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In what wavelength range do protostars emit most of their energy?


A) optical
B) radio
C) infrared
D) ultraviolet

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

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Massive stars on the main sequence generate energy through the:


A) proton-proton chain.
B) CNO cycle.
C) triple alpha reaction.
D) onion model.

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

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A brown dwarf is a:


A) low-mass star.
B) failed star.
C) stellar remnant supported by electron degeneracy pressure.
D) stellar remnant supported by neutron degeneracy pressure.

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

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Which of the following nuclei can a compact astronomical object with a mass of 0.05 MSun create through fusion?


A) none
B) deuterium
C) helium
D) carbon

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

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A protostar becomes a star when:


A) its luminosity reaches a maximum.
B) its surface temperature reaches 5,000 K.
C) it loses all its gravitational energy.
D) nuclear fusion begins.

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

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What would happen to the Milky Way's interstellar medium if more supernovae occurred than usual?

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It would b...

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Which of the following is an important effect of interstellar dust?


A) a platform for the formation of molecules
B) pressure equilibrium in the interstellar medium
C) a source of diagnostic emission lines
D) heating of the interstellar medium

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

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Why does the initial mass function of stars differ from the actual distribution of stars in the Milky Way at the present day?

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The initial mass function describes the ...

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Which of the following provides the best example of turbulence?


A) a molecular cloud with large whorls containing many smaller whorls
B) a jet launched at near the speed of light by a supermassive black hole
C) a large network of convection cells inside a star
D) an accretion disk rotating around a black hole

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

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Which of the following is most strongly affected by interstellar dust?


A) infrared light
B) visible light
C) microwaves
D) radio waves

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

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What is the wavelength of radiation produced by the system in the figure below? What is the wavelength of radiation produced by the system in the figure below?   A)  91 nm B)  121 nm C)  656 nm D)  21 cm


A) 91 nm
B) 121 nm
C) 656 nm
D) 21 cm

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

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List the five phases of the interstellar medium in order from coolest to hottest.

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Molecular clouds,H I...

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What does it mean for a giant molecular cloud to have a hierarchy of structures?

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The cloud has smalle...

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An interstellar gas cloud with a density of 100 particles per cubic centimeter and with a temperature of 100 K is in equilibrium with a medium with a density of 0.1 particles per cubic centimeter and 10⁶ K.What is the most likely explanation?


A) supernova blast waves
B) photoionization
C) turbulence
D) the ideal gas law

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

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Suppose a star forms with 10 times the mass of the Sun and without any elements heavier than helium.How will the central temperature of this star compare to a star with the same mass but the same composition as the Sun?

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The metal-free star will be ho...

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A Herbig-Haro object is moving at 100 km/s and lies 10 parsecs from a protostar.What is a lower limit for the lifetime of the protostar? Express your answer in years.

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How might an astronomer measure the initial mass function?


A) catalog the masses of all the stars in the Milky Way
B) catalog the masses of all nearby galaxies
C) catalog the masses of all the molecular clouds in the Milky Way
D) catalog the masses of all the stars in a young open cluster

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

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What is the typical size of an interstellar dust grain?


A) 50 microns
B) 5 microns
C) 5 nm
D) 500 nm

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

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What are two reasons that molecules are so abundant within giant molecular clouds?

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The high densities enable them...

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Why do massive stars use the CNO cycle to generate energy,rather than the proton-proton chain?


A) It is more temperature sensitive.
B) Massive stars have more carbon.
C) It produces more energy per helium nucleus.
D) It uses up the carbon too quickly in low-mass stars.

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

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