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 14, Problem 2LTL
To determine
Why the background isn’t perfectly uniform? What does the size of these irregularities tell?
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Explain what is an excitation table?
The difference in absolute magnitude between two objects at the same distance is related to their fluxes by the flux-magnitude relation.
FA
FB
= 2.51(MB − MA)
A distant galaxy contains a type I classical Cepheid whose period results in an absolute magnitude estimate of
−6.3.
If this star were placed next to our Sun
(M = +4.8)
and you observed them both from the same distance, how much more flux would the Cepheid emit than the Sun?
FCepheid
FSun
=
If a galaxy contains a supernova that at its brightest has an apparent magnitude of +11, how far away is the galaxy? Assume that the absolute magnitude of the supernova is
−18.
Hint:
Use the magnitude-distance formula:
d = 10(mV − MV + 5)/5 .
The hydrogen Balmer line H? has a wavelength of 486.1 nm. It is shifted to 559.7 nm in a quasar's spectrum. What is the redshift of this quasar? (Hint: What is Δ??)
Chapter 14 Solutions
Horizons: Exploring the Universe (MindTap Course List)
Ch. 14 - How does the darkness of the night sky tell you...Ch. 14 - How can Earth be located at the center of the...Ch. 14 - Prob. 3RQCh. 14 - Prob. 4RQCh. 14 - Why couldn’t atomic nuclei exist when the e of the...Ch. 14 - Why are measurements of the present density of the...Ch. 14 - Prob. 7RQCh. 14 - Prob. 8RQCh. 14 - What is the evidence that the Universe was very...Ch. 14 - Prob. 10RQ
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- Why would we not expect to detect X-rays from a disk of matter about an ordinary star?arrow_forwardUsing the information from Example 28.1, how much longer will it take you to do your second survey?arrow_forwardH II regions can exist only if there is a nearby star hot enough to ionize hydrogen. Hydrogen is ionized only by radiation with wavelengths shorter than 91.2 nm. What is the temperature of a star that emits its maximum energy at 91.2 nm? (Use Wien’s law from Radiation and Spectra.) Based on this result, what are the spectral types of those stars likely to provide enough energy to produce H II regions?arrow_forward
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