16.1 Define absolute magnitude. How does the Sun compare in size and brightness to other main-sequence stars? Describe how the H-R diagram is used to determine which stars are “giants.”
16.2 Describe how main-sequence stars become giants. Why are less massive stars thought to age more slowly than more massive stars despite the fact they have much less “fuel”? List the steps thought to be involved in the evolution of Sun-like stars.
16.3 Explain how it is possible for the smallest white dwarfs to be the most massive. What is the final state of a medium-mass (Sun-like) star? How do the “lives” of the most massive stars end? What are the two possible products of this event?
16.4 Compare the three main types of galaxies. What type of galaxy is our Milky Way? Describe a possible scenario for the formation of a large elliptical galaxy.
16.5 Explain how Edwin Hubble used Cepheid variables to change our view of the structure of the universe. In your own words, explain how astronomers determined that the universe is expanding. Which view of the fate of the universe is currently favored: the Big Crunch or the Big Chill?