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The density wave theory attempts to explain why the spiral arm structure persists over a long time.

A) True
B) False

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This diagram shows the period- luminosity relationship. A Cepheid variable with a period of 5 days will have a luminosity of _ _ solar luminosities. This diagram shows the period- luminosity relationship. A Cepheid variable with a period of 5 days will have a luminosity of _ _ solar luminosities.

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Open clusters are found in the of our Milky Way Galaxy.

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disc (or s...

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Which of these objects have NOT been found in the Galactic Halo?


A) Population II stars
B) emission nebulae
C) Cepheid variables
D) globular clusters
E) RR Lyrae variables

F) All of the above
G) A) and B)

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Which statement about Population II is false?


A) They formed first as the Galaxy formed.
B) They are made of almost nothing but hydrogen and helium.
C) At almost five billion years old, our Sun must belong to this older Population.
D) Their orbits around the Galaxy resemble those of comets.
E) The globular clusters are their most obvious groupings.

F) A) and B)
G) All of the above

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Cepheids are good examples of cataclysmic variable stars.

A) True
B) False

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Compare the orbital motion of stars in the Galactic disk with those in the halo.

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Stars in the disk orbit the galactic cen...

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All RR Lyrae stars have about the same


A) luminosity of about 100 Suns.
B) galactic location and speed.
C) locations in the centers of globular star clusters.
D) period of six days.
E) distance of 32 light-years.

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

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What are the three main parts of our Galaxy?

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The disk, ...

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It was _ in the Galactic disk that threw Herschel's model of the size and structure of the Galaxy off badly.

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Most of the mass of the Milky Way seems to exist in the form of


A) the black hole in the Galactic Center.
B) dark matter out in the Halo.
C) hydrogen gas in the disk and spiral arms.
D) population II stars in the Halo.
E) population I stars in the disk.

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

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What is one of the differences between Cepheids and RR Lyrae variables?


A) Cepheids are giants, but RR Lyrae stars are still on the main sequence.
B) The pulsations of RR Lyrae stars are much less regular than those of Cepheids.
C) The RR Lyrae stars have much shorter periods than Cepheids.
D) The period- luminosity relation holds only for RR Lyrae stars.
E) All Cepheids have the same brightness, but RR Lyrae stars vary greatly in luminosity.

F) B) and C)
G) B) and D)

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All Cepheid variables discovered so far lie in other galaxies.

A) True
B) False

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To determine the distance to a Cepheid, we must measure its of pulsation.

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Which method relies on the mass of a dark object revealing its presence?


A) temporary brightening of a distant star by a gravity lens
B) asteroidal occultations
C) ring occultations
D) pulsars slowing down irregularly
E) stellar eclipses

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

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According to the ages of the globular clusters, our Galaxy is about times as old as the solar system.

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It would be very unlikely to find a massive, young star out in the halo.

A) True
B) False

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Which of these is NOT typical of the Galaxy's spiral arms?


A) O and B stars
B) Population II giants like orange Arcturus
C) emission nebulae like M42
D) hot, young blue Population I stars
E) open clusters

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

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Harlow Shapley found the Milky Way was


A) much larger than previously thought.
B) uniformly spherical in shape.
C) much smaller than previously thought.
D) centered on the Earth.
E) rapidly expanding.

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

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What use are 21- cm radio waves to galactic astronomers?


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

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

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