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.
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Multiple Choice
A) WIMPs
B) MACHOs
C) black holes
D) clouds of cool, neutral hydrogen
E) brown dwarfs
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Multiple Choice
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.
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Short Answer
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Short Answer
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Essay
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Multiple Choice
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.
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Multiple Choice
A) tidal streams.
B) globular clusters.
C) small satellite galaxies.
D) spiral arms.
E) old white dwarfs.
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Multiple Choice
A) RR Lyrae stars.
B) trigonometric parallaxes.
C) spectroscopic parallaxes.
D) Cepheid variables.
E) pulsars.
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Multiple Choice
A) period-luminosity relation.
B) mass-luminosity relation.
C) instability strip.
D) horizontal branch.
E) main sequence appendix.
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Multiple Choice
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.
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Multiple Choice
A) Galactic bulge.
B) spiral arm.
C) Galactic disk.
D) Galactic halo.
E) globular cluster.
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Multiple Choice
A) RR Lyrae variables
B) T Tauri variables
C) Cepheids
D) cataclysmic variables
E) planetary nebulae
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True/False
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True/False
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True/False
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True/False
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