Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 20, Problem 33Q
To determine
The substitute names for white dwarf, brown dwarf, and red dwarf stars respectively that perfectly describe their stellar properties.
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Which of the following most correctly explains why we have not yet observed any white dwarfs derived from M stars:
Group of answer choices
Most M stars end up as neutron stars or black holes.
The lifetime of M stars is longer than the age of the universe.
Most M stars are located near the edge of the universe, beyond the visible horizon.
Most M stars are members of a binary system, and the white dwarf would be obscured by the glare of the more massive companion.
White dwarfs are too dim to be observed with currently available techniques.
Globular clusters contain no stars more massive than the Sun. Which of the following seems like the least reasonable implication of this observation?
Group of answer choices
Globular clusters are very old.
Globular clusters are very young.
Only the low-mass stars are still "alive" in the clusters.
Many red giants can probably be found in globular clusters.
The very massive stars in the globular clusters have already burnt out.
Which of the following is least reasonable regarding novae and supernovae?
Group of answer choices
A type I (carbon-detonation) supernova results when a white dwarf in a binary system absorbs enough mass from its companion to push it over the Chandrasekhar limit.
A type II supernova results from any supermassive star at the end of its life, when it runs out of fusion energy and collapses.
A nova can occur multiple times in a binary system.
If a white dwarf in a binary system absorbs enough mass to go beyond the Chandrasekhar limit, the white dwarf explodes as a supernova.
The reason a type I supernova does not produce hydrogen lines is that the explosion originates from a stellar core (white dwarf), where hydrogen has already fused to produce heavier elements (so there is no longer any hydrogen).
More supernovae are observed in the Milky Way because they are much closer to us than those in other galaxies.
Chapter 20 Solutions
Universe
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