Deck 8: The Sun
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Deck 8: The Sun
1
The upper chromosphere is hot enough to emit X-rays.
True
2
The visible surface of the Sun is composed of solid matter.
False
3
The layer above the chromosphere is the photosphere.
False
4
The Sun is a ball of hot gas held together by its own gravity.
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5
Helioseismology maps of rotation in the Sun's interior show that its internal gases rotate with equal periods.
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6
Spicules can trigger communications blackouts and auroras on Earth.
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7
Sunspots are parts of active solar regions dominated by magnetic fields that encompass all layers of the Sun's atmosphere.
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8
Nuclear fusion in the Sun is tremendously powerful.
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9
What is the approximate average temperature of the Sun's surface?
A) 5000 o C
B) 5800oC
C) 5800 K
D) 6400 K
E) 10,000oC
A) 5000 o C
B) 5800oC
C) 5800 K
D) 6400 K
E) 10,000oC
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10
Nuclear fusion within the Sun proceeds step by step in a series of reactions called the neutron-neutron chain.
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11
Sunspots tend to occur in groups, or pairs, with the magnetic field around the pair resembling that around a bar magnet.
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12
Granulation is caused by convection currents just below the photosphere.
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13
What are the dark regions that give the Sun's photosphere a mottled appearance?
A) sunspots
B) spicules
C) granules
D) flares
E) CMEs
A) sunspots
B) spicules
C) granules
D) flares
E) CMEs
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14
Almost all the light we receive from the Sun escapes from underneath its photosphere.
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15
Sunspot numbers follow a seven-year cycle.
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16
The corona is so dim that it is not visible in Earth's daytime sky.
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17
Which two elements are most abundant within the Sun?
A) hydrogen and oxygen
B) hydrogen and helium
C) helium and carbon
D) helium and nitrogen
E) hydrogen and carbon
A) hydrogen and oxygen
B) hydrogen and helium
C) helium and carbon
D) helium and nitrogen
E) hydrogen and carbon
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18
Which is the correct order of the Sun's atmospheric layers, from the innermost to outermost?
A) chromosphere → corona → photosphere
B) corona → chromosphere → photosphere
C) chromosphere → photosphere → corona
D) photosphere → chromosphere → corona
E) photosphere → corona → chromosphere
A) chromosphere → corona → photosphere
B) corona → chromosphere → photosphere
C) chromosphere → photosphere → corona
D) photosphere → chromosphere → corona
E) photosphere → corona → chromosphere
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19
What is the average distance between the Sun and Earth?
A) 1 AU
B) 2 AU
C) 5 AU
D) 10 AU
E) 20 AU
A) 1 AU
B) 2 AU
C) 5 AU
D) 10 AU
E) 20 AU
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20
When the Sun generates its own energy, it uses weak forces to bind together atomic nuclei.
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21
Astronomers often record solar images in the ____ part of the electromagnetic spectrum because the gaseous layers high in the Sun's atmosphere are very hot and emit most of their light at short wavelengths.
A) visible light
B) microwave
C) ultraviolet
D) gamma
E) infrared
A) visible light
B) microwave
C) ultraviolet
D) gamma
E) infrared
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22
The corona can reach temperatures of up to ____.
A) 5800 K
B) 10,000 K
C) 500,000 K
D) 1,000,000 K
E) 2,000,000 K
A) 5800 K
B) 10,000 K
C) 500,000 K
D) 1,000,000 K
E) 2,000,000 K
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23
Why does the temperature of the corona rise with latitude?
A) Atoms within the corona become more ionized at higher altitudes.
B) Atoms are forced upward from the chromosphere to the corona.
C) Atoms become neutralized as they dissipate in higher altitudes.
D) Atoms undergo fission when repelled by the corona.
E) Atoms are less excited as they move from the photosphere to the corona.
A) Atoms within the corona become more ionized at higher altitudes.
B) Atoms are forced upward from the chromosphere to the corona.
C) Atoms become neutralized as they dissipate in higher altitudes.
D) Atoms undergo fission when repelled by the corona.
E) Atoms are less excited as they move from the photosphere to the corona.
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24
How many nuclear reactions occur in a proton-proton chain?
A) one
B) two
C) three
D) four
E) five
A) one
B) two
C) three
D) four
E) five
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25
The pink color of the chromosphere is produced by the combined light of three emission lines of hydrogen: ____.
A) blue, green, and yellow
B) red, blue, and violet
C) green, blue, and violet
D) red, magenta, and violet
E) indigo, blue, and red
A) blue, green, and yellow
B) red, blue, and violet
C) green, blue, and violet
D) red, magenta, and violet
E) indigo, blue, and red
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26
Consider the complete magnetic cycle of sunspot activity on the Sun. Approximately how many years is this cycle?
