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Astronomy 1010 Final Exam Study Guide 2025

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Which two energy sources can help a star maintain its internal thermal pressure? -Correct Answer Nuclear fusion and gravitational contraction What is the source of luminosity for protostars that have not yet become hot enough for fusion in their cores? -Correct Answer Gravitational energy released by infalling matter What can we learn about a star from its life track on an H-R diagram? -Correct Answer What surface temperature and luminosity it will have at each stage of life Which of the following statements about degeneracy pressure is not true? -Correct Answer Degeneracy pressure varies with the temperature of the star What percentage of a star's total lifetime is spent on the main sequence? -Correct Answer 90% What happens when a star like the sun exhausts its core hydrogen supply? -Correct Answer Its core contracts, but its outer layers expand and the star becomes bigger and brighter Helium fusion directly results in the formation of -Correct Answer Carbon What happens after the helium flash in the core of a star? -Correct Answer The core quickly heats up and expands as helium fusion begins all at once throughout the core Which of the following sequences correctly describes the stages of life for a one solar mass star? -Correct Answer Protostar, main-sequence, red giant, white dwarf What is the CNO cycle? -Correct Answer a type of hydrogen fusion that uses carbon, nitrogen, and oxygen nuclei as catalysts Why does stellar main-sequence lifetime decrease with increasing stellar mass? -Correct Answer Higher core temperatures cause fusion to proceed much more rapidly Which element has the lowest mass per nuclear particle and therefore cannot release energy by either fusion or fission? -Correct Answer Iron What happens when the gravity of a massive star's collapsing core is able to overcome neutron degeneracy pressure? -Correct Answer The core contracts and becomes a black hole

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Astronomy 1010 Final Exam Study
Guide 2025
Which two energy sources can help a star maintain its internal thermal pressure? -
Correct Answer ✔Nuclear fusion and gravitational contraction

What is the source of luminosity for protostars that have not yet become hot enough for
fusion in their cores? -Correct Answer ✔Gravitational energy released by infalling matter

What can we learn about a star from its life track on an H-R diagram? -Correct Answer
✔What surface temperature and luminosity it will have at each stage of life

Which of the following statements about degeneracy pressure is not true? -Correct
Answer ✔Degeneracy pressure varies with the temperature of the star

What percentage of a star's total lifetime is spent on the main sequence? -Correct
Answer ✔90%

What happens when a star like the sun exhausts its core hydrogen supply? -Correct
Answer ✔Its core contracts, but its outer layers expand and the star becomes bigger
and brighter

Helium fusion directly results in the formation of -Correct Answer ✔Carbon

What happens after the helium flash in the core of a star? -Correct Answer ✔The core
quickly heats up and expands as helium fusion begins all at once throughout the core

Which of the following sequences correctly describes the stages of life for a one solar
mass star? -Correct Answer ✔Protostar, main-sequence, red giant, white dwarf

What is the CNO cycle? -Correct Answer ✔a type of hydrogen fusion that uses carbon,
nitrogen, and oxygen nuclei as catalysts

Why does stellar main-sequence lifetime decrease with increasing stellar mass? -
Correct Answer ✔Higher core temperatures cause fusion to proceed much more rapidly

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

What happens when the gravity of a massive star's collapsing core is able to overcome
neutron degeneracy pressure? -Correct Answer ✔The core contracts and becomes a
black hole



Astronomy 1010

, Astronomy 1010



Which of the following statements about the stages of nuclear burning in a massive star
is not true? -Correct Answer ✔Each successive stage lasts for approximately as long as
the first, hydrogen fusion stage.

Which event marks the beginning of a supernova? -Correct Answer ✔The sudden
collapse of an iron core into a compact ball of neutrons

You discover a binary star system in which one member is a 15 solar mass main-
sequence star and the other star is a 10 solar mass giant star. Why should you be
surprised, at least at first? -Correct Answer ✔The two stars should be the same age, so
the more massive one should have become a giant first

Consider a large molecular cloud that will give birth to a cluster of stars. Which of the
following would you expect to be true? -Correct Answer ✔A few massive stars will form,
live, and die before the majority of the star's clusters even complete their protostar
stage.

This diagram represents the life track of a 1 solar mass star. Refer to the life stages
labeled with roman numerals. Which stage lasts the longest? -Correct Answer ✔Main
sequence line

Carbon fusion occurs in high-mass stars but not in low-mass stars because... -Correct
Answer ✔The cores of low-mass stars never get hot enough for carbon fusion

A spinning neutron star has been observed at the center of a -Correct Answer
✔Supernova remnant

Degeneracy pressure stops the crush of gravity in all the following except -Correct
Answer ✔A very massive main-sequence star

Suppose a white dwarf is gaining mass because of accretion from a binary companion.
What happens if its mass reaches the 1.4 solar mass limit? -Correct Answer
✔Temperatures skyrocket to the point where carbon fusion is possible, which leads to a
white dwarf supernova explosion

Which of the following statements about novae is not true? -Correct Answer ✔Our Sun
will probably undergo at least one nova when it becomes a white dwarf about 5 billion
years from now

What kind of star is most likely to become a white-dwarf supernova? -Correct Answer
✔A white dwarf star with a red giant binary companion

From an observational standpoint, what is a pulsar? -Correct Answer ✔An object that
emits flashes of light several times per second, with near perfect regularity


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