Chapter 19: Problem 54
Discuss how H-R diagrams of star clusters could be used to set limits on the age of the universe. Could they be used to set lower limits on the age? Could they be used to set upper limits? Explain your reasoning.
Chapter 19: Problem 54
Discuss how H-R diagrams of star clusters could be used to set limits on the age of the universe. Could they be used to set lower limits on the age? Could they be used to set upper limits? Explain your reasoning.
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Get started for freeThe larger star in the Algol binary system (see Figure 19-21a) is of spectral class \(\mathrm{K}\), while the smaller star is of spectral class B. Discuss how the color of Algol changes as seen through a small telescope (through which Algol appears as a single star). What is the color during a deep eclipse, when the large star eclipses the small one? What is the color when the small star eclipses the large one?
Eventually the Sun's luminosity will increase to the point where the Earth can no longer sustain life. Discuss what measures a future civilization might take to preserve itself from such a calamity.
The Sun has increased in radius by \(6 \%\) over the past \(4.56\) billion years. Its present-day radius is \(696,000 \mathrm{~km}\). What was its radius \(4.56\) billion years ago? (Hint: The answer is not \(654,000 \mathrm{~km}\).)
Explain why the Earth is expected to become inhospitable to life long before the Sun becomes a red giant.
Although Polaris, the North Star, is a Cepheid variable, it pulsates in a somewhat different way than other Cepheids. Search the World Wide Web for information about this star's pulsations and how they have been measured by astronomers at the U.S. Naval Observatory. How does Polaris pulsate? How does this differ from other Cepheids?
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