The Solar System
The Solar System
10th Edition
ISBN: 9781337672252
Author: The Solar System
Publisher: Cengage
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Chapter 6, Problem 3LL
To determine

The location of the primary optical element and the behaviour of the element and the reason for it.

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Which of the following pairings of telescope diameter and observational wavelength would give the best resolution images of an object with a telescope? Explain why you chose the telescope and wavelength combination you did, and calculate the angular resolution you could achieve with it.  It would be best to observe with... Option 1:   a 10 m diameter optical telescope on the ground with λ= 550 nm Option 2:  a 2.4 m diameter optical telescope in space with λ=500 nm  Option 3:  a 100 m radio telescope on the ground with λ=100 cm
You want to create a telescope with a resolving powe of 0.100 arc seconds at a wavelength of 550 nm. Wha diameter (in m) do you need? If you want to increase the light gathering power by a factor of 10, by what factor does the diameter need to increase? What would the new resolving power be (in arc seconds)?
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