground state. For Balmer lines to be prominent in a star's spectrum, electrons need to be excited to the second energy level before they can transition back down, emitting or absorbing light in the visible range. In cooler stars, there are fewer electrons in the second energy level, making Balmer lines less prominent or absent.

Would You Expect to See Hydrogen Balmer Lines in the Spectra