Exam 14: Modern Cosmology
Exam 1: Here and Now97 Questions
Exam 2: A Users Guide to the Sky116 Questions
Exam 3: Cycles of the Sun and Moon154 Questions
Exam 4: The Origin of Modern Astronomy144 Questions
Exam 5: Light and Telescopes156 Questions
Exam 6: Atoms and Spectra125 Questions
Exam 7: The Sun146 Questions
Exam 8: The Family of Stars190 Questions
Exam 9: The Formation and Structure of Stars136 Questions
Exam 10: The Deaths of Stars128 Questions
Exam 11: Neutron Stars and Black Holes99 Questions
Exam 12: The Milky Way Galaxy117 Questions
Exam 13: Galaxies: Normal and Active151 Questions
Exam 14: Modern Cosmology112 Questions
Exam 15: Origin of the Solar System and Extrasolar Planets104 Questions
Exam 16: Earth and Moon: Bases for Comparative Planetology98 Questions
Exam 17: Mercury, Venus, and Mars83 Questions
Exam 18: The Outer Solar System137 Questions
Exam 19: Meteorites, Asteroids, and Comets91 Questions
Exam 20: Astrobiology: Life on Other Worlds97 Questions
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The night sky is dark because the Universe is not infinitely old.
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True
Observations of type Ia supernovae reveal that the expansion of the universe is speeding up because of the presence of ___________ in empty space.
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(Short Answer)
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dark energy
During the first moments of the big bang when elements could be created, nuclear fusion reactions made few heavy elements because
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B
Describe how we know that the expansion rate of the Universe is currently accelerating.
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Which of the following simulated curvatures best matches the above observations of non-uniformity (i.e., irregularities) in the CMB?
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If the Universe were infinitely large, infinitely old, and static, then the CMB would appear uniform (i.e., homogenous and isotropic).
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Why is the primordial background radiation visible in all directions?
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Which of the following agrees with a no-center, no-edge Universe?
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Prior to 10-36 seconds, the Universe existed as one unified force.
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The above cartoon shows the present Universe as it appears from the vantage point of our solar system, which is in the upper left corner of the figure. According to the cosmological principle, how will the view change if we turned around 180 degrees and looked in the other direction? How do you know?
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The sum of the baryonic and non-baryonic matter is 27.9% and thus equal to the critical density.
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What do the size and distribution of small scale temperature variations suggest about the geometry of the Universe?
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Most of the elements heavier than helium were made during the first few minutes after the big bang.
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Cosmology is the study of the structure, history, and evolution of the observable Universe.
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