Horizons: Exploring the Universe (MindTap Course List)
Horizons: Exploring the Universe (MindTap Course List)
14th Edition
ISBN: 9781305960961
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
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Chapter 5, Problem 1LTL
To determine

The causes of distortion observed in the star before adapting optics correct the image.

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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.
The light-gathering power of a telescope is directly related to the area of the telescope's primary mirror.  A mirror with four times the diameter of another mirror collects how many times more light as the smaller mirror does in the same amount of time?  (Numerical answer only, please.)
What are some advantages of radio telescopes over optical scopes?  Explain how adaptive optics can help produce a sharper image.
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