Universe: Stars And Galaxies
6th Edition
ISBN: 9781319115098
Author: Roger Freedman, Robert Geller, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 19, Problem 3Q
To determine
To define:
Red dwarfs
The way thermonuclear reactions in the core of a red dwarf can consume hydrogen from its outer layers.
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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?
You discover a binary star system in which one member is a 15 solar-mass main-sequence star and the other star is a 10
solar-mass giant. Why should you be surprised, at least at first?
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B. The two stars in a binary system should both be at the same point in stellar evolution; that is, they should either both
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C. The two stars should be the same age, so the more massive one should have become a giant first.
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that such a system could be discovered.
E. A star with a mass of 15 solar-mass is too big to be a main-sequence star.
All massive main sequence stars reside in clouds of glowing gas. The four powerful stars in the center of the Orion Nebula are good examples. Lower mass stars like the Sun generally don't have clouds of gas around them. a. Why do powerful stars reside in gas clouds? b. What is making the gas glow exactly? For the last question, refer to the surface temperature of these stars, and to Wien's Law.
Chapter 19 Solutions
Universe: Stars And Galaxies
Ch. 19 - Prob. 1QCh. 19 - Prob. 2QCh. 19 - Prob. 3QCh. 19 - Prob. 4QCh. 19 - Prob. 5QCh. 19 - Prob. 6QCh. 19 - Prob. 7QCh. 19 - Prob. 8QCh. 19 - Prob. 9QCh. 19 - Prob. 10Q
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