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A) The initial luminosity of the protostar
B) The size of the interstellar cloud from which the protostar formed
C) The initial temperature of the protostar
D) The mass of the protostar
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Multiple Choice
A) thermal energy emitted as a continuous spectrum by very hot gas,much like that emitted by a hot body on Earth.
B) blue light,preferentially scattered by tiny dust grains.
C) emission lines from hydrogen,which itself has been ionized by UV light from embedded stars.
D) light from embedded stars,reflected over a wide range of wavelengths toward Earth by crystals of water.
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A) large quantities of dust that absorb light but no gas,either atomic or molecular.
B) gas,made up of atoms,molecules,and dust particles.
C) a perfect vacuum.
D) variable amounts of gas but no dust,because dust forms only in planetary systems near stars.
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A) older the cluster is.
B) younger the cluster is.
C) farther away the cluster is.
D) closer the cluster is.
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Multiple Choice
A) If the star gets too big,it will collapse into a black hole.
B) If the stellar gas is suddenly heated,it will expand and cool.
C) If the pressure gets too high,electrons will combine with protons to relieve the pressure.
D) If thermonuclear reactions proceed too quickly,the star will run out of fuel before anything drastic happens.
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A) creating hydrogen from heavier elements absorbing energy in the process.
B) creating hydrogen from heavier elements releasing energy in the process.
C) consuming hydrogen and forging heavier elements absorbing energy in the process.
D) consuming hydrogen and forging heavier elements releasing energy in the process.
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A) asymptotic giant branch stars.
B) T Tauri stars.
C) red-giant stars.
D) main-sequence stars.
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A) hydrogen in the outer layers is fundamentally different from the hydrogen in the core.
B) hydrogen in the outer layers is pure,and hydrogen must be mixed with helium,as it is in the core,in order to undergo fusion.
C) temperature in the outer layers is too low to allow the hydrogen nuclei to come close enough together to undergo fusion.
D) hydrogen atoms in the surface layers are not ionized,as they are in the core,and ionization is one requirement for nuclear fusion.
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A) blue,caused by the preferential scattering of starlight by very small dust grains.
B) starlight of all colors from cool stars,predominantly in the red part of the spectrum,reflected by ice crystals of water,ammonia,and methane.
C) a mixture of several specific colors coming from fluorescence of atoms excited by ultraviolet radiation emitted by hot stars.
D) red,coming from the emission of light from hydrogen gas.
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Multiple Choice
A) When it is expanding in size as a red giant or supergiant
B) Wfter all nuclear reactions have ended in its core
C) Before nuclear reactions begin in its core
D) While it is converting hydrogen to helium in its core
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Multiple Choice
A) A contracting sphere of gas produced by the collapse of an interstellar cloud with,as yet,no nuclear reactions occurring in its interior
B) A shell of gas left behind from the explosion of a star as a supernova
C) A small,cold,interstellar cloud before it collapses to become a star
D) A star near the end of its life,just before it explodes as a supernova
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True/False
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Multiple Choice
A) observing its position in the sky with respect to the Sun.
B) measuring its speed of motion relative to the Sun.
C) carrying out a number count of the stars in the cluster.
D) determining the turnoff point on the main sequence of its H-R diagram.
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A) Scattering of starlight from dust grains within the nebula
B) Thermal (blackbody) radiation from dust grains heated to high temperatures by stellar UV
C) Electrons dropping from n = 3 to n = 2 in hydrogen atoms
D) Electrons dropping from n = 2 to n = 1 in hydrogen atoms
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