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 1Q
To determine

The definition of refraction and reflection. Explain the way in which these processes help astronomers to build telescopes.

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Use diagrams to describe how the following types of telescope collect light from a single point- source at infinity, and form a focused image in the focal plane: (i) refractor (ii) Newtonian reflector (iii) catadioptric telescope. A telescope with focal ratio f/10 and diameter D = 0.5 m has a CCD detector placed at its focal plane. The CCD chip has dimensions 3 × 3 cm2 . Determine the size of the field of view that can be imaged on the CCD detector in units of arcminutes × arcminutes, and state whether or not an image of the full moon can be captured. Assume the angular diameter of the full moon is 30 arcminutes.
How does light travel?  How does a prism split white light into a spectrum?  How can we produce Magenta, cyan, and yellow?  How does a pinhole camera work?
Imagine that you are the head of a funding agency that can afford to build one telescope. Which of the following proposed telescopes would be best to support?   A. a visible light telescope in Earth orbit   B. An x-ray telescope located on a mountain in Chile    C. A gamma ray telescope in Hawaii    D. An ultraviolet telescope located in Earth orbit
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