A) atoms and ions
B) molecules
C) dust
D) radioactive elements
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Multiple Choice
A) heating of an interstellar cloud by concentrated beams of neutrinos from nearby stars
B) compression of cold interstellar gas by radiation pressure from light from very bright stars
C) condensation of matter by the shock wave from a nearby supernova
D) collision of two cold interstellar clouds
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Multiple Choice
A) Our location in the galactic plane is particularly rich in gas and dust, so an unusually large number of giants and supergiants formed here.
B) Early in the history of our Galaxy, a shock wave passed through our part of the spiral arm, creating a large number of stars all at one time. These stars are now mostly in their giant phases.
C) This is an example of a selection effect. The bright giants and supergiants are the most likely to be seen, even though they are not in the majority numerically.
D) We do not have an explanation for this discrepancy.
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Multiple Choice
A) its orbit around the center of the galaxy in which it resides.
B) changes in its luminosity and temperature on a graph of these two parameters as the star ages.
C) its path across Earth's sky as a consequence of its true motion in space.
D) changes in its size and mass on a graph of these two parameters as the star ages.
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Multiple Choice
A) protostar that is ejecting mass near the end of its pre-main-sequence lifetime.
B) young, massive O or B star.
C) young protostar embedded in a cocoon of dust clouds, visible only by infrared radiation.
D) high-mass yellow giant star that pulsates regularly in size and brightness.
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Multiple Choice
A) isolated atoms
B) isolated molecules
C) small pieces of dust
D) meteoroids
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Multiple Choice
A) gravitational contraction before the start of core hydrogen burning
B) hydrogen-shell burning, with a degenerate helium core
C) core helium burning
D) core hydrogen burning
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Multiple Choice
A) a few million years.
B) half a billion years.
C) 10 billion years.
D) infinite.
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verified
Multiple Choice
A) 1 billion years
B) 1 million years
C) 10¹¹ years
D) 10¹⁰ years
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Multiple Choice
A) The more massive the original star, the faster is the evolution.
B) The chemical make-up of the original nebula is the major factor in deciding the rate of evolution, whatever the mass of the star.
C) Star mass has no bearing on stellar evolution since all stars evolve at the same rate, controlled by nuclear fusion.
D) The more massive the original star, the slower is the evolution since there is more material for thermonuclear burning.
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Multiple Choice
A) at least 200 billion years (2 × 10¹¹) years.
B) about 1 million years.
C) about 4.5 million years.
D) about 10 billion years (10¹⁰ years) .
Correct Answer
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Multiple Choice
A) Type II Cepheids are older, having evolved from Type I Cepheids.
B) The two types have different metallicities.
C) Type I Cepheids are members of binary systems, whereas Type II Cepheids are solitary stars.
D) Type II Cepheids have gone through the helium flash, whereas Type I Cepheids have yet to do so.
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Multiple Choice
A) mass
B) surface temperature
C) abundance of heavy elements
D) speed of rotation
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Multiple Choice
A) If thermonuclear reactions proceed too quickly, the star runs out of fuel before anything drastic happens.
B) If the stellar gas is suddenly heated, it expands and cools.
C) If the star gets too big, it collapses into a black hole.
D) If the pressure becomes too high, electrons combine with protons to relieve the pressure.
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Multiple Choice
A) Neither produces energy by hydrogen fusion.
B) They are primarily composed of hydrogen and helium.
C) They produce similar spectra.
D) They are both fully convective at various stages.
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Multiple Choice
A) white dwarfs.
B) brown dwarfs.
C) the Sun.
D) variable stars.
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Multiple Choice
A) The star is fusing hydrogen into helium in its core.
B) The star is no longer contracting.
C) The gas and dust around the pre-main-sequence star have largely dissipated.
D) Helium burning has begun as the principal energy generating mechanism in the star's core.
Correct Answer
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Multiple Choice
A) hydroxyl (OH)
B) water vapor (H₂O)
C) carbon dioxide (CO₂)
D) carbon monoxide (CO)
Correct Answer
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Multiple Choice
A) ammonia (NH₃)
B) hydrogen (H₂)
C) formaldehyde (H₂CO)
D) carbon monoxide (CO)
Correct Answer
verified
Multiple Choice
A) 0.2
B) 1.2
C) 2.6
D) 4.2
Correct Answer
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