Exam 19: The Expanding Universe
Exam 1: Why Learn Astronomy92 Questions
Exam 2: Patterns in the Skymotions of Earth96 Questions
Exam 3: Motion of Astronomical Bodies91 Questions
Exam 4: Gravity and Orbits88 Questions
Exam 5: Light87 Questions
Exam 6: The Tools of the Astronomer94 Questions
Exam 7: The Birth and Evolution of Planetary Systems87 Questions
Exam 8: The Terrestrial Planets and Earths Moon99 Questions
Exam 9: Atmospheres of the Terrestrial Planets92 Questions
Exam 10: Worlds of Gas and Liquid the Giant Planets92 Questions
Exam 11: Planetary Adornmentsmoons and Rings93 Questions
Exam 12: Dwarf Planets and Small Solar System Bodies89 Questions
Exam 13: Taking the Measure of Stars88 Questions
Exam 14: Our Starthe Sun88 Questions
Exam 15: Star Formation and the Interstellar Medium89 Questions
Exam 16: Evolution of Low-Mass Stars90 Questions
Exam 17: Evolution of High-Mass Stars90 Questions
Exam 18: Relativity and Black Holes90 Questions
Exam 19: The Expanding Universe90 Questions
Exam 20: Galaxies95 Questions
Exam 21: The Milky Waya Normal Spiral Galaxy96 Questions
Exam 22: Modern Cosmology92 Questions
Exam 23: Large-Scale Structure in the Universe65 Questions
Exam 24: Life61 Questions
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If the density of normal matter, such as protons and electrons, were higher in the early universe, would there have been more or less 4He made in the Big Bang?
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The cosmic microwave background (CMB) has a temperature of approximately 2.7 K and a Planck blackbody spectrum. Calculate the wavelength where the CMB spectrum peaks.
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What were the positions taken by Heber Curtis and Harlow Shapley in their "Great Debate," and how were both of them partially correct?
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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?
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Astronomers have known that galaxies are separate entities outside of our own for roughly the last:
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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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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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Does the expansion of the Universe make the Sun bigger? What about the Milky Way? Why or why not?
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If the distance of a galaxy is 10 Mpc, what is its recessional velocity if the Hubble constant is 70 km/s/Mpc?
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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 galaxies recessional velocities that are 10 times this peculiar velocity?
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The apparent recessional velocities of galaxies at large distances are due mainly to the actual motions of the galaxies through space.
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What is a standard candle, and why is it useful for measuring distances?
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Name two predictions of the standard Big Bang theory that have been verified by observations.
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Which of the following is NOT a prediction of the standard Big Bang theory that has been successfully verified by observations?
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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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What do astronomers mean when they say that the universe is isotropic?
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If you found a galaxy with an H emission line that had a wavelength of 756.3 nm, what would be the galaxy's redshift? Note that the rest wavelength of the H emission line is 656.3 nm.
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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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The only chemical elements that formed as the universe cooled down after the Big Bang were hydrogen, deuterium, and helium.
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