Universe
Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 6, Problem 6CC
To determine

Whether the telescope mirror is deformed more rapidly or less rapidly, by the adaptive optics actuators, on a night when the atmosphere is unusually turbulent than usual night.

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A Kepler telescope has an objective lens of focal length 120 cm. It is used to observe a star cluster of true angular diameter 4 arcmin (where 60 arcmin = 1 degree); and it is desired that the apparent angular diameter of the star cluster when viewed through the telescope is 10 degrees. Calculate the required focal length of the eyepiece.
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(a) What is the angular separation of two stars if their images are barely resolved by the Thaw refracting telescope at the Allegheny Observatory in Pittsburgh? The lens diameter is 76 cm and its focal length is 14 m. Assume l = 550 nm. (b) Find the distance between these barely resolved stars if each of them is 10 light-years distant from Earth. (c) For the image of a single star in this telescope, find the diameter of the first dark ring in the diffraction pattern, as measured on a photographic plate placed at the focal plane of the telescope lens. Assume that the structure of the image is associated entirely with diffraction at the lens aperture and not with lens “errors.”
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