1. Scientists can determine the temperature and chemical composition of stars like the Sun by analyzing their light spectra, which show unique absorption patterns for each element. 2. The Sun cannot be simply a burning ball of gas, as it would have consumed all its fuel long ago. Nuclear fusion within the Sun combines hydrogen nuclei into helium, releasing energy over billions of years. 3. Heavy elements like those found on Earth are produced when larger stars undergo supernovae, fusing hydrogen and helium into heavier elements through successive nuclear fusion until the star explodes, distributing these elements throughout the universe.