Chapter 6: Problem 17
Explain why combining the light from two or more optical telescopes can give dramatically improved angular resolution.
Chapter 6: Problem 17
Explain why combining the light from two or more optical telescopes can give dramatically improved angular resolution.
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Get started for freeWhat is active optics? What is adaptive optics? Why are they useful? Would either of these be a good feature to include on a telescope to be placed in orbit?
Discuss the advantages and disadvantages of using a small telescope in Earth's orbit versus a large telescope on a mountaintop.
What is chromatic aberration? For what kinds of telescopes does it occur? How can it be corrected?
Three of the telescopes shown in Figure 6-16-the James Clerk Maxwell Telescope (JCMT), the Caltech Submillimeter Observatory (CSO), and the Submillimeter Array (SMA)are designed to detect radiation with wavelengths close to \(1 \mathrm{~mm}\). Search for current information about JCMT, CSO, and SMA on the World Wide Web. What kinds of celestial objects emit radiation at these wavelengths? What can astronomers see using JCMT, CSO, and SMA that cannot be observed at other wavelengths? Why is it important that they be at high altitude? How large are the primary mirrors used in JCMT, CSO, and SMA? What are the differences among the three telescopes? Which can be used in the daytime? What recent discoveries have been made using JCMT, CSO, or SMA?
Why are radio telescopes so large? Why does a single radio telescope have poorer angular resolution than a large optical telescope? How can the resolution be improved by making simultaneous observations with several radio telescopes?
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