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Transcript
Review 4
Chapters 22: The Milky way
How do we know that there is gas and dust in interstellar space? How were the size and shape
of the Milky Way discovered? What is the shape, form, structure, and various parts of the
Milky Way? Where is our sun located in the Milky Way? Why do astronomers think that much
of the Milky Way consists of “dark matter”? Why does the galaxy have spiral arms? Is there a
massive black hole at the center of the galaxy? What is an HII region and how does it evolve?
What is the origin of the 21 cm line and how do we utilize it in astronomy? What are the
various types of nebulae in the Milky Way?
Chapter 23:
What are the different kinds of galaxies? How have astronomers determined the distances to
galaxies? What makes astronomers think that galaxies contain vast amounts of dark matter?
How do we think galaxies formed? Why do nearly all galaxies have redshifted spectra? Why
do the red-shifts of galaxies increase with their distances?
A galaxy is moving away from us at a speed of 30,000 km/s . How far is the galaxy away
from us?
Hint: Use Hubble’s law: V=H d and take the value of H from the book and the above
value for V and solve for d. Make sure that you find d in the correct units. For this you
may need to convert the units of Hubble’s constant H in the right units.
Chapter 24-25:
What is the significance of the large red-shifts of quasars? Why are quasars so luminous yet so
small? In which part of the spectrum do the quasars emit most of the energy? How old are the
quasars? Why do the components of some quasars seem to be moving apart faster than the
speed of light?
To what extent are galaxies found in clusters rather than in isolation? Are galaxies in clusters
different from galaxies not in clusters? What evidence do we have that there is dark matter?
How are galaxies and clusters of galaxies distributed in space? Why are there enormous voids
in which there are few galaxies?
What does Hubble’s law tell us about the beginning of the universe? How can
we tell how old the universe is? Can space itself be curved? What does that mean? How could
we tell? What important events happened early in the history of the universe? What will the
future of the universe be like?
Chapters 26:
Use a value for Hubble’s constant of 70 km/s/Mpc to calculate the age of the Universe
assuming a constant rate of expansion.