Life in the Universe (4th Edition)
4th Edition
ISBN: 9780134089089
Author: Jeffrey O. Bennett, Seth Shostak
Publisher: PEARSON
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Textbook Question
Chapter 9, Problem 4RQ
What is tidal heating? Briefly explain how it can arise and persist as a result of orbital resonances. How does tidal heating affect Io?
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Assuming all other variables were earth based besides atmospheric pressure, calculate the temperature at which water would boil at sea level on Titan versus Earth? And explain why using molecular concepts. Consider the pressure of Earth’s atmosphere at sea level to be 1 atm and the pressure of Titan’s atmosphere at sea level to be 1.45 atm.
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Chapter 9 Solutions
Life in the Universe (4th Edition)
Ch. 9 - Briefly explain how the larger jovian moons tend...Ch. 9 - Briefly describe the cause of the tides on Earth,...Ch. 9 - What is synchronous rotation, and why is it so...Ch. 9 - What is tidal heating? Briefly explain how it can...Ch. 9 - Describe the evidence suggesting that Europa has a...Ch. 9 - What energy sources might be available to life on...Ch. 9 - Describe the evidence for subsurface oceans on...Ch. 9 - Why was Titan chosen for such intense study by the...Ch. 9 - Based on recent data, describe the general nature...Ch. 9 - What evidence suggests that Enceladus might be...
Ch. 9 - Could Triton be habitable? Briefly discuss the...Ch. 9 - What do we mean by chemical equilibrium and...Ch. 9 - Prob. 13RQCh. 9 - Based on our understanding of the chemistry of...Ch. 9 - Io is riddled with volcanoes because of its...Ch. 9 - Europa is likely to have fishlike organisms the...Ch. 9 - While Europa, Ganymede, and Callisto are all...Ch. 9 - The fact that our Moon keeps one side always...Ch. 9 - Titan is simply too cold to have any life.Ch. 9 - Triton might have life that uses liquid ammonia,...Ch. 9 - Io doesnt have a significant atmosphere because it...Ch. 9 - Orbital resonances like those among Io, Europa,...Ch. 9 - If there is life on Enceladus, it probably gets...Ch. 9 - If our solar system is typical, other star systems...Ch. 9 - The moons of Saturn may have large amounts of...Ch. 9 - Which statement about synchronous rotation is...Ch. 9 - Io is covered in volcanoes while Europa is covered...Ch. 9 - Which of the following is not an indication of...Ch. 9 - Photosynthesis is an unlikely source of energy for...Ch. 9 - Its assumed that, even if Europa has life, the...Ch. 9 - The chances for life on Titans surface are...Ch. 9 - Where might we find liquid water on Titan? (a) in...Ch. 9 - Why were scientists so surprised to find active...Ch. 9 - Chemical disequilibrium is likely to be present in...Ch. 9 - Cost-Effective Exploration. Given its budget, NASA...Ch. 9 - Lessons for Life. Considering everything weve...Ch. 9 - Exploring Europa I. Although Europa is a promising...Ch. 9 - Exploring Europa II. One suggestion for...Ch. 9 - Europan Fish. On Earth, fish breathe oxygen that...Ch. 9 - Life on Titan. Several possibilities have been...Ch. 9 - Migrating Life. As we discussed in Chapter 6,...Ch. 9 - Orbital Resonances I. Using the data in Appendix...Ch. 9 - Orbital Resonances II. Using the data in Appendix...Ch. 9 - Tidal Force on the Moon. In Cosmic Calculations...Ch. 9 - Tidal Force on Io. Using the procedure from Cosmic...Ch. 9 - Tidal Force on Europa and Ganymede. Using the...Ch. 9 - Limited Thinking. Throughout this book, we have...Ch. 9 - Europa Orbiter. Find out the current status of...
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- Why are the belts and zones on Saturn less distinct than those on Jupiter?arrow_forwardDoes Titan experience volcanism today? Impact cratering? How do you know?arrow_forwardWhat is the frost line in the solar nebula? Explain how temperature differences led to the formation of two distinct types of planets.arrow_forward
- O e. as a moon QUESTION 3 You observe a large, round object orbiting Uranus. How would you classify this object? O a. as a planet Ob. as a dwarf planet Oc. as an asteroid Od. as a Kuiper belt object e. as a moon QUESTION 4 What is one difference between asteroids and Kuipter Belt Objects (KBOS)? O a. asteroids are composed of rock and ice, while KBOS are composed of just rock b. asteroids orbit the Sun, while KBOS orbit Pluto C. asteroids orbit between Mars and Jupiter, while KBO's orbit near Pluto d. asteroids have very elliptical orbits, while KBOS have very circular orbits e. asteroids are small and potato-shaped, while KBOS are large and round DO000arrow_forwardCompare Titan to Rhea. Estimate the strength of surface gravity on Titan compared to the gravity on Titan. How does this affect the possibility of an atmosphere on each? Use g=GM/R2 Titan Radius: 2,575 km, Mass: 2.31 x 1021 kg Rhea Radius: 764 km, Mass: 1.35 x 1023 kgarrow_forwardWhy is it unlikely that humans will be traveling to Io? (Hint: Review the information about Jupiter’s magnetosphere in The Giant Planets.)arrow_forward
- Describe the different processes that lead to substantial internal heat sources for Jupiter and Saturn. Since these two objects generate much of their energy internally, should they be called stars instead of planets? Justify your answer.arrow_forward1) Why is life more likely to be found on the moons of the Gas Giants instead of on the Gas Giants themselves? 2) Describe what we think the interior of jupiter is like. What are the different layers inside jupiter? How do we know this?arrow_forwardWhat is the escape velocity for Enceladeus in m/sec2 and could the plume particles form a ring around Saturn? Answer choices: 239, no 230, yes 250, no 239, yesarrow_forward
- Even if the Europa Clipper can't send a lander down to Europa's surface, it may still be able to sample the sub-ice ocean during some of its flybys. How would this work? a The spacecraft would rendezvous with one of the large number of comets that we know are made of water erupted from Europa's ocean through its volcanoes. b There is some evidence that plumes of water shoot out of Europa, and the spacecraft could fly through them. c The spacecraft would crash into Europa, sampling the sub-ice ocean during the last seconds of its mission. d The spacecraft would drop powerful bombs onto Europa, shattering the ice and blasting some of the water into space to be sampled there.arrow_forwardSaturn’s E ring is broad and thin, and far from Saturn. It requires fresh particles to sustain itself. What is the source of new E-ring particles?arrow_forwardWe have a lot of good images of the large moons of Jupiter and Saturn from the Galileo and Cassini spacecraft missions (check out NASA’s Planetary Photojournal site, at http://photojournal.jpl.nasa.gov, to see the variety). Now that the New Horizons mission has gone to Pluto, why don’t we have as many good images of all sides of Pluto and Charon?arrow_forward
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