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Which of these distance-measuring techniques works for the farthest objects?


A) Parallax
B) Supernovae Ia
C) Tully-Fisher
D) Cepheid variables

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

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At the conclusion of the Shapley-Curtis debate in April 1920,the general understanding of the astronomical community toward the "spiral nebulae" was


A) that the "spiral nebulae" were part of the Milky Way Galaxy.
B) that the "spiral nebulae" were distant island universes like the Milky Way Galaxy.
C) still inconclusive.
D) that some "spiral nebulae" were within the Milky Way Galaxy and others were far outside it.

E) A) and D)
F) C) and D)

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Which of the following statements is NOT characteristic of elliptical galaxies?


A) They are almost devoid of interstellar gas and dust.
B) They stopped forming stars billions of years ago.
C) Different elliptical galaxies appear to be flattened by different amounts.
D) They have a disk and central bulge,but no spiral arms.

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

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What would happen if the Andromeda Galaxy (a spiral about the same size as ours) collided with our own Milky Way Galaxy?


A) The two galaxies would pass through each other,the stars sailing past one another unharmed,while the interstellar gas and dust clouds would collide and stop,thereby becoming extremely heated.
B) The two galaxies would pass through each other almost unchanged,with essentially no interactions at all.
C) The supermassive black holes of the two galaxies would collide and explode,the resulting radiation essentially destroying their stars,planets,and any life forms that there may have been (including us) .
D) All of the gas and dust clouds and a great many of the stars would collide with each other,stopping both galaxies and creating a galactic merger.

E) B) and C)
F) None of the above

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There are two distinct period-luminosity relations,Type I and Type II.


A) Type I is metal rich and more luminous.
B) Type II is metal rich and more luminous.
C) Type I is metal poor and more luminous.
D) Type II is metal poor and more luminous.

E) A) and D)
F) A) and C)

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What evidence suggests that supermassive black holes are at the center of most large galaxies?

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Rapid fluctuations in the brightness of ...

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What is gravitational lensing and what can it be used to detect in astronomy?

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Gravitational lensing is when an object ...

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How were quasars discovered?

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Some strange objects had radio wave sour...

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A barred spiral galaxy has young,hot,blue stars in its disk.

A) True
B) False

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Compared to an E4,an E0 elliptical galaxy appears to


A) be much smaller.
B) be much larger.
C) be nearly perfectly circular.
D) rotate clockwise.

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

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The Tully-Fisher relation can be used for measuring distance.

A) True
B) False

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The Tully-Fisher relation provides a method of determining distances to galaxies by estimating the galaxy luminosity from the measurement of what parameter relating to the 21-centimeter atomic hydrogen radio emission line?


A) Its position and Doppler shift
B) The split between its two components
C) Its width
D) Its intensity

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

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The energy generation mechanism for active galaxies is believed to be


A) large numbers of supernovae erupting simultaneously.
B) cosmic radioactive decay.
C) black holes colliding.
D) accretion disks around supermassive black holes.

E) None of the above
F) B) and C)

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Rapid fluctuations in the brightness of active galaxies indicate that the region that emits radiation is quite small.

A) True
B) False

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Why do we find a larger percentage of spiral galaxies in distant clusters compared to nearby clusters?


A) Distant clusters are younger,and this contrast in the percentage of spirals shows evidence for the natural evolution of spirals into ellipticals.
B) Distant clusters are older,and this contrast in the percentage of spirals shows evidence for the natural evolution of ellipticals into spirals.
C) Over time,galactic collisions and mergers have destroyed many of the spiral arms that give spirals their distinctive appearance.
D) Spirals contain more gas and dust than ellipticals.In older,nearby clusters,less gas and dust remain and fewer spirals are created.

E) B) and C)
F) None of the above

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The following distance-measuring techniques,arranged in order of the distance for which they are most effective,from smallest to greatest,are


A) Cepheid variables,spectroscopic parallax,Type Ia supernovae,Tully-Fisher relation.
B) Spectroscopic parallax,Tully-Fisher relation,Cepheid variables,Type Ia supernovae.
C) Spectroscopic parallax,Cepheid variables,Tully-Fisher relation,Type Ia supernovae.
D) Cepheid variables,spectroscopic variables,Type Ia supernovae,Tully-Fisher relation.

E) None of the above
F) All of the above

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What determines whether a protogalaxy evolves into a spiral or an elliptical galaxy?

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The rate at which stars form within a pr...

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Which one of the following statements is TRUE about clusters of galaxies?


A) The mass observed in the galaxies of the cluster is about 10 times larger than the amount needed to hold the cluster together,causing the cluster to collapse.
B) The mass observed in the galaxies of the cluster is typically almost exactly equal to that needed to hold the cluster together.
C) The mass observed in the galaxies of the cluster is many thousands of times too small to hold the cluster together.
D) The mass observed in the galaxies of the cluster is about 10 times too small to hold the cluster together.

E) None of the above
F) All of the above

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In the Hubble classification scheme for spiral galaxies,the tightness of the winding of the spiral arms appears to be directly related to the


A) overall intrinsic size of the galaxy,or the diameter across the spiral arms.
B) number of globular clusters in the halo of the galaxy.
C) age of the galaxy,as determined from the age of its individual stars.
D) size of the central bulge of the galaxy.

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

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In observations of a double-quasar image produced by gravitational lensing,fluctuations on the intensity of one image appear to be delayed compared to equivalent variations on the other image.Why is this?


A) Rotation of the lensing galaxy has delayed the beam of light on one side compared to the other because of the Doppler effect.
B) One beam has had to pass through material with a greater refractive index than the other beam within the lensing galaxy.
C) The gravitational field of the lensing object slows down the light on one beam compared to the other.
D) The optical path through the gravitational lens producing one image is longer than that for the other image.

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

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