A) A cold, dense gas cloud
B) A hot, dense gas cloud
C) A cold, low-density gas cloud
D) A hot, low-density gas cloud
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Multiple Choice
A) hydrogen.
B) oxygen.
C) carbon.
D) nitrogen.
E) iron.
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Multiple Choice
A) less than 1 billion years.
B) about 1 billion years.
C) about 4.5 billion years.
D) about 10 billion years.
E) more than 15 billion years.
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Multiple Choice
A) Protostar, main-sequence star, red giant, planetary nebula, white dwarf
B) Protostar, main-sequence star, red giant, supernova, neutron star
C) Protostar, main-sequence star, planetary nebula, red giant
D) Main-sequence star, white dwarf, red giant, planetary nebula, protostar
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Multiple Choice
A) low-mass star
B) intermediate-mass star
C) high-mass star
D) brown dwarf
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Multiple Choice
A) red giant, protostar, main-sequence, white dwarf
B) white dwarf, main-sequence, red giant, protostar
C) protostar, red giant, main-sequence, white dwarf
D) protostar, main-sequence, white dwarf, red giant
E) protostar, main-sequence, red giant, white dwarf
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Multiple Choice
A) hotter and brighter.
B) hotter and dimmer.
C) cooler and brighter.
D) cooler and dimmer.
E) the same temperature and brightness.
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Multiple Choice
A) The giant must once have been the more massive star, but is now less massive because it transferred some of its mass to its companion.
B) Although both stars probably formed from the same clump of gas, the more massive one must have had its birth slowed so that it became a main sequence stars millions of years later than its less massive companion.
C) The two stars probably were once separate, but became a binary when a close encounter allowed their mutual gravity to pull them together.
D) The two stars are simply evolving normally and independently, and one has become a giant before the other.
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Multiple Choice
A) Fusion reactions with neutrons
B) Radioactive decay of nuclei with odd numbers of protons
C) Fusion reactions with helium nuclei
D) Fusion reactions with hydrogen nuclei
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Multiple Choice
A) the onset of helium burning after a helium flash in a star with mass comparable to that of the Sun
B) the sudden outpouring of X-rays from a newly formed accretion disk
C) the sudden collapse of an iron core into a compact ball of neutrons
D) the beginning of neon burning in an extremely massive star
E) the expansion of a low-mass star into a red giant
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Multiple Choice
A) its surface temperature and luminosity increase.
B) its surface temperature increases and its luminosity decreases.
C) its surface temperature and luminosity decrease.
D) its surface temperature decreases and its luminosity increases.
E) its surface temperature and luminosity remain the same.
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Multiple Choice
A) thermal pressure
B) degeneracy pressure
C) radiation pressure
D) stellar winds
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Multiple Choice
A) A main-sequence star is hotter and dimmer than it was as a protostar.
B) A main-sequence star is hotter and brighter than it was as a protostar.
C) A main-sequence star is cooler and dimmer than it was as a protostar.
D) A main-sequence star is cooler and brighter than it was as a protostar.
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Multiple Choice
A) At the end of a high-mass star's life, it produces new elements through a series of helium capture reactions.
B) The apparent pattern is thought to be a random coincidence.
C) Elements with atomic mass numbers divisible by 4 tend to be more stable than elements in between.
D) This pattern in elemental abundances was apparently determined during the first few minutes after the Big Bang.
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Multiple Choice
A) viii
B) iv
C) vi
D) iii
E) ii
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Multiple Choice
A) The two stars should be the same age, so we'd expect the subgiant to be more massive than the main-sequence star.
B) The two stars in a binary system should both be at the same stage of life; that is, they should either both be main sequence stars or both be subgiants.
C) It doesn't make sense to find a subgiant in a binary star system.
D) A star with a mass of 3.7 M Sᵤn is too big to be a main sequence star.
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Multiple Choice
A) H fusion by the proton-proton chain
B) H fusion by the CNO cycle
C) helium fusion
D) matter-antimatter annihilation
E) gravitational contraction
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Multiple Choice
A) It is produced during the supernova explosions of high-mass stars.
B) It is produced by mass transfer in close binaries.
C) It is produced during the late stages of fusion in low-mass stars.
D) It was produced during the Big Bang.
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Multiple Choice
A) It doesn't make sense to find a giant in a binary star system.
B) The odds of ever finding two such massive stars in the same binary system are so small as to make it inconceivable.
C) The two stars in a binary system should both be at the same point in stellar evolution; that is, they should either both be main-sequence stars or both be giants.
D) The two stars should be the same age, so the more massive one should have become a giant first.
E) A star with a mass of 15 solar masses is too big to be a main-sequence star.
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Multiple Choice
A) Brown dwarfs eventually collapse to become white dwarfs.
B) Brown dwarfs are supported against gravity by degeneracy pressure, which does not depend on the object's temperature.
C) Brown dwarfs form like ordinary stars but are too small to sustain nuclear fusion in their cores.
D) All brown dwarfs have masses less than about 8% that of our Sun.
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