The Cosmic Perspective (9th Edition)
The Cosmic Perspective (9th Edition)
9th Edition
ISBN: 9780134874364
Author: Jeffrey O. Bennett, Megan O. Donahue, Nicholas Schneider, Mark Voit
Publisher: PEARSON
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Chapter 18, Problem 43EAP
To determine

The life story of a white dwarf star with mass 0.8Msun

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Choose the correct statements from the following list referring to white dwarfs. (Give ALL correct answers, i.e., B, AC, BCD...) A) The pressure that balances gravity in a white dwarf is called degenerate electron pressure.   B) The power source of white dwarfs is left-over heat.   C) White dwarfs cool slowly because they are small and eventually fade-out to become black dwarfs.   D) White dwarfs with mass greater than 1.4 times the Sun's mass cannot exist.   E) Stars with a mass like the Sun will end up as a white dwarf star.   F) White dwarfs are less dense than red giants.   G) White dwarfs are the coolest main sequence stars.
A. Estimate the surface gravity of a neutron star with R = 10 km and M = 2M. . B. Determine the density of such a neutron star in g/cm³. C. How much would a teaspoon (5 cm³) of this neutron star weigh on Earth? This material is known as neutronium. Give your answer in pounds. D. Which would be heavier: a teaspoon of neutronium weighed on Earth, or a teaspoon of water weighed on the surface of a neutron star?
What kind of star is most likely to become a white-dwarf supernova? A. a star like our Sun B. a white dwarf star with a red giant binary companion C. a pulsar D. an O star   Is the answer B?  For D, as the surface temperature of a star would change over time so spectral type cannot tell us about the fate of the stars?

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The Cosmic Perspective (9th Edition)

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