Paragraph 1 — What the author does / talks about:The author introduces the relationship between matter, radiation, and gravity in stars. The paragraph explains that thermonuclear fusion provides the pressure needed to prevent stars from collapsing and that the final state of a star depends on its remaining mass after fusion stops.
Short summary: The paragraph explains why fusion is essential for a star’s stability and introduces the idea that a star’s mass determines its final fate.
Paragraph 2 — What the author does / talks about:The author explains the life cycle of a star after it uses up its hydrogen fuel. The paragraph describes how a massive star continues fusing heavier elements until it creates an iron core, and it introduces the three possible final states of a star: white dwarf, neutron star, or black hole.
Short summary: The paragraph describes how stars evolve after hydrogen depletion and identifies their three possible end states.
Paragraph 3 — What the author does / talks about:The author focuses on the future of our Sun and explains that it will become a white dwarf. The paragraph describes how the Sun will lose its outer layers and how electron pressure will eventually stabilize the remaining core.
Short summary: The paragraph explains the process by which a Sun-like star becomes a white dwarf.
Paragraph 4 — What the author does / talks about:The author contrasts white dwarfs with neutron stars and explains that neutron stars form from the violent collapse of much more massive stars. The paragraph describes how a supernova ejects most of the star’s material while leaving behind an extremely dense core.
Short summary: The paragraph explains the formation of neutron stars through massive stellar explosions.
Paragraph 5 — What the author does / talks about:The author explains the final stage of stellar collapse leading to a black hole. The paragraph describes how mass loss through neutrino radiation reduces the pressure supporting the star, allowing gravity to cause complete collapse.
Short summary: The paragraph explains how a collapsing star can become a black hole when gravity overwhelms all remaining pressure.
1. Which of the following is NOT true of all stars?(A) They generated helium as a product of thermonuclear fusion.Wrong:The passage says that in a live star, hydrogen fuses into helium. This describes stars in general, so this is true.
(B) They rely on internally produced pressures to counteract the effects of gravity on their own mass.Wrong:The passage states that thermonuclear fusion provides pressure that supports stars against gravitational contraction. All stars need internal pressure to balance gravity.
(C) They possess cores hot enough to combine nuclei.Wrong:Stars are defined by having hot cores where nuclear fusion can occur, so this is true.
(D) They eventually produce iron cores through thermonuclear burning. Correct: This is
not true of all stars. The passage says that
massive stars continue burning helium and heavier elements until they produce an iron core. A star like the Sun does not become massive enough to create an iron core; it becomes a white dwarf after exhausting its fuel.
(E) Their ultimate form is related to the mass they possess as they begin to die.Wrong:The passage explicitly states that a star’s final fate depends on its remaining mass after fusion can no longer support it.
2. The primary purpose of the passage is to...(A) Present a commonplace idea and its inaccuraciesWrong:The passage does not introduce a common belief and then correct mistakes. It simply explains how stars evolve.
(B) Explore the implications of a findingWrong:The passage does not discuss a specific discovery or research finding and its consequences.
(C) Propose a hypothesis for unexplained observationsWrong:The author does not propose a new theory or attempt to explain something unknown.
(D) Analyze a frequent source of misunderstandingWrong: The passage does not focus on correcting misconceptions about stars.
(E) Describe a process and its outcomesCorrect:The passage describes the
process of stellar evolution: how stars burn fuel, lose stability, collapse, and eventually become white dwarfs, neutron stars, or black holes.
3. Which of the following can most logically be inferred from the passage?(A) Our Sun has fused the majority of the hydrogen contained within it.Correct:The passage states that the Sun will eventually expand and expel its outer matter when it has exhausted its available hydrogen. Since the Sun is currently a live star and will eventually enter this stage, it can be inferred that it has already fused a large portion of its hydrogen.
(B) A supernovae shock precedes the formation of a black hole.Wrong:The passage states that a supernova shock occurs during the formation of a neutron star, not necessarily before every black hole. A black hole forms later if the remaining core collapses further after losing supporting pressure.
(C) Neutrino radiation is caused by ultra-relativistically electrons.Wrong:The passage mentions ultra-relativistic electrons in relation to neutron stars and separately discusses neutrino radiation during collapse. It does not state that electrons cause neutrino radiation.
(D) Fermi pressure is brought about by the gravitational pressure of a collapsing star.Wrong:The passage explains that Fermi pressure from degenerate electrons counters gravitational pressure; it is not caused by gravity.
(E) A white dwarf star is incapable of melting the tails of passing comets.Wrong:The passage does not discuss comets or the ability of white dwarfs to melt comet tails, so this cannot be inferred.