A) hydrogen burning in a thin shell around the core
B) helium burning in the core
C) carbon burning
D) death (it becomes either a supernova or a white dwarf)
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Multiple Choice
A) of indeterminate age since the age of the cluster cannot be estimated from the information given.
B) impossible because cool stars cannot be above the main sequence when hot stars are on the main sequence.
C) old because the G and K stars are already evolving off (away from) the main sequence.
D) very young because the G and K stars are still evolving toward the main sequence.
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Multiple Choice
A) Open clusters contain very hot stars that produce metals by nuclear reactions in their outer layers.
B) Globular clusters have "burned" their heavy elements over their longer lifetime.
C) Globular clusters are too young for their stars to have produced any significant amount of metals.
D) Open clusters are young and stars have formed from material that has been enriched in metals by supernova explosions of previous stars.
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Multiple Choice
A) the same age.
B) the same mass.
C) moving in the same direction.
D) the same spectral type.
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Multiple Choice
A) The star explodes, forming a supernova remnant.
B) Gas is spun off from the star's equator, from which planets may form.
C) Nuclear reactions begin in the star's core, converting hydrogen into helium.
D) The star begins a long period of contraction in which gravitational energy is converted into heat.
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Multiple Choice
A) just before red giant phase, when variability begins
B) well established on the main sequence
C) the end of its life, decaying away and cooling
D) protostar, before the main-sequence phase
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Multiple Choice
A) stars with masses less than 0.08 solar mass
B) stars with masses less than 0.75 solar mass
C) stars with masses greater than 100 solar masses
D) stars with masses greater than 10 solar masses
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Multiple Choice
A) You will see mostly main-sequence stars; yes, these are the most numerous of stars.
B) You will see mostly main-sequence stars, but most stars are actually giants.
C) You will see mostly giants, but most stars are actually main-sequence stars.
D) You will see mostly giants; yes, most stars are actually giants.
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Multiple Choice
A) ¹H + ⁴He combine to form C,
B) ⁴He fuses to form C.
C) ²He fuses to form C.
D) ³He fuses to form C.
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Multiple Choice
A) Lower-mass stars run through their lives faster and have shorter lifetimes.
B) The lifetimes of stars are too long to measure, so it is not known how (or if) their lifetimes depend on mass.
C) A star's lifetime does not depend on its mass.
D) Higher-mass stars run through their lives faster and have shorter lifetimes.
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Multiple Choice
A) tidal distortion of the shapes of the stars
B) reduction of the quantum mechanical limitation on continued shrinking of one star by the gravitational field of the second star
C) mass exchange between the stars
D) radiation from one star heating the surface of the second star
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Multiple Choice
A) The stars all have the same apparent magnitude, the same surface temperatures, and the same sizes.
B) The stars are all at the same distance from Earth, have the same surface temperature, and joined the cluster at various times.
C) The stars all have the same intrinsic brightness but differ in size and surface temperature.
D) The stars are at the same distance from Earth, were formed at approximately the same time, and were made from the same chemical mix.
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Multiple Choice
A) with a surface temperature equal to that of the Sun.
B) in which nuclear fusion reactions generate sufficient energy to oppose further condensation of the star.
C) whose age after birth is about 1 million years.
D) with a luminosity precisely equal to that of the Sun.
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Multiple Choice
A) Most stars die at the end of the main-sequence phase.
B) The main-sequence phase is the longest-lasting phase in each star's life.
C) The main-sequence phase is the only phase that is common to all stars.
D) Most stars in the sky were created at about the same time, so these are all in the same phase of their lives.
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Multiple Choice
A) 10-¹⁴ solar mass per year
B) 10-³ solar mass per year
C) Red giant stars do not suffer mass loss.
D) 10-⁷ solar mass per year
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Multiple Choice
A) radioactive elements.
B) gravitational potential energy being converted to heat as the protostar collapses.
C) infalling material colliding with the protostar's surface.
D) nuclear fusion.
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Multiple Choice
A) detached
B) overcontact
C) contact
D) semidetached
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Multiple Choice
A) 50%
B) 2%
C) 10%
D) 25%
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Multiple Choice
A) helium
B) carbon
C) nitrogen
D) iron
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Multiple Choice
A) X-ray
B) visible
C) ultraviolet
D) radio
Correct Answer
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