The Cosmic Perspective (9th Edition)
9th Edition
ISBN: 9780134874364
Author: Jeffrey O. Bennett, Megan O. Donahue, Nicholas Schneider, Mark Voit
Publisher: PEARSON
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Chapter 10, Problem 49EAP
(a)
To determine
To Explain: No-greenhouse temperature of Venus is lower than Earth though it is closer to the Sun.
(b)
To determine
The surface temperature of Venus of it had no clouds and greenhouse gases.
(c)
To determine
The way clouds and volcanoes are linked on Venus and the way change in volcanism might result in the disappearance of clouds.
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CO2 and planetary warming: understanding Earth’s complicated atmosphere Mars has an atmospheric pressure of 6 mbar (compared with Earth atmosphere pressure of 1013 mbar), 96% of which is CO2. The average calculated temperature of Mars is -57°C, whereas the actual average temperature is -55°C so that the amount of warming due to CO2 is only 2°C. On the other hand, the average calculated temperature of Earth, with 0.4 mbar of CO2, is -19°C, whereas the actual average temperature is 15°C so that the amount of warming due to CO2 is 34°C, much greater than that on Mars, which has higher CO2 concentration. Explain how this is possible.
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Chapter 10 Solutions
The Cosmic Perspective (9th Edition)
Ch. 10 - Prob. 1VSCCh. 10 - Use the following questions to check your...Ch. 10 - Use the following questions to check your...Ch. 10 - Use the following questions to check your...Ch. 10 - Use the following questions to check your...Ch. 10 -
Briefly describe the basic atmospheric...Ch. 10 - Prob. 2EAPCh. 10 - Prob. 3EAPCh. 10 - What is the greenhouse effect? Describe how it...Ch. 10 - What factors determine a world’s “no greenhouse”...
Ch. 10 - Describe Earth’s basic atmospheric structure, from...Ch. 10 - Prob. 7EAPCh. 10 - Why does convection occur in the troposphere,...Ch. 10 - Prob. 9EAPCh. 10 - What is a magnetosphere? Describe its role in...Ch. 10 - Prob. 11EAPCh. 10 - Prob. 12EAPCh. 10 - Prob. 13EAPCh. 10 - Prob. 14EAPCh. 10 - Prob. 15EAPCh. 10 - Prob. 16EAPCh. 10 - Prob. 17EAPCh. 10 - Prob. 18EAPCh. 10 - Prob. 19EAPCh. 10 - Describe four ways in which Earth’s atmosphere is...Ch. 10 - What is the carbon dioxide cycle, and why is it so...Ch. 10 - Prob. 22EAPCh. 10 - Prob. 23EAPCh. 10 - Prob. 24EAPCh. 10 - Prob. 25EAPCh. 10 - Does It Make Sense? Decide whether the statement...Ch. 10 - Prob. 27EAPCh. 10 - Prob. 28EAPCh. 10 - Prob. 29EAPCh. 10 - Prob. 30EAPCh. 10 - Prob. 31EAPCh. 10 - Prob. 32EAPCh. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Prob. 37EAPCh. 10 - Prob. 38EAPCh. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Choose the best answer to each of the following....Ch. 10 - Prob. 44EAPCh. 10 - Prob. 45EAPCh. 10 - Prob. 49EAPCh. 10 - Atmospheric Structure. Study Earth’s average...Ch. 10 - Magic Mercury. Suppose we could magically give...Ch. 10 - A Swiftly Rotating Venus. Suppose Venus rotated as...Ch. 10 - Prob. 53EAPCh. 10 - Prob. 54EAPCh. 10 - Two Paths Diverged. Briefly explain how the...Ch. 10 - Prob. 56EAPCh. 10 - Feedback Processes in the Atmosphere. As the Sun...Ch. 10 - Prob. 58EAPCh. 10 - Prob. 59EAPCh. 10 - Prob. 60EAPCh. 10 - The Mass of an Atmosphere. What is the total mass...Ch. 10 - The Role of Reflectivity. By assuming 0% and 100%...Ch. 10 - The Cooling Clouds of Venus. Table 10.2 shows that...Ch. 10 - Mars’s Elliptical Orbit. Mars’s distance from the...Ch. 10 - Escape from Venus. Calculate the escape velocity...
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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
- Why do small planets cool faster than large planets? Choose any two of the five Terrestrial worlds and calculate for each one the ratio of its surface area to its volume. Why is this ratio important? (Hint: Does this ratio have anything to do with the ability of a planet to lose internal heat?) (Note: The surface area of a sphere is 4r2, and the volume of a sphere is 43r3.)arrow_forwardThe runaway greenhouse effect and its inverse, the runaway refrigerator effect, have led to harsh, uninhabitable conditions on Venus and Mars. Does the greenhouse effect always cause climate changes leading to loss of water and life? Give a reason for your answer.arrow_forwardDescribe the current atmosphere on Mars. What evidence suggests that it must have been different in the past?arrow_forward
- How might Venus’ atmosphere have evolved to its present state through a runaway greenhouse effect?arrow_forwardWhich of the following planetary traits is well established? choose one of the following: a) Mercury has a similar compositon to that of our moon, in that they both have a substantial metal content. b) Venus rotates more rapidly than Earth, but in the opposite direction. c) Earth's atmosphere exhibits a slightly stronger greenhouse effect than that seen on Venus. d)Astronomers have precisely calculated the mass of Mercury thanks to artificial satellites sent from Earth.arrow_forwardDescribe the planet Venus. Attributes like atmosphere, rotation, etc. should be included in your description.arrow_forward
- Venus is very bright and reflective because of its a. high surface temperatures b. large number of active volcanoes c. thick cover of sulfuric-acid clouds d. planet-wide oceans 2. The first six Soviet Venera landers failed to return pictures and data from Venus because they all a. got excessively corroded during their passage through Venus's sulfuric-acid clouds b. fell too slowly through Venus's thick atmosphere and got fried before landing c. missed their rendezvous withe Venus because of errors in their orbits d. got cancelled due to technical or budgetary problemsarrow_forwardA new Terrestrial planet has been discovered orbiting a nearby Sun-like star. Astronomers have obtained spectra of this planet and determined that the atmosphere is composed of roughly 99% CO2, and the remaining 1% is mostly N2 and is very thin compared to Earth's atmosphere. Briefly describe how the planet could have developed such an atmosphere.arrow_forwardFully describe the greenhouse effect. How is this important for life on earth?arrow_forward
- Eventually, space telescopes have shown that Venus is shrouded by a very dense atmosphere (see Figure 6). To pierce through the dense clouds and study its surface, astronomers had to use radio imaging (see Figure 7). Venus’ atmosphere is transparent to radio waves. Research and explain briefly how, through radio imaging, Venus’ surface could be reconstructed.arrow_forwardLearn about current and planned missions to study a terrestrial planet's atmosphere (including Earth). Write a one-page essay describing the mission and the lessons learned.arrow_forwardWhat component of Venus’s atmosphere causes the planet to be so hot? Explain whythere is so much of this gas in the atmosphere of Venus, compared with its presence inEarth’s atmosphere. What happened to all the water that Venus must have had when theplanet formed?arrow_forward
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