21st Century Astronomy
21st Century Astronomy
6th Edition
ISBN: 9780393428063
Author: Kay
Publisher: NORTON
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Chapter 16, Problem 43QP
To determine

The density of degenerate material and radius of sun.

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How would the interior temperature of the Sun be different if the strong force that binds nuclei together were 10 times as strong?
given that the suns lifetime is about 10 billion years, estimate the life expectancy of (A) a 0.2-solar mass, 0.01-solar luminosity red dwarf
The Sun is estimated to have about 5.00 billion years left in it’s “normal” (main sequence) lifetime. Assume the average “burn” rate that you computed in question #1, what % of the Sun’s current mass will have been converted at the end of it’s estimated 5.00 billion years of additional life? Actually, the Sun will lose more mass due to the solar wind, CMEs, the neutrio flux etc. the answer to number one was 3.683x10^14
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