21ST C ASTRO EBOOK+SW5=SS+VGCRD+LEARN/DO
21ST C ASTRO EBOOK+SW5=SS+VGCRD+LEARN/DO
6th Edition
ISBN: 9780393870152
Author: PALEN
Publisher: Norton, W. W. & Company, Inc.
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Chapter 6, Problem 40QP

(a)

To determine

The angular resolution of array.

(a)

To determine

Compare the resolution calculated in part (a) with that of the given interferometer.

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a) Describe what is meant by the term Point Spread Function (PSF), explain the relationship between the PSF and the aperture (entrance pupil) of a telescope. You should refer to the ideas of diffraction and Fourier Optics in your answer. b) Determine the plate scale and theoretical resolving power at a wavelength of 380 x 10-9 m of a telescope with 2 m aperture diameter and focal length of 4m.
a. What is the resolving power (in arc seconds) of a 84 cm (33 in.) telescope at a wavelength of 560 nm? b. What do two stars 1.5 arc seconds apart look like through this telescope? - The two points of light are well separated from each other. -The two points of light are only just separated from each other — they are distinguishable but appear to touch.  - The two points of light are indistinguishable from each other.
4. For a space-based imaging system that uses a fixed size aperture for both visible and infrared sensors, given the characteristics listed, what would be the theoretical resolution for each of the sensors?  Aperture diameter = 1.1 m. Visible wavelength = 0.5 micron.  IR wavelength = 2.0 micron.  Altitude = 400 km. (note: 1 micron = 1E-6 m)
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