Chapter 19: Problem 16
Explain how and why the turnoff point on the H-R diagram of a cluster is related to the cluster's age.
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Chapter 19: Problem 16
Explain how and why the turnoff point on the H-R diagram of a cluster is related to the cluster's age.
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Use the Stary Night Enthusiast \({ }^{\mathrm{TM}}\) program to look for signs of stellar evolution in our Milky Way Galaxy. In the menu, select Favourites \(>\) Stars \(>\) Sun in Milky Way. You can zoom in or out using the buttons at the right of the toolbar. You can move your viewpoint around the Galaxy by holding down the Shift key and the mouse button as you drag the mouse. (a) What is the color of the central part of the Galaxy? Based on the color of this region, do you expect that there are many massive mainsequence stars there? Would you expect to find many young stars there? Explain your reasoning. (b) Repeat part (a) for the outer regions of the Galaxy.
Why do Cepheid stars pulsate? Why are these stars important to astronomers who study galaxies beyond the Milky Way?
What is the difference between a detached binary, a semidetached binary, a contact binary, and an overcontact binary?
What is a Roche lobe? What is the inner Lagrangian point? Why are Roche lobes important in close binary star systems?
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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