Chapter 12
1. How big is the Sun compared to the
Earth?
2. How can we measure the SunŐs size, mass
and temperature?
3. What is the Sun made of? How do we know this?
4. What holds the Sun together?
5. Why doesnŐt the Sun collapse?
6. Why must the interior of the Sun be so
hot?
7. How does energy get to the SunŐs surface
from its core?
8. What visible evidence do we have that the
Sun has a convective zone?
9. What are the photosphere, chromosphere
and corona? Which of these layers
is hottest? How do we know this?
10. How is solar energy generated? In what form(s)
does it leave the core?
11. Explain the Ňsolar neutrino problemÓ and
how its resolution was a good example of the scientific process.
12. What is solar seismology? What does it tell us about the Sun?
13. What is meant by solar activity?
14. What role does magnetic activity play in
solar activity?
15. Why do sunspots appear dark?
16. Ho do a prominence and a flare differ?
17. How do we know there are magnetic fields
in the Sun?
18. What is the solar cycle?
19. What is the period between maximum
sunspot numbers? How does this
differ from the full solar cycle?
20. What is the Maunder minimum? Why is it of interest?
Chapter 13
1. Describe the method of distance
measurement by triangulation.
2. How do astronomers triangulate a starŐs
distance?
3. How is the parsec defined? How big is a parsec compared with a
light-year?
4. How do astronomers measure a starŐs
temperature?
5. What do astronomers mean by an
inverse-square law?
6. What is luminosity? What two characteristics of a star
determine its luminosity?
7. What does a starŐs magnitude measure? Which is brighter, a star of magnitude 1
or a star of magnitude 3?
8. What are the stellar spectral types? Which are hot and which are cool?
9. Why do stars have dark lines in their
spectra?
10. What is different about the spectra of
different types of stars?
11. What is a binary? How are they useful to astronomers?
12. How do visual and spectroscopic binaries
differ?
13. What is an eclipsing binary? What can be learned from eclipsing
binaries?
14. What is the H-R diagram? What are its axes?
15. What is the main sequence?
16. How do we know that giant stars are big
and dwarf stars are small?
17. How does mass vary along the main
sequence?
18. What is the massĐluminosity relation?
19. What is a standard candle and how is it
used?
Chapter 14
1. What processes and forces determine the
structure of stars?
2. Through what stages will the Sun evolve? Through what stages will a high-mass
star evolve?
3. What heats a protostar? How can we observe protostars? Why are they surrounded by dust and gas?
4. What is bipolar flow?
5. What is a T Tauri
star?
6. What is a Bok globule?
7. What determines when a star become a
main-sequence star?
8. How long do stars stay on the main
sequence?
9. What makes a star move off the main
sequence?
10. Where do main-sequence stars end up as
they evolve?
11. Why is it easier for a high-mass star
than for a low-mass star to burn helium?
12. Why do high- and low-mass stars evolve
differently as they become red giants?
13. What is a variable star? What is meant by the period of a
variable star?
14. Where in the H-R diagram are variable
stars found?
15. What is meant by a pulsating star? Why do stars pulsate?
16. What happens to a solar-mass star when
it starts to burn helium in its core?
What does it turn into?
17. What is a planetary nebula?
18. What is one explanation for how a
low-mass star expels its outer layers to make a planetary nebula?
19. What is left when a planetary nebula
dissipates?
20. What makes a high-mass starŐs core
collapse?
21. Why do neutrons form in a massive starŐs
iron core?
22. What is a supernova explosion?
23. What kind of subatomic particles have
been observed when a supernova explodes?
24. How are clusters of stars used to test
theories of stellar evolution?
Chapter 15
1. What are the approximate mass and radius
of a white dwarf compared with those of the Sun?
2. How does a white dwarf form?
3. What keeps a white dwarf hot?
4. Can a white dwarf have a mass of 10
solar masses? Why? What happens if a white dwarf increases
in mass?
5. What is meant by degeneracy
pressure? How is it related to
white dwarfs and neutron stars?
6. Explain what makes a nova occur.
7. What is a neutron star?
8. What are the mass and radius of a
typical neutron star compared with those of the Sun? Can a neutron star have a mass of 10
solar masses?
9. How does a neutron star form?
10. How do we observe neutron stars?
11. What is a pulsar? Does it pulsate?
12. Are all neutron stars
pulsars? Are all pulsars neutron
stars?
13. What creates the beams of radiation seen
in pulsars?
14. What is nonthermal
radiation?
15. What happens when a gravitational wave
moves? What does it affect? Compare this to how light waves move.
16. What is a black hole? Are they truly ŇblackÓ? What properties can they have?
17. What is the Schwarzschild radius?
18. Why might the distance to the event
horizon of a black hole vary depending on which direction you measure from the
center?
19. Can astronomers see black holes? Explain.
20. What is Hawking radiation?