Exam 22: The Origin of Structure
Exam 1: Why Learn Astronomy65 Questions
Exam 2: Patterns in the Skymotions of Earth70 Questions
Exam 3: Gravity and Orbitsa Celestial Ballet68 Questions
Exam 4: Light70 Questions
Exam 5: The Tools of the Astronomer68 Questions
Exam 6: The Birth and Evolution of Planetary Systems67 Questions
Exam 7: The Terrestrial Planets and Earths Moon71 Questions
Exam 8: Atmospheres of the Terrestrial Planets71 Questions
Exam 9: Worlds of Gas and Liquidthe Giant Planets68 Questions
Exam 10: Gravity Is More Than Keplers Laws69 Questions
Exam 11: Planetary Adornmentsmoons and Rings68 Questions
Exam 12: Dwarf Planets and Small Solar System Bodies69 Questions
Exam 13: Taking the Measure of Stars70 Questions
Exam 14: A Run-Of-The-Mill G-Type Starour Sun68 Questions
Exam 15: Star Formation and the Interstellar Medium67 Questions
Exam 16: Stars in the Slow Lanelow-Mass Stellar Evolution69 Questions
Exam 17: Live Fast,die Younghigh-Mass Stellar Evolution70 Questions
Exam 18: Our Expanding Universe70 Questions
Exam 19: Galaxies69 Questions
Exam 20: The Milky Waya Normal Spiral Galaxy70 Questions
Exam 21: Modern Cosmology70 Questions
Exam 22: The Origin of Structure45 Questions
Exam 23: Life40 Questions
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In clusters of galaxies,the total mass of dark matter exceeds the luminous matter by about a factor of 1,000.
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The peculiar velocities of galaxies allow us to determine how matter is distributed in the universe.
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