Exam 10: The Interstellar Medium
Exam 1: Here and Now50 Questions
Exam 2: A Users Guide to the Sky68 Questions
Exam 3: Moon Phases and Eclipses68 Questions
Exam 4: Origins of Modern Astronomy64 Questions
Exam 5: Gravity76 Questions
Exam 6: Light and Telescopes69 Questions
Exam 7: Atoms and Spectra73 Questions
Exam 8: The Sun70 Questions
Exam 9: The Family of Stars70 Questions
Exam 10: The Interstellar Medium51 Questions
Exam 11: Formation and Structure of Stars44 Questions
Exam 12: Stellar Evolution51 Questions
Exam 13: Deaths of Stars74 Questions
Exam 14: Neutron Stars and Black Holes69 Questions
Exam 15: The Milky Way Galaxy72 Questions
Exam 16: Galaxies75 Questions
Exam 17: Supermassive Black Holes and Active Galaxies68 Questions
Exam 18: Modern Cosmology71 Questions
Exam 19: Origin of the Solar System and Extrasolar Planets69 Questions
Exam 20: Earth the Active Planet71 Questions
Exam 21: The Moon and Mercury70 Questions
Exam 22: Venus and Mars67 Questions
Exam 23: Jupiter and Saturn68 Questions
Exam 24: Uranus Neptune Pluto and the Kuiper Belt68 Questions
Exam 25: Meteorites Asteroids and Comets65 Questions
Exam 26: Astrobiology68 Questions
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Because blue light has a shorter wavelength than red light, it will be more readily scattered.
(True/False)
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The type of radiation that is emitted when the electron in a hydrogen atom experiences a spin flip is a (n) _______________.
(Short Answer)
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The emission lines from O III are called ____ because they are not visible laboratories on Earth due to the much greater pressure of the gas on Earth.
(Multiple Choice)
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Interstellar extinction and the reddening of light by the interstellar medium (ISM) are both caused by _____.
(Multiple Choice)
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Describe three ways in which astronomers can distinguish between interstellar absorption lines and stellar absorption lines.
(Essay)
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What observations indicate the presence of dust in the interstellar medium?
(Essay)
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Stars are born from the interstellar medium, and aging or dying stars return gas and dust back into the interstellar medium.
(True/False)
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Large molecular clouds will form into protostars because of ____.
(Multiple Choice)
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_______________ require that a young hot star (T ≥ 25,000 K) be relatively nearby.
(Short Answer)
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Molecular clouds are mapped using _____ gas instead of the most-abundant hydrogen because itradiates at radio wavelengths more efficiently.
(Multiple Choice)
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Which type of nebula is produced when a star, hotter than 25,000 K, excites the gas near it to produce an emission spectrum producing a distinctive pink color?
(Multiple Choice)
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Calculations of the Sun's future evolution indicate that it will blow away almost half of its mass in several relatively short episodes about 4 to 5 billion years from now before it is finally extinguished.
(True/False)
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Elements such as carbon, silicon and oxygen have been produced in stars and expelled as stars age in the interstellar medium. This is most likely due to these elements having cooled and condensed from aging stars to form dust grains, and carried out by a powerful winds.
(True/False)
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