Bundle: Foundations of Astronomy, Enhanced, Loose-Leaf Version, 13th + MindTap Astronomy, 2 terms (12 months) Printed Access Card
13th Edition
ISBN: 9781337214353
Author: Seeds, Michael A., Backman, Dana
Publisher: Cengage Learning
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Textbook Question
Chapter 18, Problem 23RQ
How does the inflationary universe hypothesis resolve the flatness problem? How does that hypothesis resolve the horizon problem?
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The figure below is based on an assumed Hubble constant of 70 km/s/Mpc. How would you change the diagram to fit a Hubble constant of 50 km/s/Mpc?
If the evolution of the universe were
determined only by gravity, then its
fate would be linked to its geometry.
Open
Negligible normal matter
Flat
Closed
14
9.5
Past Future
Time
Billion years ago
Now
The slope of the "negligible normal matter" line would be ---Select---
C and cross the time axis ---Select---
O than 14 billion years ago. The curved line separating the open and closed
universe regions would cross the time axis
O than 9.5 billion years ago.
---Select---
Scale of the universe, R
© Cengage Learning 2013
What is the difference between hot dark matter and cold dark matter? What difference does that
make to cosmology?
Does Hubble's Law work well for galaxies in the Local Group (such as Andromeda)?
No, because dark energy is accelerating the universe's expansion over those distances.
No, because we do not know the precise value of Ho.
No, because Hubble did not know the Local Group existed when he discovered his law.
Yes, it works well for all galaxies.
No, because galaxies in the Local Group are bound gravitationally together.
Chapter 18 Solutions
Bundle: Foundations of Astronomy, Enhanced, Loose-Leaf Version, 13th + 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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Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.Similar questions
- What is the difference between hot dark matter and cold dark matter? How does this difference affect cosmology?arrow_forwardWhy cant an open universe have a center? How can a closed universe not have a center?arrow_forwardExplain what we mean when we call the universe homogeneous and isotropic. Would you say that the distribution of elephants on Earth is homogeneous and isotropic? Why?arrow_forward
- How does the darkness of the night sky tell you something important about the age and size of the observable universe?arrow_forwardWhat does it mean to say that the universe is expanding? What is expanding? For example, is your astronomy classroom expanding? Is the solar system? Why or why not?arrow_forwardIt is possible to derive the age of the universe given the value of the Hubble constant and the distance to a galaxy, again with the assumption that the value of the Hubble constant has not changed since the Big Bang. Consider a galaxy at a distance of 400 million light-years receding from us at a velocity, v. If the Hubble constant is 20 km/s per million light-years, what is its velocity? How long ago was that galaxy right next door to our own Galaxy if it has always been receding at its present rate? Express your answer in years. Since the universe began when all galaxies were very close together, this number is a rough estimate for the age of the universe.arrow_forward
- There is still some uncertainty in the Hubble constant. (a) Current estimates range from about 19.9 km/s per million light-years to 23 km/s per million light-years. Assume that the Hubble constant has been constant since the Big Bang. What is the possible range in the ages of the universe? Use the equation in the text, T0=1H , and make sure you use consistent units. (b) Twenty years ago, estimates for the Hubble constant ranged from 50 to 100 km/s per Mps. What are the possible ages for the universe from those values? Can you rule out some of these possibilities on the basis of other evidence?arrow_forwardSuppose you were Hubble and Humason, working on the distances and Doppler shifts of the galaxies. What sorts of things would you have to do to convince yourself (and others) that the relationship you were seeing between the two quantities was a real feature of the behavior of the universe? (For example, would data from two galaxies be enough to demonstrate Hubble’s law? Would data from just the nearest galaxies-in what astronomers call “the Local Group”-suffice?)arrow_forwardWhat evidence shows that the Universe is expanding? What evidence shows that the Universe began with a Big Bang?arrow_forward
- What percentage of matter is ordinary matter? What percentage is dark matter? What makes up the rest of the Universes density?arrow_forwardThe Andromeda Galaxy is a member of the Local Group of galaxies. It is approaching us. Does this mean that the Hubble Law is wrong? Why or why not? Explain.arrow_forwardExplain the expanding Universe theory and its relationship to the Big Bang theory?arrow_forward
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