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Based on star counts, 100 years ago most astronomers thought:


A) we lay about 30,000 ly out from the center of the Galaxy.
B) we lay near the center of a disk about 10 kpc wide and 2 kpc thick.
C) we lay in a spiral arm of the largest galaxy in the universe.
D) we lay near the edge of the only galaxy in the universe.
E) we were not a part of any structure larger than the known solar system.

F) None of the above
G) D) and E)

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These objects are no longer considered a good explanation for the dark matter in the Galactichalo.


A) WIMPs
B) MACHOs
C) black holes
D) clouds of cool, neutral hydrogen
E) brown dwarfs

F) A) and B)
G) B) and D)

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The first attempt to map the Galaxy via star counts was done by:


A) Galileo in 1612.
B) William Herschel in the late eighteenth century.
C) Edward Barnard with long exposure photos about 1900.
D) Harlow Shapley with the RR Lyrae variables in 1920.
E) Edwin Hubble with the new 100" Mt. Wilson telescope in the 1930s.

F) A) and E)
G) B) and C)

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In age, Population I stars are typically much ________ than those of Population II.

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The interstellar ________ absorbs light from stars and makes them appear fainter and redderthan they otherwise would appear.

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What is the evidence to support the existence of a black hole at the center of the Milky Way?

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A large amount of activity is present. T...

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What use are 21 cm radio waves to galactic astronomers?


A) They cut through the dusty cocoons to let us watch star birth.
B) We can reflect them off the core of the Galaxy.
C) Their Doppler shifts let us map the motions and locations of gas in the spiral arms.
D) They bounce off stars like our Sun to let us precisely measure their distances.
E) They pick up the cool, dark matter much better than can optical telescopes.

F) B) and E)
G) A) and B)

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In the Galactic halo, we do NOT find:


A) tidal streams.
B) globular clusters.
C) small satellite galaxies.
D) spiral arms.
E) old white dwarfs.

F) A) and B)
G) None of the above

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The period-luminosity relation is critical in finding distances with:


A) RR Lyrae stars.
B) trigonometric parallaxes.
C) spectroscopic parallaxes.
D) Cepheid variables.
E) pulsars.

F) B) and E)
G) A) and E)

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The region on the H-R diagram where pulsating variables occur is called the:


A) period-luminosity relation.
B) mass-luminosity relation.
C) instability strip.
D) horizontal branch.
E) main sequence appendix.

F) A) and D)
G) A) and C)

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Density waves may explain:


A) the lack of blue stars in the Galactic halo.
B) the random orbits of Galactic halo stars.
C) the density of red stars in the Galactic bulge.
D) the spiral arm structure of the Galaxy.
E) the large number of open clusters in the Galactic halo.

F) A) and B)
G) None of the above

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From Earth, the view of the Milky Way is a thin band of stars across the night sky. The partof the Milky Way Galaxy that is described here is the:


A) Galactic bulge.
B) spiral arm.
C) Galactic disk.
D) Galactic halo.
E) globular cluster.

F) A) and D)
G) B) and E)

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For what type of object is the period-luminosity relation used for determining distances?


A) RR Lyrae variables
B) T Tauri variables
C) Cepheids
D) cataclysmic variables
E) planetary nebulae

F) A) and C)
G) A) and B)

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The majority of the mass of the Milky Way lies farther out than the Sun's orbit.

A) True
B) False

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How old is the Galaxy? How do we know this?

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The H-R diagrams of the globular cluster...

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A pulsating variable star with a period of 10 days would be a Cepheid.

A) True
B) False

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Of what is the Galactic halo presumed to be composed? What evidence supports thisconclusion?

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The globular clusters are most obvious, ...

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Spiral arms are regions of star formation, which accounts for their blue color.

A) True
B) False

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Shapley correctly argued that the rotation of the spiral nebulae proved they could not be verydistant.

A) True
B) False

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How are Cepheids and RR Lyrae stars different?

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Cepheids are large mass variable stars w...

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