Exam 11: The Formation and Structure of Stars
Exam 1: Here and Now44 Questions
Exam 2: A Users Guide to the Sky80 Questions
Exam 3: Cycles of the Moon56 Questions
Exam 4: The Origin of Modern Astronomy58 Questions
Exam 5: Gravity61 Questions
Exam 6: Light and Telescopes65 Questions
Exam 7: Atoms and Spectra60 Questions
Exam 8: The Sun68 Questions
Exam 9: The Family of Stars76 Questions
Exam 10: The Interstellar Medium51 Questions
Exam 11: The Formation and Structure of Stars52 Questions
Exam 12: Stellar Evolution56 Questions
Exam 13: The Deaths of Stars59 Questions
Exam 14: Neutron Stars and Black Holes48 Questions
Exam 15: The Milky Way Galaxy54 Questions
Exam 16: Galaxies55 Questions
Exam 17: Active Galaxies and Supermassive Black Holes58 Questions
Exam 18: Modern Cosmology52 Questions
Exam 19: The Origin of the Solar System59 Questions
Exam 20: Earth: the Standard of Comparative Planetology56 Questions
Exam 21: The Moon and Mercury: Comparing Airless Worlds63 Questions
Exam 22: Venus and Mars68 Questions
Exam 23: Jupiter and Saturn62 Questions
Exam 24: Uranus,neptune,and the Kuiper Belt55 Questions
Exam 25: Meteorites,asteroids,and Comets67 Questions
Exam 26: Astrobiology: Life on Other Worlds48 Questions
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High mass stars evolve more slowly to the main sequence than lower mass stars.
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False
A star on the ____________________ generates enough energy from nuclear fusion to halt gravitational collapse.
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main-sequence
The condition of ____________________ means that the force due to gravity pushing down on a layer is exactly equal to the pressure pushing outward on that layer.
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hydrostatic equilibrium
If the sun produces energy by the proton-proton chain,then the center of the sun must have a temperature of at least
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What force(s)are responsible for the collapse of an interstellar cloud?
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Ninety percent of all stars fuse helium and lie on the main sequence.
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Stars with masses greater than 1.1 solar masses use the ____________________ to convert H into He and energy.
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The diagram below is an HR diagram.The line indicates the location of the main sequence.Which of the five labeled locations on the HR diagram indicates a luminosity and temperature similar to that of a T Tauri star? 

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Ionization from the ____ in the Orion Nebula makes it glow.
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Energy transport by ____________________ is important when photons cannot readily travel through a gas.
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____________________ is the resistance of a gas to the flow of radiation.
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Ionization from the ____ in the Orion Nebula makes it glow.
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____ is the thermonuclear fusion of hydrogen to form helium operating in the cores of massive stars on the main sequence.
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What causes the outward pressure that balances the inward pull of gravity in a star?
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The nuclear reactions in a star's core remain under control so long as
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