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All stars that become supernovae will leave behind a neutron star.

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What happens when a main- sequence star exhausts its core hydrogen fuel supply?


A) The star becomes a neutron star.
B) The core shrinks while the rest of the star expands.
C) The entire star shrinks in size.
D) The core immediately begins to fuse its helium into carbon.

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Which of the following types of data provide evidence that helps us understand the life tracks of low- mass stars?


A) spacecraft observations of the Sun
B) H- R diagrams of open clusters
C) observing a low- mass star over many years
D) H- R diagrams of globular clusters

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What kind of gas cloud is most likely to give birth to stars?


A) a cold, low- density gas cloud
B) a cold, dense gas cloud
C) a hot, low- density gas cloud
D) a hot, dense gas cloud

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The main source of energy for a star as it grows in size to become a red giant is _ _.


A) hydrogen fusion in a shell surrounding the central core
B) hydrogen fusion in the central core
C) gravitational contraction
D) helium fusion in the central core

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Which two energy sources can help a star maintain its internal thermal pressure?


A) nuclear fusion and gravitational contraction
B) nuclear fusion and chemical reactions
C) nuclear fission and gravitational contraction
D) nuclear fusion and nuclear fission
E) chemical reactions and gravitational contraction

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What does the CNO cycle and the hydrogen proton- proton cycle have in common? Choose the best answer to the question.


A) They both are ways to fuse hydrogen nuclei to make helium.
B) They both trigger at the same temperature.
C) They are both nuclear reactions; the CNO cycle makes carbon, nitrogen, and oxygen, and the proton cycle makes helium.
D) They are both cycles in star lives.

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Where would a brown dwarf be located on an H- R diagram?


A) in the lower left corner of the H- R diagram
B) below and to the right of the lowest part of the main sequence
C) above and to the left of the highest part of the main sequence
D) in the upper right corner of the H- R diagram

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Stars with high masses live longer than stars with lower masses.

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After a supernova event occurring in a high- mass star, what is left behind?


A) always a black hole
B) always a neutron star
C) always a white dwarf
D) either a white dwarf or a neutron star
E) either a neutron star or a black hole

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Which element has the lowest mass per nuclear particle and therefore cannot release energy by either fusion or fission?


A) oxygen
B) iron
C) silicon
D) hydrogen

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The figure above shows the abundance of elements in the galaxy relative to hydrogen. Why does iron have a higher abundance than nearby elements?


A) It has a higher density than other elements, and thus becomes locked away in dust.
B) It is the end product of core fusion in massive stars, and can only be destroyed in rare supernova fusion reactions.
C) It does not; this apparent higher abundance is due to iron's many spectral lines making it easier to find.

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Photographs of many young stars show long jets of material apparently being ejected from their poles.

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Which process is required to allow a gravitationally- collapsing gas cloud to continue to collapse?


A) The cloud must collide with other clouds.
B) The cloud must radiate much of its thermal energy.
C) The cloud must trap most of its thermal energy.
D) New dust particles must continually be made in the cloud.

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Stars spend about 90% of their lifetime on the main sequence.

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At approximately what temperature can helium fusion occur?


A) 100,000 K
B) 100 billion K
C) 1 million K
D) 100 million K
E) 10 million K

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The helium fusion process works by fusing two helium nuclei into one beryllium nucleus.

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This diagram represents the life track of a 1 solar mass star. Refer to the life stages labeled with roman numerals. During which stage does the star have an inert (non- burning) helium core?


A) iii
B) vi
C) viii
D) iv
E) vii

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The most massive stars generate energy at the end of their lives by fusing iron in their cores.

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Most interstellar clouds remain stable in size because the force of gravity is opposed by within the cloud.


A) thermal pressure
B) stellar winds
C) radiation pressure
D) degeneracy pressure

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