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A) the Coulomb barrier
B) hydrostatic equilibrium
C) the birth line
D) the zero-age main sequence
E) the evolutionary track
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A) 1 solar masses
B) 80 solar masses
C) 8 solar masses
D) 0.08 solar masses
E) 0.001 solar masses
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Multiple Choice
A) the balance between the pressure and force of gravity inside a star.
B) the force that binds protons and neutrons together to form a nucleus.
C) the force that binds an electron to the nucleus in an atom.
D) a measure of the resistance to the flow of radiation (photons) through a gas.
E) the temperature and density at which a gas will undergo thermonuclear fusion.
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True/False
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Multiple Choice
A) HI regions
B) HII regions
C) Emission nebulae
D) Bok globules
E) Reflection nebulae
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Multiple Choice
A) luminosity depends on mass.
B) pressure depends on temperature.
C) density depends on mass.
D) weight depends on temperature.
E) temperature depends on mass.
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A) The rapid outward flow of gas.
B) The rapid inward flow of the gas.
C) The high temperature of the gas.
D) The high density of the gas.
E) c and d
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True/False
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A) 0.01 solar masses
B) 0.1 solar masses
C) 1.1 solar masses
D) 11 solar masses
E) 110 solar masses
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Multiple Choice
A) no neutrinos are produced.
B) energy is released because a hydrogen nucleus has a greater mass than a helium nucleus.
C) no photons are produced.
D) carbon serves as a catalyst for the nuclear reaction.
E) energy is produced in the form of gamma rays and the velocity of the created nuclei.
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Not Answered
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Multiple Choice
A) has been disproved by the results of later experiments.
B) can be explained if the sun is not undergoing thermonuclear fusion of hydrogen in its core.
C) indicates that the sun s core is much hotter than expected.
D) indicates that the sun s core is convective.
E) none of the above
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A) the protostar stage is very short.
B) they are surrounded by cocoons of gas and dust.
C) they radiate mainly in the infrared.
D) all of the above
E) they are all so far away that the light hasn t reached us yet.
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