Section 1:
• Describe the major processes involved in a star’s birth and initiation of thermonuclear fusion.
• Explain how reactions differ in high mass, intermediate mass, and low mass stars.
Section 2:
• Describe the fates of stars as they leave the main sequence.
• Explain how and why fates of stars differ so dramatically.
• Describe giant and supergiant stars.
• Describe the chemical elements that are produced in their cores and what types of reactions are involved in their production.
• Explain how the color of stars depends on the temperature.
• Describe how the scientific method was applied in determining the source of energy in the Sun and stars.
Section 3:
• Explain degeneracy pressure and its importance to white dwarfs and neutron stars.
• Describe the difference between electron degeneracy pressure and neutron degeneracy pressure.
• Explain the Chandrasekhar limit.
• Describe approximately how much a paperclip made of neutron star matter would weigh on Earth’s surface.
• Describe what type of star (mass, spectral class) can end up as a black hole and the ways astronomers use to spot it.
Section 4:
• Describe the types of stars that may host planets that support life.
• Describe the formation of planetary systems around cool and hot stars.
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