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The most striking example of solar variability was the


A) Dust Bowl drought of the 1930s.
B) Maunder Minimum from 1645-1715.
C) Sporer Minimum that doomed the Anasazi.
D) fall of Rome.
E) Joseph's seven lean years in the Old Testament.

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On the Sun, what takes approximately 22 years to happen?


A) The Sun takes that time to rotate on its axis.
B) The complete sunspot cycle, including magnetic field reversals.
C) Solar vibrations begin every 22 years.
D) Solar activities goes from its maximum to minimum.
E) The corona reaches its maximum temperature and ejects gas every 22 years.

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In the proton-proton cycle, you must first make deuterium, then helium.

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What do sunspots tell us about the Sun's rotation rate?

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Watching and timing sunspots as they tra...

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When the chromosphere can be seen during a solar eclipse, it appears


A) invisible.
B) violet.
C) blue.
D) yellow.
E) red.

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The luminosity of the Sun is a measure of


A) the energy received by the Sun on Earth's surface.
B) the energy received by the Sun at the location of Earth.
C) the energy received by the Sun at any location in the solar system.
D) the energy emitted by the Sun at the photosphere.
E) the total energy emitted by the Sun in all directions.

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Presently, what is happening to the helium in the sun's core?

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It builds up there, ...

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The energy of the Sun starts as radiation, but is actually transported to its surface by convection, where it is radiated off into space at last.

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Which is the net result of the proton-proton chain?


A) 4 protons = 1 helium 4 + a positron + a neutrino + gamma rays
B) 2 protons = deuterium + a positron + an antineutrino + X-rays
C) 4 protons = 2 heliums 2 + 2 positrons + ultraviolet radiation
D) 4 protons = 1 helium 4 + 2 neutrinos + gamma rays
E) 6 protons = 2 heliums + 3 positrons + 3 neutrinos + gamma rays

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Why is it hard to observe the chromosphere?

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Most of its energy is in the b...

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Studies by the Global Oscillations Network Group, along with satellite observations, indicate


A) that the standard solar model requires substantial modification.
B) that all stars show the same kind of vibrations that our Sun does.
C) that there is an unknown energy transport mechanism in the Sun.
D) that there is less convection in the Sun than predicted by the standard solar model.
E) that the standard solar model accurately models the observed solar vibrations.

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Hydrostatic equilibrium in our Sun is the balance between


A) convection and radiation.
B) convection and gravitation.
C) pressure and radiation.
D) radiation and gravitation.
E) gravitation and pressure.

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  -The above diagram indicates that A)  the Sun is hottest somewhere between its surface and its core. B)  the Sun is coolest somewhere between its surface and its core. C)  the Sun is hotter at its surface than at its core. D)  the Sun is hotter at its core than at its surface. E)  the Sun has about the same temperature throughout its interior. -The above diagram indicates that


A) the Sun is hottest somewhere between its surface and its core.
B) the Sun is coolest somewhere between its surface and its core.
C) the Sun is hotter at its surface than at its core.
D) the Sun is hotter at its core than at its surface.
E) the Sun has about the same temperature throughout its interior.

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How long does the sunspot cycle last, on average?


A) Between 25 and 35 days
B) 365.25 days
C) About seven years
D) About 11 years
E) About 76 years

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Initially, fewer neutrinos were detected than predicted by theoretical models because


A) neutrinos changed form to undetected types of neutrinos.
B) the wrong liquid was being used in neutrino detectors.
C) particle physicists did not understand the proton-proton chain.
D) the proton-proton chain does not actually produce neutrinos.
E) neutrinos take many years to pass out of the sun from its core.

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We know the Sun rotates differentially by observing sunspots; as with Jupiter the solar equator rotates the fastest.

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The solar magnetic field is strongest in those regions called ________, which are poles and usually thus occur in pairs.

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In the proton-proton cycle, the helium atom and neutrino have less mass than the original hydrogen. What happens to the "lost" mass?


A) It is recycled back into hydrogen.
B) It is ejected into space.
C) It is converted to energy.
D) It is transformed into electrons.
E) Conservation of mass dictates no mass can be lost.

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The temperature of the layer of gas that produces the visible light of the Sun is


A) 3,500 K
B) 5,800 K
C) 12,300 K
D) 300,000 K
E) 15 million K

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The ________-year solar cycle is characterized by a variation in the number of sunspots and a reversal of the polarity of the Sun as a whole.

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