Exam 15: Origin of the Solar System and Extrasolar Planets
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 oldest objects found so far in our solar system are Earth rocks that are 1 billion years old.
(True/False)
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We observe a planet crossing in front of its host star and the planet is smaller than the star. We call this crossing motion a ____________.
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The iron in our solar system was created from smaller-mass atomic nuclei in
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The ___________ hypothesis of the formation of the solar system uses sudden events that drastically alter the form of the early solar system.
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Once a terrestrial planet had formed from a large number of planetesimals, heat could have melted it and allowed it to differentiate into a metallic core of ____________density and a rocky mantle or crust of ____________ density.
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A meteoroid, meteor, and meteorite could come from the same celestial body.
(True/False)
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All planets in the solar system orbit counterclockwise as seen from the north.
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All old surfaces in the solar system were heavily cratered during the ________________ period by leftover debris from when the planets formed.
(Short Answer)
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Describe some characteristics that all the planets seem to share and use the solar nebula theory to explain them.
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The speed of the solar wind is approximately 400 km/s and the distance from the Sun to Saturn is 9.5 AU (1 AU = 1.5 × 108 km). How long does it take a particle in the solar wind to reach Saturn?
(Multiple Choice)
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How do the motions of the Sun and planets reflect the disk shape of the solar nebula?
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Massive planets create ____________ Doppler shifts of their stars than lower-mass planets.
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In one sentence, write a scenario involving a meteor, meteorite, and meteoroid.
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Using the graph shown above, find out how many half-lives does it take for all radioactive atoms to decay into daughter products,

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