Exam 12: The Deaths and Remnants of Stars

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What happens to the wavelength of light as it travels outward through the gravitational field of a planet or star so that the field becomes less strong?

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The great breakthrough in understanding the nature of pulsars was the:

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Expansion under high pressure and temperature results in gas from the accretion disk being propelled away from the black hole as jets.What direction do these jets take?

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What is the observed distribution of the shorter-living gamma-ray bursters in the sky?

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Suppose you were far from a planet that had a very strong gravitational field and you were watching a clock on the surface of the planet.During the time in which your own clock ticks out a time of 1 hour,how much time does the clock on the planet tick out?

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In the process of helium shell fusion in a low-mass star near the end of its life,the star moves upward and to the right on the asymptotic giant branch of the Hertzsprung-Russell diagram.In this process,the star is:

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The mechanism that gives rise to the phenomenon of the nova is:

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A planetary nebula is a(n):

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Which statement about starquakes is CORRECT?

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Neutron stars are believed to be created by:

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In a TV tube,the picture is created by a beam of electrons that travels down the tube at a very high speed.What is the mass of one of these electrons,compared with an electron at rest?

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What is the Schwarzschild radius of a black hole?

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What physical theory has been developed to describe adequately the details of what happens inside a black hole?

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If nothing can ever leave a black hole,can the mass of a black hole ever decrease?

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In which location would a clock run at its fastest rate?

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We have seen that electron degeneracy occurs when the carbon core of a white dwarf becomes dense enough.We have also seen that neutron degeneracy occurs when a neutron star becomes dense enough.Why do you suppose we do not find "proton degeneracy" in some density range between electron and neutron degeneracy?

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What is the typical duration of a gamma-ray burst?

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The period of pulsation for most pulsars is in the range between:

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In the language of general relativity,what we usually call "gravitational force" is described in terms of:

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Type II supernovae show prominent lines of hydrogen in their spectra,whereas hydrogen lines are absent in spectra of Type Ia supernovae.Explain.(Hint: Think about the type of star that gives rise to each of the two types of supernova.)

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