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What is the Sun made of (by mass) ?


A) 70% hydrogen,28% helium,2% other elements
B) 100% hydrogen and helium
C) 50% hydrogen,25% helium,25% other elements
D) 90% dark matter,10% ordinary matter

E) A) and B)
F) None of the above

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Why are neutrinos so difficult to detect?


A) because there are so rare
B) because they have no mass
C) because they move at nearly the speed of light
D) because they rarely interact with matter
E) because they are so small

F) A) and E)
G) B) and C)

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Why does the Sun emit neutrinos?


A) Solar flares create neutrinos with magnetic fields.
B) Fusion in the Sun's core creates neutrinos.
C) Convection releases neutrinos,which random walk through the radiation zone.
D) The Sun was born with a supply of neutrinos that it gradually emits into space.
E) The Sun does not emit neutrinos.

F) B) and C)
G) B) and E)

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How is the sunspot cycle directly relevant to us here on Earth?


A) The sunspot cycle strongly influences Earth's weather.
B) The Sun's magnetic field,which plays a major role in the sunspot cycle,affects compass needles that we use on Earth.
C) The brightening and darkening of the Sun that occurs during the sunspot cycle affects plant photosynthesis here on Earth.
D) Coronal mass ejections and other activity associated with the sunspot cycle can disrupt radio communications and knock out sensitive electronic equipment.
E) The sunspot cycle is the cause of global warming.

F) B) and C)
G) C) and E)

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When is/was gravitational contraction an important energy-generation mechanism for the Sun?


A) only during solar minimum
B) only during solar maximum
C) when the Sun was being formed from a collapsing cloud of gas
D) right after the Sun began fusing hydrogen in its core
E) when the Sun transports radiation through the convection zone

F) None of the above
G) A) and B)

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Why do sunspots appear dark in pictures of the Sun?


A) They are too cold to emit any visible light.
B) They are holes in the solar surface through which we can see through to deeper,darker layers of the Sun.
C) They are extremely hot and emit all their radiation as X-rays rather than visible light.
D) They actually are fairly bright,but appear dark against the even brighter background of the surrounding photosphere.

E) A) and C)
F) A) and B)

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What observations characterize solar maximum?


A) The Sun becomes much brighter.
B) The Sun emits light of longer average wavelength.
C) The Sun rotates faster at the equator.
D) We see many sunspots on the surface of the Sun.
E) all of the above

F) A) and D)
G) None of the above

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Which is closest to the temperature of the core of the Sun?


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

F) B) and C)
G) A) and E)

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What is the solution to the solar neutrino problem?


A) The Sun is generating energy other than by nuclear fusion.
B) The Sun is generating much less energy than we think it is.
C) We do not know how to detect electron neutrinos.
D) Not all fusion reactions create electron neutrinos.
E) The electron neutrinos created in the Sun change into another type of neutrino that we could not detect with our original equipment.

F) B) and E)
G) A) and C)

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The chromosphere is the layer of the Sun that we see as its visible surface.

A) True
B) False

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Although the Sun does not generate energy by gravitational contraction today,this energy-generation mechanism was important when the Sun was forming.

A) True
B) False

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Might changes in the Sun affect weather or climate on Earth?

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During the last Maunder minimum period,t...

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What do we mean when we say that the Sun is in gravitational equilibrium?


A) The hydrogen gas in the Sun is balanced so that it never rises upward or falls downward.
B) The Sun maintains a steady temperature.
C) This is another way of stating that the Sun generates energy by nuclear fusion.
D) There is a balance within the Sun between the outward push of pressure and the inward pull of gravity.
E) The Sun always has the same amount of mass,creating the same gravitational force.

F) A) and B)
G) C) and E)

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Which of the following best explains why nuclear fusion requires bringing nuclei extremely close together?


A) Nuclei normally repel because they are all positively charged and can be made to stick only when brought close enough for the strong force to take hold.
B) Nuclei are attracted to each other by the electromagnetic force,but this force is only strong enough to make nuclei stick when they are very close together.
C) Nuclei have to be very hot in order to fuse,and the only way to get them hot is to bring them close together.
D) Fusion can proceed only by the proton-proton chain,and therefore requires that protons come close enough together to be linked up into a chain.

E) A) and C)
F) C) and D)

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The intricate patterns visible in an X-ray image of the Sun generally show


A) helioseismological fluctuations.
B) a bubbling pattern on the photosphere.
C) extremely hot plasma flowing along magnetic field lines.
D) structure within sunspots.

E) A) and C)
F) A) and B)

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Why must the Sun's rate of fusion gradually rise over billions of years?


A) The Sun becomes less efficient and must increase the rate of fusion to produce the same amount of energy.
B) Fusion reactions decrease the overall number of particles in the core,causing the core to shrink,converting gravitational potential energy into thermal energy,and increasing the rate of fusion.
C) The radiation produced by fusion reactions that is trapped in the core gradually raises the temperature,increasing the rate of fusion.
D) The Sun gets heavier as it gets older,and the stronger inward pull of gravity increases the fusion rate.
E) The rate of fusion is not rising;it is actually decreasing over time.

F) A) and D)
G) B) and C)

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According to modern science,approximately how old is the Sun?


A) 4 12 \frac{1}{2} billion years
B) 25 million years
C) 10,000 years
D) 400 million years

E) A) and C)
F) A) and B)

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Process of Science: How do we know what is going on in the center of the Sun so well if we cannot see it or send spacecraft to it?

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We can apply our knowledge of how gases ...

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Which statement best describes the solar neutrino problem?


A) Theoretical models predict that neutrinos should be produced in the Sun,but no neutrinos have ever been observed to be coming from the Sun.
B) Solar neutrinos were detected but in fewer numbers than predicted by theoretical models.
C) No one understands how it can be possible for neutrinos to be produced in the Sun.
D) Our current understanding of fusion in the Sun suggests that all neutrinos should be destroyed before they arrive at Earth,yet neutrinos are being detected.
E) The term solar neutrino problem refers to the fact that neutrinos are extremely difficult to detect.

F) A) and D)
G) A) and C)

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In the late 1800s,Kelvin and Helmholtz suggested that the Sun stayed hot due to gravitational contraction.What was the major drawback to this idea?


A) It predicted that the Sun would shrink noticeably as we watched it,but the Sun appears to be stable in size.
B) It is physically impossible to generate heat simply by making a star shrink in size.
C) It predicted that the Sun could shine for about 25 million years,but geologists had already found that Earth is much older than this.
D) It predicted that Earth would also shrink in size with time,which would make it impossible to have stable geology on our planet.

E) A) and B)
F) A) and C)

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