The Cosmic Perspective (9th Edition)
The Cosmic Perspective (9th Edition)
9th Edition
ISBN: 9780134874364
Author: Jeffrey O. Bennett, Megan O. Donahue, Nicholas Schneider, Mark Voit
Publisher: PEARSON
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Chapter 6, Problem 58EAP

Visible-Light Interferometry. Technological advances are now making it possible to link visible-light telescopes so that they can achieve the same angular resolution as a single telescope over 300 meters in size. What is the angular resolution (diffraction limit) of such a system of telescopes for observations at a wavelength of 500 nanometers?

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11:55 phys.libretexts.org Submit Both the Keck Telescope and Hubble Space Telescope (HST) observe visible light. Given a typical visible light wavelength of 500 nm, and the diameters of 10 m for Keck and 2.4 m for Hubble, which telescope do you think would have better angular resolution? Based on the equation for angular resolution, what is the resolution of Keck at 500 nm? Of HST? How can we help VIEW Submit %D
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.
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

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The Cosmic Perspective (9th Edition)

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