Exam 19: The Expanding Universe
Exam 1: Why Learn Astronomy 86 Questions
Exam 2: Patterns in the Skymotions of Earth89 Questions
Exam 3: Motion of Astronomical Bodies78 Questions
Exam 4: Gravity and Orbits74 Questions
Exam 5: Light81 Questions
Exam 6: The Tools of the Astronomer88 Questions
Exam 7: The Birth and Evolution of Planetary Systems77 Questions
Exam 8: The Terrestrial Planets and Earths Moon82 Questions
Exam 9: Atmospheres of the Terrestrial Planets81 Questions
Exam 10: Worlds of Gas and Liquid the Giant Planets88 Questions
Exam 11: Planetary Adornments Moons and Rings91 Questions
Exam 12: Dwarf Planets and Small Solar System Bodies87 Questions
Exam 13: Taking the Measure of Stars83 Questions
Exam 14: Our Starthe Sun86 Questions
Exam 15: Star Formation and the Interstellar Medium84 Questions
Exam 16: Evolution of Low-Mass Stars88 Questions
Exam 17: Evolution of High-Mass Stars88 Questions
Exam 18: Relativity and Black Holes87 Questions
Exam 19: The Expanding Universe86 Questions
Exam 20: Galaxies93 Questions
Exam 21: The Milky Waya Normal Spiral Galaxy93 Questions
Exam 22: Modern Cosmology85 Questions
Exam 23: Large-Scale Structure in the Universe59 Questions
Exam 24: Life61 Questions
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How did Edwin Hubble definitively prove that "spiral nebulae" were individual galaxies that were separate from the Milky Way?
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Charles Messier published the first galaxy catalog containing over 2,000 nearby galaxies.
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Why is it not possible to look all the way back to the Big Bang itself?
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The temperature of the CMB is hotter on one side of the sky than on the other by approximately 3 mK.What does this tell us?
(Multiple Choice)
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The current temperature of the cosmic microwave background radiation is 17 K.
(True/False)
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According to Hubble's law,as the distance of a galaxy __________ its __________ increases.
(Multiple Choice)
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Order the following objects by the maximum distance they can be detected: Cepheid variables,RR Lyrae stars,Type I supernovae,and low-mass main-sequence stars.Explain your reasoning.
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If the Hubble constant were equal to 50 km/s/Mpc,what would the approximate age of the universe (the Hubble time)be,assuming that the expansion rate has stayed approximately constant over time? Note that 1 Mpc = 3.1 × 1019 km and 1 year = 3.17 × 107 s.
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If the distance of a galaxy at a redshift z 0.5 is 1,800 Mpc,how many years back into the past are we looking when we observe this galaxy?
(Multiple Choice)
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If you found a galaxy with an Hα emission line that had a wavelength of 756.3 nm,what would be the galaxy's redshift? Note that the rest wavelength of the Hα emission line is 656.3 nm.
(Multiple Choice)
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What is a standard candle,and why is it useful for measuring distances?
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In the early 1960s,physicists named Penzias and Wilson detected a persistent noise at a wavelength of 1 mm in their radio telescope that came from all directions in the sky due to:
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In the Great Debate of 1920,Curtis and Shapley argued over whether or not:
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Distant galaxies we can see today with a redshift of z ≈ 6 emitted their light when the universe was:
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We see the universe around us expanding,which gives distant galaxies an apparent velocity of 70 km/s/Mpc.If you were an astronomer living today in a galaxy that was located 1 billion light years away from us,at what rate would you see the galaxies moving away from you?
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You observe a distant quasar in which the Lyman alpha line of hydrogen (rest wavelength = 121.6 nm)is found at a wavelength of 547.2 nm.When the light from this quasar was emitted,how large was the universe compared to its current size?
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When we look at galaxies in the universe and measure their star formation rates,we find that galaxies at redshifts z ≈1 have higher star formation rates than they do now.At that time,the universe was __________ times the size it is today.
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