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During its existence in the Sun's interior, a particular photon experiences


A) only one collision.
B) thousands of collisions.
C) millions of collisions.
D) collisions numbering more than millions.

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The Stefan-Boltzmann law indicates that the energy emitted per second per area of an emitting surface varies with the fourth power of the Kelvin temperature. Suppose the center of a granule on the Sun's photosphere is 6000 K and the edges of the cell are 100 K cooler. About how much energy is emitted each second from each unit area on the edge compared with that from the center?


A) 10-8
B) 50%
C) 93%
D) 127%

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By how much does the mass of the Sun decrease each second because of the energy radiated from it (its luminosity) ?


A) 6.0 * 1011 kg
B) 2.0 * 107 kg
C) 3.9 *1026 kg
D) 4.3 * 109 kg

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The core of the Sun, in which the Sun's thermonuclear energy is produced, takes up about


A) 1/2 the Sun's radius.
B) 1/4 of the Sun's radius.
C) less than 1/100 of the Sun's radius.
D) 1/10 of the Sun's radius.

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Which of these is NOT considered to be a feature of the quiet Sun?


A) solar wind
B) sunspot
C) spicule
D) granule

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What change in spectral lines emitted by atoms is described by the Zeeman effect?


A) broadening of the lines associated with the high temperature of the emitting gas
B) change in relative intensity of different lines from sources of different temperature
C) shift in the lines because of the movement of the source
D) splitting of lines because the atoms are within an intense magnetic field

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Sunspots are regions where the Sun's magnetic field penetrates the photosphere. What holds each spot together?


A) the mutual attraction of the magnetic field lines
B) the attraction of the magnetic field lines for the plasma inside the sunspot
C) rapid circulation of plasma around the field region
D) gravitational attraction within the colder, more condensed gases within the spot

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Spicules on the solar surface are


A) jets of gas surging out of the photosphere of the Sun into the chromosphere, usually at supergranule boundaries.
B) intense eruptions from sunspot groups and active regions, associated with solar flares.
C) streams of solar coronal material, usually seen only during a total solar eclipse.
D) curtainlike structures hanging over sunspot regions.

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Where is the chromosphere on the Sun?


A) The chromosphere is the outermost part of the Sun's atmosphere.
B) The chromosphere is the layer below the visible surface of the Sun, where convection begins.
C) The chromosphere is the visible surface of the Sun.
D) The chromosphere is the layer above the visible surface of the Sun.

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Where is the coolest region in the Sun?


A) just below the photosphere, in the convective zone
B) in the lower corona
C) in the lower photosphere
D) in the lower chromosphere

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The sunspot cycle on the Sun is a(n)


A) regular movement of a relatively constant number of sunspots from the poles to the equator of the Sun over an 11-year period.
B) somewhat irregular cycle of buildup and decay of sunspot numbers, averaging about 11 years and with a variable number of sunspots for each cycle.
C) extremely regular buildup and decay in the number of sunspots, with a precise period of 11 years but with widely varying numbers of sunspots
D) Extremely regular buildup and decay in the number of sunspots, with a precise period of 11 years with every cycle having the same number of sunspots at maximum.

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The Sun has nearly the same temperature today that it had 4.5 billion years ago, but it is now 30% more luminous. Why?


A) The Sun has a stronger magnetic field today.
B) The Sun has a larger surface area today.
C) The Sun has more sunspots today.
D) Energy took longer to escape the young Sun.

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Mean temperatures in Europe during the Maunder minimum, when virtually no sunspots were seen between 1645 and 1715, were


A) more strongly fluctuating above and below the average temperature compared with the period from 1715 to the present.
B) unchanged, within statistical uncertainty.
C) higher than average.
D) lower than average.

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The Stefan-Boltzmann law indicates that the energy emitted per second per area of an emitting surface varies with the fourth power of the Kelvin temperature. Suppose the center of a sunspot on the Sun's photosphere is 4000 K and the normal photosphere is about 6000 K. About how much energy is emitted each second from each unit area in the center of this sunspot compared with that from the normal photosphere?


A) 10-8
B) 0.20
C) 0.67
D) 0.98

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What is the threshold temperature for the fusion of hydrogen to helium to occur?


A) 19,000 K
B) 153,000 K
C) 107 K
D) 1.55 * 107 K

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What is the name of a sudden, highly energetic, eruptive surge on the surface of the Sun?


A) prominence
B) sunspot
C) plage
D) flare

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How much hydrogen is converted to helium each second in the Sun?


A) 6 billion tons
B) 600 tons
C) 6 tons
D) 600 million tons

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The two most important processes by which energy is transported from the core of the Sun to the photosphere are


A) conduction and convection.
B) radiation and convection.
C) radiation and conduction.
D) radiation and neutrino emission.

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Which of these astronomers was the first to detect the rotation of the Sun by watching sunspot motions?


A) Halley, while watching his comet
B) Copernicus
C) Galileo
D) Ptolemy

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How does the average density of the Sun compare with that of the planet Jupiter?


A) It is not possible to specify an average density for an object as large as the Sun.
B) The Sun is many times denser than Jupiter.
C) The Sun is considerably less dense than Jupiter.
D) The Sun has approximately the same average density as Jupiter.

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