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A) It would produce less energy per second than it does now.
B) It would produce more energy per second than it does now.
C) Its energy production would vary more than it does now.
D) Its energy production would be more stable than it is now.
E) The Sun's energy production would not change.
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A) we observe it emitting radiation at visible wavelengths.
B) the chromosphere and the photosphere are that hot, too.
C) we observe absorption from highly ionized atoms of iron and calcium in its spectrum.
D) the gas emits most of its radiation at radio wavelengths.
E) all of the above
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A) is larger than the Moon.
B) is warmer than the Moon.
C) is shielded by the Moon.
D) has a magnetic field while the Moon does not.
E) is farther from the Sun than the Moon is.
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A) one-half as many
B) one-third as many
C) one-fourth as many
D) one-fifth as many
E) We would detect no neutrinos.
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A) They quickly pass through the Sun's outer layers and are emitted into space.
B) They recombine to form electrons.
C) They eventually turn into neutrinos.
D) They are absorbed by other atoms, heating the Sun's core.
E) They are reflected around inside the Sun forever.
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A) coronal holes.
B) coronal mass ejections.
C) differential rotation.
D) temperature changes in the Sun's core.
E) all of these phenomena contribute.
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A) radiation.
B) convection.
C) conduction.
D) convection and conduction.
E) radiation and conduction.
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A) region A
B) region B
C) region C
D) They are all the same temperature.
E) We would also need an X-ray image to determine relative temperatures.
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A) the energy production rate in the core equals the rate of radiation escaping the Sun's surface.
B) the source of energy in the core is stable and will sustain the Sun for millions of years.
C) the outer layers of the Sun absorb and re-emit the radiation from the core at increasingly shorter wavelengths.
D) radiation pressure does not contribute to supporting the weight of the overlying solar layers.
E) the core of the Sun has pressure that is lower than that of the outer layers.
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A) gravitational contraction.
B) nuclear fission of uranium.
C) hydrogen fusion.
D) helium burning.
E) burning material as in a fire.
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Multiple Choice
A) They interact very weakly with other particles.
B) They interact very strongly with other particles.
C) They are the only particles that move quickly.
D) They move very slowly.
E) They can only be found in atomic nuclei.
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Multiple Choice
A) None
B) 2
C) 4
D) 6
E) 12
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