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Multiple Choice
A) our solar system.
B) our Sun.
C) Jupiter.
D) Earth.
E) a white dwarf.
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Multiple Choice
A) 1,000 Suns.
B) 50,000 Suns.
C) a million Suns.
D) a billion Suns.
E) a trillion Suns.
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True/False
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Essay
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Multiple Choice
A) the heavier the element, the less time it takes to make it.
B) the heavier the element, the higher the temperature to fuse it.
C) helium to carbon fusion takes at least 100 million K to start.
D) photodisintegration of iron nuclei begins at 10 billion K to ignite the supernova.
E) All of the above are correct.
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Multiple Choice
A) the upper mass limit for a white dwarf.
B) the temperature at which hydrogen fusion starts.
C) the temperature at which helium fusion starts.
D) the point at which a planetary nebula forms.
E) the lower mass limit for a Type II supernova.
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Multiple Choice
A) iron is the heaviest element, and sinks upon differentiation.
B) iron has poor nuclear binding energy.
C) iron cannot fuse with other nuclei to produce energy.
D) iron supplies too much pressure.
E) iron is in the form of a gas, not a solid, in the center of a star.
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Multiple Choice
A) astrometric binary.
B) detached binary.
C) spectroscopic binary.
D) mass-transfer binary.
E) eclipsing binary.
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True/False
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Essay
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Multiple Choice
A) Neutrinos travel faster than photons.
B) Neutrinos are easier to detect than photons.
C) Neutrinos are produced in the explosion before photons.
D) Neutrinos are emitted from the outer part of the star; photons come from the core.
E) Neutrinos escape from the star quickly because they hardly interact with matter; photons aredelayed by interactions with matter.
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True/False
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Multiple Choice
A) 1572 AD by Tycho Brahe.
B) 1604 AD by Johannes Kepler.
C) 1054 AD by Chinese and Middle Eastern astronomers.
D) 1006 by observers in the southern hemisphere.
E) about 9,000 BC by all our ancestors.
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True/False
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