A) 7 years
B) 11 years
C) 22 years
D) 40 years
E) 100 years
A) 7 years
B) 11 years
C) 22 years
D) 40 years
E) 100 years
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27
When mapping the interior of the Sun, astronomers must measure _____ as the photosphere moves up and down.
A) sunspots
B) magnetic fields
C) supergranules
D) limb darkening
E) Doppler shifts
A) sunspots
B) magnetic fields
C) supergranules
D) limb darkening
E) Doppler shifts
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28
What causes granulation on the photosphere?
A) convection
B) solar cycle
C) magnetic fields
D) bursts of energy
E) differential rotation
A) convection
B) solar cycle
C) magnetic fields
D) bursts of energy
E) differential rotation
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29
Galileo proposed that the Sun is a rotating sphere after he ____.
A) timed a full rotation of the Sun's equator
B) observed sunspots move across the surface of the Sun
C) measured different spectral lines of emission on different days
D) noted how the Sun rose in the east and set in the west
E) discovered the parallax of the Sun
A) timed a full rotation of the Sun's equator
B) observed sunspots move across the surface of the Sun
C) measured different spectral lines of emission on different days
D) noted how the Sun rose in the east and set in the west
E) discovered the parallax of the Sun
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30

Which layer of the Sun's atmosphere is represented in the accompanying visual-wavelength image?
A) magnetic carpet
B) chromosphere
C) heliosphere
D) solar wind
E) corona
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31
The Babcock model of the solar magnetic cycle explains the sunspot cycle as primarily a consequence of the Sun's ____.
A) meridional flow
B) convection currents
C) differential rotation
D) coronal mass ejections
E) helioseimologic activity
A) meridional flow
B) convection currents
C) differential rotation
D) coronal mass ejections
E) helioseimologic activity
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32
The _____ occurs when some of the energy in the convective motion of gas is converted into magnetic field energy.
A) Zeeman effect
B) Maunder minimum
C) meridional flow
D) dynamo effect
E) reconnection event
A) Zeeman effect
B) Maunder minimum
C) meridional flow
D) dynamo effect
E) reconnection event
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33
What methodology do astronomers use to map the inside of the Sun?
A) heliogeology
B) chromography
C) coronagraphy
D) helioseismology
E) magnetic field mapping
A) heliogeology
B) chromography
C) coronagraphy
D) helioseismology
E) magnetic field mapping
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34
What occurs on the surface of the Sun during a solar cycle minimum?
A) reversal in rotation of the Sun
B) little to no sunspot activity
C) decreased temperature of the photosphere
D) partial dissipation of the corona
E) little to no solar wind
A) reversal in rotation of the Sun
B) little to no sunspot activity
C) decreased temperature of the photosphere
D) partial dissipation of the corona
E) little to no solar wind
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35

What process on the Sun's photosphere does this figure represent?
A) solar cycle
B) sunspot cycle
C) convection currents
D) magnetic field shifts
E) differential rotation
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36
Granulation is evidence that energy in the photosphere ____.
A) is flowing downward towards the core
B) stays horizontal on the surface
C) is spiraling westward
D) is spiraling eastward
E) is flowing upward
A) is flowing downward towards the core
B) stays horizontal on the surface
C) is spiraling westward
D) is spiraling eastward
E) is flowing upward
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37
When two arches in a magnetic field encounter each other, ____ can cause powerful eruptions called ____.
A) reconnection events; flares
B) supergranules; Coulumb barriers
C) filaments; coronal holes
D) solar winds; convective zones
E) prominences; limb darkening
A) reconnection events; flares
B) supergranules; Coulumb barriers
C) filaments; coronal holes
D) solar winds; convective zones
E) prominences; limb darkening
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38
Of the following parts of the Sun, which is the hottest?
A) sunspots
B) corona
C) photosphere
D) supergranules
E) chromosphere
A) sunspots
B) corona
C) photosphere
D) supergranules
E) chromosphere
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39
Astronomers can measure the magnetic fields of sunspots using the ____, which splits spectral lines into multiple components.
A) Zeeman effect
B) Maunder effect
C) Babcock effect
D) Galileo effect
E) Payne effect
A) Zeeman effect
B) Maunder effect
C) Babcock effect
D) Galileo effect
E) Payne effect
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40
Astronomers refer to the dark center of a sunspot as a(n) ____
A) eye
B) flare
C) umbra
D) spicule
E) penumbra
A) eye
B) flare
C) umbra
D) spicule
E) penumbra
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41
Match between columns
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42
Which equation represents the overall nuclear fusion process of the Sun?
