Exam 11: The Sun: Our Extraordinary Star
Exam 1: Discovering the Night Sky374 Questions
Exam 2: Gravitation and the Motion of the Planets356 Questions
Exam 3: Light and Telescopes275 Questions
Exam 4: Atomic Physics and Spectra223 Questions
Exam 5: Exoplanets and the Formation of Planetary Systems98 Questions
Exam 6: Formation of the Solar System121 Questions
Exam 7: Earth and the Moon305 Questions
Exam 8: The Other Terrestrial Planets265 Questions
Exam 9: The Outer Planets360 Questions
Exam 10: Vagabonds of the Solar System198 Questions
Exam 11: The Sun: Our Extraordinary Star248 Questions
Exam 12: Characterizing Stars254 Questions
Exam 13: The Lives of Stars From Birth Through Middle Age325 Questions
Exam 14: The Death of Stars235 Questions
Exam 15: Black Holes: Matters of Gravity178 Questions
Exam 16: The Milky Way Galaxy157 Questions
Exam 17: Galaxies207 Questions
Exam 18: Quasars and Other Active Galaxies118 Questions
Exam 19: Cosmology217 Questions
Exam 20: Astrobiology71 Questions
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A hydrogen nucleus (a proton) has a charge of +1, and a helium nucleus has a charge of +2. Why, then, does it require four protons to form helium in the core of the Sun?
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B
The surface of the Sun near its edge appears dimmer and cooler than at the center of the disk when viewed in visible light because one sees
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D
The year 2013 marked a sunspot maximum. What does this mean?
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C
The total light emitted by the solar corona, which is seen MOST effectively during a total solar eclipse, is equivalent in brightness to
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How many joules of energy would be released if a U.S. penny (2.5 *10-3 kg) were converted entirely to energy? The speed of light is 3 *108 m/s.
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Convection currents in the Sun's interior occupy what fraction of the Sun's radius?
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The approximate temperature of the visible surface of the Sun is
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What are the MOST energetic eruptive events to occur on the Sun?
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The thickness of the photosphere, or the visible "surface" of the Sun, is
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The dominant energy source that powers the Sun at the present time is
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In the 1920s, Arthur Eddington made a proposal that proved vital to showing how stars generate energy. This was that
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The granulation observed on the photosphere of the Sun appears to be the result of
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Apart from the helium nuclei and energy that are produced in proton-proton reactions in the Sun's core, what are the other by-products?
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The temperature of the Sun throughout its radius and including its atmosphere
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