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What is the relationship between a giant molecular cloud and an H II region?


A) They are two names for the same entity.
B) In giant molecular clouds, H II regions surround ultraviolet-emitting stars (types O andB) , which have ionized the hydrogen around them.
C) In H II regions, giant molecular clouds are concentrations of other molecules like CO and H2O.
D) Giant molecular clouds evolve into H II regions as the molecules other than hydrogen are used up in star formation.

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

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After hydrogen burning ends in a star's core, its position on the Hertzsprung-Russell diagram moves toward the


A) lower right.
B) upper left.
C) lower left.
D) upper right.

E) None of the above
F) All of the above

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During helium burning in a star's later life, the chemical element produced by the combination of helium nuclei is


A) the light isotope of helium, 3He.
B) heavy hydrogen, 2H.
C) beryllium, 8Be.
D) carbon, 12C.

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

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What happens to the helium-rich core of a star after the core runs out of hydrogen?


A) The core cools down and contracts.
B) The core expands and cools down.
C) The core heats up and expands.
D) The core contracts and heats up.

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

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On the Hertzsprung-Russell diagram, in which direction does the position occupied by a star move after helium burning begins in the star's core?


A) toward the upper right
B) toward the lower left
C) toward the lower right
D) toward the upper left

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

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Where are protostars MOST likely to form?


A) emission nebulae
B) reflection nebulae
C) dark nebulae
D) planetary nebulae

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

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The Jeans instability describes the


A) explosion of a star at the end of its life, the supernova phenomenon.
B) overcoming of gas pressure by self-gravity in a cold and dense interstellar cloud, to form a star.
C) conditions under which sufficient numbers of neutrinos can trigger the collapse of an interstellar cloud.
D) expansion of a gas cloud after gravitational contraction because of buildup of great heat within the cloud from gravitational potential energy.

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

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How large was the Sun when it first formed as a protostar?


A) about 5 times its present diameter
B) about 15 times its present diameter
C) about 50 times its present diameter
D) same diameter it has now

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

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The components of a binary star, particularly if they are close, can influence each other in various ways. Which of these is NOT a likely effect of one star on its companion?


A) One star can be enshrouded in an accretion disk.
B) The gravitational force of one star will make its companion move in an orbit rather than remaining stationary.
C) Intense radiation from a hot star can produce nuclear reactions on the surface of a cooler companion and initiate a nova explosion.
D) Mass can be transferred from one star to its companion.

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

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How long will the Sun have spent as a main-sequence star when it finally begins to evolve toward the red giant phase?


A) 1 billion years
B) 1 million years
C) 1011 years
D) 1010 years

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

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Approximately what fraction of its main-sequence lifetime has the Sun completed at the present time?


A) about 1/4
B) less than 10 percent
C) about 1/2
D) about 3/4

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

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A protostar of about 1 solar mass is gradually contracting and becoming hotter. This activity causes its position in the Hertzsprung-Russell diagram to shift slowly


A) upward and toward the right.
B) downward and toward the left.
C) upward and toward the left.
D) downward and toward the right.

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

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Nuclear fusion reactions that convert helium into carbon and oxygen in the central core of a star occur during which phase of a star's life?


A) in the red giant stage, before the helium flash
B) during and immediately after the (first) red giant or supergiant stage
C) during the protostar stage
D) after the main-sequence phase, before the star becomes a red giant

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

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Most interstellar matter is too cold to be observed optically. In which part of the electromagnetic spectrum might its radiation be detected?


A) gamma ray
B) ultraviolet
C) infrared
D) X-ray

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

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The source of MOST of a protostar's heat is


A) gravitational energy released as the protostar expands.
B) nuclear reactions in its core converting helium to carbon and oxygen.
C) gravitational energy released as the star contracts.
D) nuclear reactions in its core converting hydrogen into helium.

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

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Giant molecular clouds, which are major sites of star formation, can be up to about


A) 10 times the size of the solar system and contain 2 to 3 solar masses of material.
B) 10 pc across and contain a few thousand solar masses of material.
C) 100 pc across and contain 2 million solar masses of material.
D) 1000 pc across and contain 100 million solar masses of material.

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

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When does a star achieve hydrostatic equilibrium?


A) when it becomes a main-sequence star
B) when it leaves the main sequence
C) when it becomes a protostar
D) This question has different answers for stars of different masses. Massive stars never achieve equilibrium; small stars achieve hydrostatic equilibrium as soon as they reach the main sequence.

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

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A low-mass red dwarf (0.08 M < M < 0.4 M) experiences which of these fusion reactions as the last fusion reaction in its core?


A) hydrogen fusion
B) helium fusion
C) carbon fusion
D) silicon fusion

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

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How many brown dwarfs and sub-brown dwarfs are estimated to exist in the Milky Way Galaxy?


A) about 450
B) at least a million, but less than 100 million
C) at least 100 billion
D) at least 100 million, but less than 100 billion

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

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When any star on the main sequence was a protostar, it was


A) larger and hotter.
B) hotter but not necessarily larger.
C) cooler but not necessarily larger.
D) larger and cooler.

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

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