A) "4 4 H => 4 He - energy"
B) "2 1 H => 1 He + energy"
C) "4 1 H => 2 1 He - energy"
D) "4 1 H => 4 He + energy"
E) " 4 H => 8 He + energy"
A) "4 4 H => 4 He - energy"
B) "2 1 H => 1 He + energy"
C) "4 1 H => 2 1 He - energy"
D) "4 1 H => 4 He + energy"
E) " 4 H => 8 He + energy"
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43
Match between columns
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44
Why was the Davis experiment only able to detect one-third of the neutrinos originally predicted?
A) Most of the neutrinos were absorbed by Earth's atmosphere.
B) The neutrinos combined with other particles as they entered Earth's atmosphere.
C) The neutrinos distributed evenly among three different flavors while traveling to Earth.
D) The number of neutrinos was too great to be held in the tank that Davis designed.
E) The other two-thirds of neutrinos dissipated while traveling to Earth.
A) Most of the neutrinos were absorbed by Earth's atmosphere.
B) The neutrinos combined with other particles as they entered Earth's atmosphere.
C) The neutrinos distributed evenly among three different flavors while traveling to Earth.
D) The number of neutrinos was too great to be held in the tank that Davis designed.
E) The other two-thirds of neutrinos dissipated while traveling to Earth.
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45
During the first reaction of the proton-proton chain of nuclear fusion, a weak force causes one of the protons to transform into a neutron and emit ____.
A) a positron and a neutrino
B) a positron and a deuterium
C) a neutrino and a deuterium
D) a neutrino and an electron
E) a deuterium and an electron
A) a positron and a neutrino
B) a positron and a deuterium
C) a neutrino and a deuterium
D) a neutrino and an electron
E) a deuterium and an electron
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46
Match between columns
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47
Which of the natural forces bind atomic nuclei?
A) strong force
B) weak force
C) gravitational force
D) Newtonian force
E) electromagnetic force
A) strong force
B) weak force
C) gravitational force
D) Newtonian force
E) electromagnetic force
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48
The Maunder minimum occurred in the 17th century, which many scientists debate the labeling of that time as the "Little Ice Age". However, it occurred before the Industrial Revolution and thus, had no significant impact on the human standard of living as we know in today's society. Suppose the Sun experienced a similar period today. How would life on Earth be impacted?
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49
The images produced by _______________ reveal streamers in the corona that follow magnetic lines of force in the Sun's magnetic field.
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50
What occurs during nuclear fusion within the Sun and how much energy is produced?
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51
The number of _______________ visible on the Sun varies in a cycle with a period of 11 years.
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52
Why do sunspots occur darker than the rest of the Sun's surface?
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53
During nuclear fusion, four hydrogen nuclei fuse into how many helium?
A) one
B) two
C) three
D) four
E) eight
A) one
B) two
C) three
D) four
E) eight
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54
The _______________ is a thin layer of gas from which Earth receives most of the Sun's light.
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55
The solar wind extends to the _______________ , marking an outer boundary of the Solar System.
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56
What is released from the proton-proton chain and is immediately absorbed by the surrounding gas, thereby heating it?
A) positrons
B) deuterium
C) gamma rays
D) neutrinos
E) electron motion
A) positrons
B) deuterium
C) gamma rays
D) neutrinos
E) electron motion
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57
The most abundant gas making up the Sun's composition is _______________.
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58
In order for nuclear fusion to occur, atomic nuclei must overcome the ____ by colliding violently.
A) coronal hole
B) dynamo effect
C) convective zone
D) radiative zone
E) Coulomb barrier
A) coronal hole
B) dynamo effect
C) convective zone
D) radiative zone
E) Coulomb barrier
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59
What is the safest way to view the Sun and its sunspots?
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60
Stars, like our Sun, generate their energy by way of nuclear _______________.
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61
Explain the role of convection on the Sun's surface.
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62
What causes auroras and where are they most prominent on Earth?
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63
What forms of electromagnetic radiation from the Sun's emissions do we experience here on Earth? Illustrate how we know this to be the case with one practical example for each form.
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64
The _______________ of the solar disk is dimmer than the center, which is caused by the absorption of light in the photosphere.
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65
Gas flows away from the Sun in the _______________, which can be considered an extension of the corona.
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66
The magnetic polarities of sunspots _______________ at the end of an 11-year cycle.
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67
Explain the Babcock model and why the solar cycle should really be considered as a 22-year cycle instead of 11-year cycle.
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68
The _______________ predicts that pairs of sunspots should occur where magnetic tubes burst through the Sun's surface.
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69
Historical records show that there were very few sunspots from about 1645 to 1715, a phenomenon known as the _______________.
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70
The chromosphere is roughly _______________ times fainter than the photosphere.
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71
What are the only four forces that can affect matter?
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72
How is the Sun's rotation different than that of Earth's?
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