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AST 101 - LESSON 10 EXAM QUESTIONS WITH CORRECT ANSWERS LATEST UPDATE 2026

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AST 101 - LESSON 10 EXAM QUESTIONS WITH CORRECT ANSWERS LATEST UPDATE 2026 Shown below here is the track on the H-R diagram of a star like the Sun. At Point A the star is - Answers fusing hydrogen in a shell around a collapsing core. Submit From the same H-R diagram above, at Point B, the star is - Answers fusing helium in its core and hydrogen in a shell. From the same H-R diagram above, at Point C, the star is - Answers has a stable, inert carbon core and essentially no hydrogen or helium. A supernova occurs when - Answers a massive star fuses through successively heavier elements until it has an iron core, which will not release energy from fusion. Consider a young globular star cluster where all the cluster stars formed at about the same time. If you were to observe this star cluster over several billion years, you would see - Answers many supernovae early on, and then no more. Why are red giant stars rare compared to main-sequence stars? - Answers The amount of time a red giant lasts is small compared to the lifespan of a main-sequence star. Why doesn't a high-mass star fuse its iron into heavier elements, like uranium? - Answers No mass-energy is released due to the fusion of iron. In the dying stages of our Sun, it will fuse helium into carbon. After that, what will occur? - Answers The core contracts, but the carbon never fuses. Listed following are characteristics that describe either high-mass or low-mass stars. Match these characteristics to the appropriate category. - Answers High-mass stars: late in-life fuse carbon into heavier elements have higher fusion rate during main sequence life end life as supernova Low-mass stars: the Sun is an example have longer lifetimes final corpse is a white dwarf end life as a planetary nebula Provided following are various stages during the life of a high-mass star. Rank the stages based on when they occur, from first to last. - Answers contracting cloud of gas and dust, protostar, main sequence star, red supergiant, supernova, neutron star Provided following are various elements that can be produced during fusion in the core of a high mass main sequence star. Rank these elements based on when they are produced, from first to last. - Answers helium, carbon, oxygen, iron The diagram indicates that the third most abundant element in the Milky Way Galaxy is _____. - Answers oxygen According to the diagram, the approximate abundance of oxygen atoms in the galaxy is __________. - Answers 1/1000 that of hydrogen According to the diagram, what is the most abundant element with an atomic number greater than or equal to 20? - Answers iron Based on the diagram, which of the following statements best describes the observed pattern of abundances for elements with an atomic number between 6 and 20? - Answers There is a general trend of decreasing abundance with increasing atomic number, but elements with even atomic numbers tend to be more abundant than those with odd atomic numbers. According to current understanding, the two most abundant elements in the universe were made __________. - Answers in the Big Bang In Part D, you saw that elements with even atomic numbers tend to be more abundant than neighboring elements with odd atomic numbers. What nuclear process explains why this is the case? - Answers Starting from carbon (atomic number is 6), the most common nuclear reactions involve the fusion of an additional helium nucleus. The observational data for the element abundances agree quite well with what we expect based on our current understanding of nuclear fusion and stellar evolution. But imagine the data had turned out to be different. Which of the following differences, if it had actually been observed, would have forced us to rethink our entire picture of stellar evolution? - Answers The abundance of elements heavier than uranium turned out to be greater than the abundance of carbon. The following figures show the spectral types of four main-sequence stars. Rank them based on the time each takes, from longest to shortest, to go from a protostar to a main-sequence star during the formation process. - Answers Longest to shortest time: -M6 -G2 -A5 -O9 Provided following are the spectral types of four different main-sequence stars. Rank the stars based on the strength of the radiation pressure that pushes outward as they are forming, from highest pressure to lowest pressure. - Answers Highest to lowest radiation pressure: -O9 -A5 -G2 -M6 Provided following are four different ranges of stellar masses. Rank the stellar mass ranges based on how many stars in each range you would expect to be born in a star cluster, from highest number to lowest number. - Answers Highest to lowest number: -less than 1 solar mass -between 1 and 10 solar masses -between 10 and 30 solar masses -between 30 and 60 solar masses The following figures show various stages during the life of a star with the same mass as the Sun. Rank the stages based on when they occur, from first to last. - Answers contracting cloud of gas and dust, protostar, main sequence star, red supergiant, planetary nebula, white dwarf Each item following is a characteristic of a one-solar-mass star either during its protostar phase or during its main-sequence phase. Match the items to the appropriate phase. - Answers Protostar phase: -energy generated by gravitational contraction -radius much larger than the Sun -pressure and gravity are Not precisely balanced -luminosity much greater than the Sun Main-sequence phase: -energy generated by nuclear fusion -lasts about 10 billion years -surface radiated energy at same rate that core generates energy The Crab Nebula is the result of a ____ that was witnessed on Earth in the year 1054. - Answers supernova Betelgeuse is a supergiant star that will eventually supernova, which means that by mass it is classified as a ____ . - Answers high-mass star The debris from the death of a high-mass star forms a ___ several light years across - Answers supernova remnant A _____ has a density higher than the density of a white dwarf. - Answers neutron star ____ actually occurred about 150,000 years ago in the Large Magellanic Cloud. - Answers Supernova 1987A The ____ is the process by which hydrogen fusion proceeds in high-mass stars. - Answers CNO cycle Carbon can be converted into oxygen in the cores of high-mass stars if carbon nuclei undergo a _____ . - Answers helium capture reaction The following items describe observational characteristics that could indicate that an object is either a white dwarf or a neutron star. Match each characteristic to the correct object. - Answers White Dwarf: •may be surrounded by a planetary nebula

