Exam 25: Galaxies and Dark Matter: The Large-Scale Structure of the Cosmos
Exam 1: Charting the Heavens: The Foundations of Astronomy106 Questions
Exam 2: The Copernican Revolution: The Birth of Modern Science105 Questions
Exam 3: Radiation: Information From the Cosmos113 Questions
Exam 4: Spectroscopy: the Inner Workings of Atoms99 Questions
Exam 5: Telescopes: The Tools of Astronomy111 Questions
Exam 6: The Solar System: Comparative Planetology and Formation Models152 Questions
Exam 7: Earth: Our Home in Space108 Questions
Exam 8: The Moon and Mercury: Scorched and Battered Worlds113 Questions
Exam 9: Venus: Earths Sister Planet96 Questions
Exam 10: Mars: a Near Miss for Life110 Questions
Exam 11: Jupiter: Giant of the Solar System115 Questions
Exam 12: Saturn: Spectacular Rings and Mysterious Moons123 Questions
Exam 13: Uranus and Neptune: The Outer Worlds of the Solar System116 Questions
Exam 14: Solar System Debris: Keys to Our Origin141 Questions
Exam 15: Exoplanets: Planetary Systems Beyond Our Own81 Questions
Exam 16: The Sun: Our Parent Star118 Questions
Exam 17: The Stars: Giants, Dwarfs, and the Main Sequence115 Questions
Exam 18: The Interstellar Medium: Gas and Dust Among the Stars105 Questions
Exam 19: Star Formation: a Traumatic Birth114 Questions
Exam 20: Stellar Evolution: The Life and Death of a Star108 Questions
Exam 21: Stellar Explosions: Novae, Supernovae, and the Formation of the Elements108 Questions
Exam 22: Neutron Stars and Black Holes: Strange States of Matter130 Questions
Exam 23: The Milky Way Galaxy: a Spiral in Space110 Questions
Exam 24: Galaxies: Building Blocks of the Universe107 Questions
Exam 25: Galaxies and Dark Matter: The Large-Scale Structure of the Cosmos106 Questions
Exam 26: Cosmology: The Big Bang and the Fate of the Universe102 Questions
Exam 27: The Early Universe: Toward the Beginning of Time113 Questions
Exam 28: Life in the Universe: Are We Alone106 Questions
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A nearby galaxy has a radius of 4,000 million A.U. and rotates once every 800 million years.What is its mass in solar masses?
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Using Kepler's third law, nd using solar system units of years,A.U.s, and solar masses, the sum of the masses must be M + m = solar masses. The sum ofthe masses, in this case represents the total mass of the galaxy.
Giant elliptical galaxies may be the result of ________ in the centers of rich clusters.
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galaxy mergers (or cannibalism)
How do head-tail radio galaxies reveal their motion?
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Their bipolar jets shock the intergalactic medium and trail behind the moving galaxylike the wake of a boat.
In its most energetic phase, a quasar can probably only last:
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What evidence has Chandra found to contradict the hypothesis that black holes merge duringgalaxy collisions?
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Why would galaxies colliding in a small cluster tend to stick together, while galaxies in alarge cluster tend to pass through each other?
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Explain the significance of the Lyman Alpha Forest in studying the universe on the grandestof scales.
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The huge, dark, almost spherical regions between the superclusters of galaxies are called________.
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Which of these is NOT considered a fine example of galactic collisions?
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Vast majority of the known volume of the universe lies in the voids.
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Contrast the results of a collision between two spiral galaxies on their stars and their gas anddust clouds.
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That we can see two images of the same quasar is due to a(n)________ lens formed by amassive galaxy lying in front of the quasar.
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In a collision between clusters of galaxies, what happens to the hot gas and dark matter,based on observations of the "bullet cluster"?
(Multiple Choice)
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Gas that has never been cycled through a galaxy or a star is said to be ________.
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Careful observations of nearby normal and active galaxies reveal that the mass of the centralblack hole is well correlated with the mass of the galactic bulge. The ratio of bulge mass to blackhole mass is roughly:
(Multiple Choice)
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While quasars may have now vanished, the large black holes they formed are still around,just not being fed as well any more.
(True/False)
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