Chapter 19: Problem 8
Explain how it is possible for the core of a red giant to contract at the same time that its outer layers expand.
Chapter 19: Problem 8
Explain how it is possible for the core of a red giant to contract at the same time that its outer layers expand.
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Get started for freeWhy do Cepheid stars pulsate? Why are these stars important to astronomers who study galaxies beyond the Milky Way?
As a red giant, the Sun's luminosity will be about 2000 times greater than it is now, so the amount of solar energy falling on the Earth will increase to 2000 times its present-day value. Hence, to maintain thermal equilibrium, each square meter of the Earth's surface will have to radiate 2000 times as much energy into space as it does now. Use the Stefan-Boltzmann law to determine what the Earth's surface temperature will be under these conditions. (Hint: The present-day Earth has an average surface temperature of \(14^{\circ} \mathrm{C}\).)
Why do astronomers attribute the observed Doppler shifts of a Cepheid variable to pulsation, rather than to some other cause, such as orbital motion?
Explain why the majority of the stars visible through telescopes are main- sequence stars.
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