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Institution
AST 101
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AST 101

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AST 101 - LESSON 10 EXAM QUESTIONS WITH CORRECT ANSWERS LATEST UPDATE 2026

Shown below here is the track on the H-R diagram of a star like the Sun. At Point A the star is -
Answers fusing hydrogen in a shell around a collapsing core.
Submit
From the same H-R diagram above, at Point B, the star is - Answers fusing helium in its core and
hydrogen in a shell.
From the same H-R diagram above, at Point C, the star is - Answers has a stable, inert carbon core
and essentially no hydrogen or helium.
A supernova occurs when - Answers a massive star fuses through successively heavier elements until
it has an iron core, which will not release energy from fusion.
Consider a young globular star cluster where all the cluster stars formed at about the same time. If
you were to observe this star cluster over several billion years, you would see - Answers many
supernovae early on, and then no more.
Why are red giant stars rare compared to main-sequence stars? - Answers The amount of time a red
giant lasts is small compared to the lifespan of a main-sequence star.
Why doesn't a high-mass star fuse its iron into heavier elements, like uranium? - Answers No mass-
energy is released due to the fusion of iron.
In the dying stages of our Sun, it will fuse helium into carbon. After that, what will occur? - Answers
The core contracts, but the carbon never fuses.
Listed following are characteristics that describe either high-mass or low-mass stars. Match these
characteristics to the appropriate category. - Answers High-mass stars:
late in-life fuse carbon into heavier elements
have higher fusion rate during main sequence life
end life as supernova

Low-mass stars:
the Sun is an example
have longer lifetimes
final corpse is a white dwarf
end life as a planetary nebula
Provided following are various stages during the life of a high-mass star. Rank the stages based on
when they occur, from first to last. - Answers contracting cloud of gas and dust, protostar, main
sequence star, red supergiant, supernova, neutron star
Provided following are various elements that can be produced during fusion in the core of a high mass
main sequence star. Rank these elements based on when they are produced, from first to last. -
Answers helium, carbon, oxygen, iron
The diagram indicates that the third most abundant element in the Milky Way Galaxy is _____. -
Answers oxygen
According to the diagram, the approximate abundance of oxygen atoms in the galaxy is __________. -
Answers 1/1000 that of hydrogen
According to the diagram, what is the most abundant element with an atomic number greater than or
equal to 20? - Answers iron
Based on the diagram, which of the following statements best describes the observed pattern of
abundances for elements with an atomic number between 6 and 20? - Answers There is a general
trend of decreasing abundance with increasing atomic number, but elements with even atomic
numbers tend to be more abundant than those with odd atomic numbers.
According to current understanding, the two most abundant elements in the universe were made
__________. - Answers in the Big Bang
In Part D, you saw that elements with even atomic numbers tend to be more abundant than
neighboring elements with odd atomic numbers. What nuclear process explains why this is the case? -
Answers Starting from carbon (atomic number is 6), the most common nuclear reactions involve the
fusion of an additional helium nucleus.
The observational data for the element abundances agree quite well with what we expect based on
our current understanding of nuclear fusion and stellar evolution. But imagine the data had turned
out to be different. Which of the following differences, if it had actually been observed, would have

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