Review Questions for Lecture 12


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  • Constellation and Sky Lore

    Perseus, Algol

    Review Questions from the Text

    p. 475, 1-10

    Review Terms

    Alpha Particle
    Triple Alpha Process
    Assymptotic Branch
    Horizontal Branch
    Subgiant Branch
    Red Giant Branch
    Helium Flash
    Helium Shell Burning
    Hydrogen Shell Burning

    Review Concepts

    What are the differences between a one-solar mass main sequences star that is one million years old and one which is 5 Billion years old?

    Why do stars run out of fuel? Why doesn't material from the outer regions of the star circulate into the stars center?

    What happens to a stars core when it runs out of hydrogen in its core? What happens to the stars luminosity and surface temperature?

    Why does helium burning begin? What conditions cause helium core burning to start?

    What is degenerate matter? How does this property lead to the helium flash?

    Why does helium shell burning begin?

    Draw an HR diagram. Diagram the evolution of a one-solar mass star from the main sequence to the assymptotic giant branch.