Bundle: Foundations of Astronomy, Enhanced, 13th + LMS Integrated MindTap Astronomy, 2 terms (12 months) Printed Access Card
13th Edition
ISBN: 9781337368360
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
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Chapter 18, Problem 11RQ
To determine
The most dominant factor during the time of re-ionization, the time of photon and particle soup and today.
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Chapter 18 Solutions
Bundle: Foundations of Astronomy, Enhanced, 13th + LMS Integrated MindTap Astronomy, 2 terms (12 months) Printed Access Card
Ch. 18 - Is cosmology the study of the Universe, the...Ch. 18 - Is a cosmologist an astronomer? Is an astronomer a...Ch. 18 - How does the darkness of the night sky tell you...Ch. 18 - Explain the differences among the observable...Ch. 18 - Prob. 5RQCh. 18 - Prob. 6RQCh. 18 - Prob. 7RQCh. 18 - Prob. 8RQCh. 18 - Prob. 9RQCh. 18 - Prob. 10RQ
Ch. 18 - Prob. 11RQCh. 18 - If you accept the cosmological principle, how can...Ch. 18 - Why cant an open universe have a center? How can a...Ch. 18 - In which type of model universe is space-time...Ch. 18 - In which type of model universe is space-time...Ch. 18 - What is the fate of a closed universe? In what...Ch. 18 - In which model universe does the average density...Ch. 18 - Prob. 18RQCh. 18 - What evidence shows that the Universe is...Ch. 18 - Why couldnt atomic nuclei exist when the Universe...Ch. 18 - Why are measurements of the current density of the...Ch. 18 - What percentage of matter is ordinary matter? What...Ch. 18 - How does the inflationary universe hypothesis...Ch. 18 - Prob. 24RQCh. 18 - What is the evidence that the Universe was...Ch. 18 - Prob. 26RQCh. 18 - If the Universe is negatively curved, and dark...Ch. 18 - What is the difference between hot dark matter and...Ch. 18 - Prob. 29RQCh. 18 - What evidence can you cite that the Universe's...Ch. 18 - Prob. 31RQCh. 18 - Reasoning by analogy often helps make complicated...Ch. 18 - Prob. 33RQCh. 18 - Prob. 1DQCh. 18 - Prob. 2DQCh. 18 - Prob. 3DQCh. 18 - Prob. 1PCh. 18 - Prob. 2PCh. 18 - Prob. 3PCh. 18 - Measure the lengths of the two arrows in the left...Ch. 18 - Prob. 5PCh. 18 - Prob. 6PCh. 18 - Find the wavelength of maximum intensity of the...Ch. 18 - Prob. 8PCh. 18 - Prob. 9PCh. 18 - Prob. 10PCh. 18 - Prob. 11PCh. 18 - Prob. 12PCh. 18 - Prob. 1LTLCh. 18 - Prob. 2LTLCh. 18 - Prob. 3LTLCh. 18 - Prob. 4LTLCh. 18 - Prob. 5LTLCh. 18 - Prob. 6LTL
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- Would a human have been possible during the first generation of stars that formed right after the Big Bang? Why or why not?arrow_forwardWhat are some answers to the Fermi paradox? Can you think of some that are not discussed in this chapter?arrow_forwardWhy couldnt atomic nuclei exist when the Universe was less than about 2 minutes old?arrow_forward
- The background radiation has an average temperature of 2.7 K, using Wien’s Law, the current background radiation in the microwave region, the peak wavelength is 1mm. In the past, when the cosmic background radiation had a peak wavelength of 51.1 µm, calculate the relative size of the universe compared to the current size of the universe, that is, the universe was how much smaller by a factor of what? Round to TWO places past the decimalarrow_forwardWhere did all the antimatter go?arrow_forwardWhat happened before the Big Bang?arrow_forward
- Consider three periods in the history of the Universe: one million years after the Big Bang (age = 1 million years), about five billion years ago (age = 9 billion years), and today. What is the ranking in the expansion rate of the Universe in these three period, from fastest to slowest expansion: O 1 million years, today, 9 billion years. today, 1 million years, 9 billion years. today, 9 billion years, 1 million years. O 1 million years, 9 billion years, today.arrow_forwardThe present number density of electrons in the Universe is the same as that of protons, about 0.2 m-3. Consider a time long before the formation of the microwave background, when the scale factor was x times smaller than its present value. What was the number density of electrons then? Value: x = 12×106arrow_forwardYour friends are talking about Olber's Paradox: Friend 1: When the universe was quite young, it was also quite small, and therefore light was trapped inside the universe. This is why we don't see light from the edge of the universe in every direction. Friend 2: No, Olber's Paradox describes only light from stars, not from galaxies, and why you can't use light from distant stars to see at night. Friend 3: You're both right and you're both wrong. The paradox concerns itself with the expansion of the universe, and explains why light from the early universe was able to be released. Are any of them right, in part or in whole?arrow_forward
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