Exam 17: Evolution of High-Mass Stars
Exam 1: Why Learn Astronomy92 Questions
Exam 2: Patterns in the Skymotions of Earth96 Questions
Exam 3: Motion of Astronomical Bodies91 Questions
Exam 4: Gravity and Orbits88 Questions
Exam 5: Light87 Questions
Exam 6: The Tools of the Astronomer94 Questions
Exam 7: The Birth and Evolution of Planetary Systems87 Questions
Exam 8: The Terrestrial Planets and Earths Moon99 Questions
Exam 9: Atmospheres of the Terrestrial Planets92 Questions
Exam 10: Worlds of Gas and Liquid the Giant Planets92 Questions
Exam 11: Planetary Adornmentsmoons and Rings93 Questions
Exam 12: Dwarf Planets and Small Solar System Bodies89 Questions
Exam 13: Taking the Measure of Stars88 Questions
Exam 14: Our Starthe Sun88 Questions
Exam 15: Star Formation and the Interstellar Medium89 Questions
Exam 16: Evolution of Low-Mass Stars90 Questions
Exam 17: Evolution of High-Mass Stars90 Questions
Exam 18: Relativity and Black Holes90 Questions
Exam 19: The Expanding Universe90 Questions
Exam 20: Galaxies95 Questions
Exam 21: The Milky Waya Normal Spiral Galaxy96 Questions
Exam 22: Modern Cosmology92 Questions
Exam 23: Large-Scale Structure in the Universe65 Questions
Exam 24: Life61 Questions
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The production of large numbers of neutrons in nuclear reactions at the core of a massive star helps rob the core of energy and speeds its eventual collapse.
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True
The nuclear reaction that produces most of the energy for massive main-sequence stars is called the CNO cycle.
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True
Neutron stars have masses that range from:
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D
Iron has 26 protons in its nucleus, and gold has 79 protons. Where did all the gold on the Earth come from?
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The Crab Nebula is an important test of our ideas about supernova explosions because:
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Every pulsar is a neutron star, but not every neutron star is a pulsar.
(True/False)
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How do Cepheid variable stars differ from RR Lyrae variable stars in their masses, luminosities, and periods?
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The CNO cycle is the dominant mechanism for hydrogen fusion only in high-mass main-sequence stars because of the greater __________ their cores.
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Explain the effect of core convection on the main-sequence lifetime of massive main-sequence stars and contrast this to the situation in low-mass stars.
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The evolutionary differences between high- and low-mass stars can be attributed to differences in the amount of mass each star possesses.
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When the first pulsar was discovered, scientists thought it might be a signal from a distant extraterrestrial civilization. However, this idea was quickly discarded because:
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Type I and Type II supernovae can be distinguished by what combination of observations?
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High-mass stars differ from low-mass stars in that they burn helium to carbon when on the main sequence.
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If you measure the average brightness and pulsation period of a Cepheid variable star, you can also determine its:
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Each stage of nuclear burning in 25 M star is __________ in duration than in a star of 15 M .
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Although a Type II supernova shines with a luminosity of 100 billion L in light, most of the energy in the explosion is emitted in another way. What is it, and how much more energy does it carry compared to the light?
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Cepheid variable stars are important because we can use them to determine the distance to any stellar group that contains some of these stars.
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