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Short Answer
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Short Answer
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View Answer
Multiple Choice
A) Population II stars
B) emission nebulae
C) Cepheid variables
D) globular clusters
E) RR Lyrae variables
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Multiple Choice
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.
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True/False
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Essay
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View Answer
Multiple Choice
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.
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Essay
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Multiple Choice
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.
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Multiple Choice
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.
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True/False
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Short Answer
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Multiple Choice
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
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Short Answer
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True/False
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Multiple Choice
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
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Multiple Choice
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.
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Multiple Choice
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.
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