Exam 10: Structure and Formation of Stars
Exam 1: Here and Now49 Questions
Exam 2: Users Guide to the Sky: Patterns and Cycles165 Questions
Exam 3: The Origin of Modern Astronomy79 Questions
Exam 4: Light and Telescopes95 Questions
Exam 5: Sun Light and Sun Atoms135 Questions
Exam 6: The Terrestrial Planets123 Questions
Exam 7: The Outer Solar System88 Questions
Exam 8: Origins of the Solar System and Extrasolar Planets69 Questions
Exam 9: The Family of Stars105 Questions
Exam 10: Structure and Formation of Stars100 Questions
Exam 11: The Deaths of Stars146 Questions
Exam 12: The Milky Way Galaxy70 Questions
Exam 13: Galaxies: Normal and Active135 Questions
Exam 14: Modern Cosmology69 Questions
Exam 15: Life on Other Worlds55 Questions
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The pressure of an interstellar gas cloud depends on the cloud s ____________________ and ____________________.
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While on the main sequence a star s primary energy source comes from
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Star clusters are important to the study the stellar evolution because stars in a given cluster have the same
(Multiple Choice)
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Why are distant stars redder than nearby stars of the same spectral type?
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The sun has a core in which energy travels outward primarily by radiation.
(True/False)
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What must occur for an object to be considered a main sequence star?
(Multiple Choice)
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Emission nebulae are also called ____ because they are composed of ionized hydrogen.
(Multiple Choice)
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Pre-main sequence stars are above and to the right of the main sequence.
(True/False)
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Why are massive stars more luminous than low mass stars? That is, why is there a mass-luminosity relation?
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A(n) ____________________ is a cool, dense cloud of dust and gas that is undergoing gravitational contraction.
(Short Answer)
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High mass stars evolve more slowly to the main sequence than lower mass stars.
(True/False)
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What force(s) are responsible for the collapse of an interstellar cloud?
(Multiple Choice)
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Ninety percent of all stars fuse helium to form carbon and lie on the main sequence.
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