Exam 21: The Expanding Universe
Exam 1: Thinking Like an Astronomer 97 Questions
Exam 2: Patterns in the Skymotions of Earth and the Moon101 Questions
Exam 3: Motion of Astronomical Bodies99 Questions
Exam 4: Gravity and Orbits100 Questions
Exam 5: Light100 Questions
Exam 6: The Tools of the Astronomer100 Questions
Exam 7: The Formation of Planetary Systems100 Questions
Exam 8: The Terrestrial Planets and Earths Moon100 Questions
Exam 9: Atmospheres of the Terrestrial Planets100 Questions
Exam 10: Worlds of Gas and Liquidthe Giant Planets100 Questions
Exam 11: Planetary Moons and Rings100 Questions
Exam 12: Dwarf Planets and Small Solar System Bodies100 Questions
Exam 13: Taking the Measure of Stars101 Questions
Exam 14: Our Starthe Sun100 Questions
Exam 15: The Interstellar Medium and Star Formation100 Questions
Exam 16: Evolution of Low-Mass Stars100 Questions
Exam 17: Evolution of High-Mass Stars100 Questions
Exam 18: Relativity and Black Holes97 Questions
Exam 19: Galaxies100 Questions
Exam 20: The Milky Waya Normal Spiral Galaxy100 Questions
Exam 21: The Expanding Universe98 Questions
Exam 22: Cosmology100 Questions
Exam 23: Large-Scale Structure in the Universe103 Questions
Exam 24: Life100 Questions
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The COBE and WMAP satellites detected fluctuations in the CMB.On average, how big were these fluctuations, and what do they that tell us about the universe at a redshift of z = 1,000?
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If we lived in a galaxy 1 billion light-years from our own, what would we see?
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It is possible for a galaxy to have an apparent velocity greater than the speed of light.This means that the galaxy
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The apparent recessional velocities of galaxies at large distances are due mainly to
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The existence of the cosmic background radiation tells us that the early universe was
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If a scientist in the distant Andromeda Galaxy studies the hydrogen gas in that galaxy, they will measure ________ what a scientist in our galaxy would measure, studying hydrogen gas
In the Milky Way.
(Multiple Choice)
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If the distance of a galaxy at a redshift z = 0.05 is 220 Mpc, how many years back into the past are we looking when we observe this galaxy?
(Multiple Choice)
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In the early 1960s, physicists Penzias and Wilson detected a persistent noise at a wavelength of about 1 mm in their radio telescope that came from all directions in the sky due to
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The CMB is a snapshot of the radiation in the universe at a redshift of z
1,000 when the universe was about

(Multiple Choice)
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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 = 3.086 * 1019 km and 1 year = 3.154 * 107 s.
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If you measured the distances and recessional velocities for a sample of galaxies and plotted the data to get the figure shown below, what value would you derive for the Hubble constant? 

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If the distance of a galaxy is 5 Mpc, what is its recessional velocity if the Hubble constant is 70 km/s/Mpc?
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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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Galaxy peculiar velocities are typically about 300 km/s.How far away do you have to look in order to see recessional velocities that are 10 times this peculiar velocity? Note that the Hubble constant has a value of 70 km/s/Mpc.
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Explain how the figure below shows evidence supporting the Big Bang theory. 

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Why did Big Bang nucleosynthesis only produce elements less massive than beryllium?
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Briefly explain how an accurate determination of Hubble constant has improved our understanding of cosmology.
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