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A large modern astronomical telescope


A) is designed for high magnifications.
B) uses a single lens.
C) uses a single mirror.
D) uses a number of smaller mirrors.

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

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Neutron stars are about


A) the size of a large house.
B) 20 km in diameter.
C) the size of the moon.
D) the size of Jupiter.

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

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White dwarfs


A) are young stars.
B) are old stars.
C) may be of any age.
D) are extremely rare.

E) C) and D)
F) B) and D)

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A star must have a certain minimum mass in order that gravity squeeze its matter sufficiently to


A) hold it together as a single body.
B) produce a temperature high enough for it to glow.
C) produce a temperature high enough for nuclear reactions to start.
D) turn its interior into liquid hydrogen.

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

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The distance of a star from the earth can be found


A) only if it is part of a double-star system.
B) by comparing its luminosity and brightness.
C) from its color.
D) from its position in the HR diagram.

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

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Streams of protons and electrons from the sun do not affect


A) auroras.
B) the airglow of the night sky.
C) comet heads.
D) comet tails.

E) B) and D)
F) B) and C)

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The sun has


A) no atmosphere.
B) an atmosphere just above its surface only.
C) an atmosphere that extends only as far as the earth.
D) an atmosphere that extends well out into the solar system.

E) A) and D)
F) All of the above

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At the end of its period in the main sequence, a star whose mass is near that of the sun


A) breaks up into several smaller stars.
B) cools down into a white dwarf.
C) expands into a red giant.
D) explodes into a supernova.

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

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Sunspot activity does not affect


A) auroras.
B) the earth's magnetic field.
C) volcanic eruptions.
D) shortwave radio communications.

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

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Auroras consist of


A) colored clouds.
B) comet tails.
C) excited gases in the lower atmosphere.
D) excited gases in the upper atmosphere.

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

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Cepheid variable stars


A) are very bright, easily seen stars.
B) have luminosities related to their periods of variation.
C) have very short periods of variation.
D) all lie in the constellation Cepheus.

E) A) and D)
F) All of the above

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In the HR diagram, most stars are


A) members of the main sequence.
B) red giants.
C) white dwarfs.
D) scattered at random.

E) C) and D)
F) None of the above

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Brown dwarfs


A) are members of the main sequence.
B) are on the way to becoming white dwarfs.
C) do not have enough mass to become true stars.
D) are extremely rare.

E) A) and B)
F) All of the above

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In order to determine the mass of a star, it must be


A) part of the main sequence.
B) part of a binary-star system.
C) be a Cepheid variable.
D) be relatively close.

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

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The sun is a(n)


A) unusually small star.
B) unusually large star.
C) unusually hot star.
D) rather ordinary star.

E) B) and D)
F) B) and C)

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The smallest of the following celestial objects is


A) a white dwarf.
B) a neutron star.
C) a planetary nebula.
D) the earth.

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

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Because the spectra of most stars consist of dark lines on a bright background, these stars must


A) have cool interiors surrounded by hot atmospheres.
B) have hot interiors surrounded by cool atmospheres.
C) have hot interiors surrounded by hot atmospheres.
D) have cool interiors surrounded by cool atmospheres.

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

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The sun will remain its present size and temperature


A) for a few thousand years longer.
B) for a few million years longer.
C) for a few billion years longer.
D) forever.

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

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White dwarf stars are not


A) comparable in size with the earth.
B) comparable in mass with the sun.
C) extremely hot.
D) extremely bright.

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

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The size of a star can be found from its


A) temperature and mass.
B) temperature and brightness.
C) temperature and luminosity.
D) mass and apparent brightness.

E) C) and D)
F) None of the above

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