COSMIC PERS: STARS GAL+COS ASTR 5 PKG
COSMIC PERS: STARS GAL+COS ASTR 5 PKG
2019th Edition
ISBN: 9780135978979
Author: Bennett
Publisher: PEARSON C
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Chapter 5, Problem 36EAP

Choose the best answer to each of the following. Explain your reasoning with one or more complete sentences.

36. A spectral line that appears at a wavelength of 321 nm in the laboratory appears at a wavelength of 328 nm in the spectrum of a distant object. We say that the object's spectrum is (a) redshifted. (b) blueshifted. (c) whiteshifted.

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Complete the following chart by using Wien's law. You may use a calculator and the Wien's law formula, or the interactive graph Planck Law for Blackbodies to calculate temperature when given wavelength (and vice-versa). Use the data table Blackbody Temperatures of the Electromagnetic Spectrum to identify the region of the electromagnetic spectrum where an object with the stated temperature emits most of its light. Case 1 2 3 4 5 T (kelvins) 5,800 4,460 8,010 Stars as Blackbodies max (angstroms) 7,600 3,640 EM Region ---Select--- ---Select--- ---Select--- ---Select--- ---Select---
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COSMIC PERS: STARS GAL+COS ASTR 5 PKG

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