Astronomy
1st Edition
ISBN: 9781938168284
Author: Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher: OpenStax
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Textbook Question
Chapter 11, Problem 21E
Would you expect to find free oxygen gas in the atmospheres of the giant planets? Why or why not?
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Chapter 11 Solutions
Astronomy
Ch. 11 - What are the main challenges involved in sending...Ch. 11 - Why is it difficult to drop a probe like Galileo?...Ch. 11 - Explain why visual observation of the gas giants...Ch. 11 - What are the seasons like on Jupiter?Ch. 11 - What is the consequence of Uranus’ spin axis being...Ch. 11 - Describe the seasons on the planet Uranus.Ch. 11 - At the pressures in Jupiter’s interior, describe...Ch. 11 - Which of the gas giants has the largest icy/rocky...Ch. 11 - In the context of the giant planets and the...Ch. 11 - What is the primary source of Jupiter’s internal...
Ch. 11 - Describe the interior heat source of Saturn.Ch. 11 - Which planet has the strongest magnetic field, and...Ch. 11 - What are the visible clouds on the four giant...Ch. 11 - Compare the atmospheric circulation (weather) of...Ch. 11 - What are the main atmospheric heat sources of each...Ch. 11 - Why do the upper levels of Neptune’s atmosphere...Ch. 11 - How do storms on Jupiter differ from storm systems...Ch. 11 - Describe the differences in the chemical makeup of...Ch. 11 - How did the giant planets grow to be so large?Ch. 11 - Jupiter is denser than water, yet composed for the...Ch. 11 - Would you expect to find free oxygen gas in the...Ch. 11 - Why would a tourist brochure (of the future)...Ch. 11 - The water clouds believed to be present on Jupiter...Ch. 11 - Describe the different processes that lead to...Ch. 11 - Research the Galileo mission. What technical...Ch. 11 - How many times more pressure exists in the...Ch. 11 - Calculate the wind speed at the edge of Neptune’s...Ch. 11 - Calculate how many Earths would fit into the...Ch. 11 - As the Voyager spacecraft penetrated into the...Ch. 11 - The ions in the inner parts of Jupiter’s...
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- Present theory suggests that giant planets cannot form without condensation of water ice, which becomes vapor at the high temperatures close to a star. So how can we explain the presence of jovian-sized exoplanets closer to their star than Mercury is to our Sun?arrow_forwardWhy is Pluto not considered a major planet, and what other peculiarity distinguishes it from the major planets?arrow_forwardWhere would you look for some “original” planetesimals left over from the formation of our solar system?arrow_forward
- Why would a tourist brochure (of the future) describing the most dramatic natural sights of the giant planets have to be revised more often than one for the terrestrial planets?arrow_forwardWhy do you think the outer planets have such extensive systems of rings and moons, while the inner planets do not?arrow_forwardAccording to the chart below, how do the gas giants differ from the terrestrial planets? THE TERRESTRIAL PLANETS THE GAS GIANTS MERCURY MARS JUPITER SATURN URANUS NEPTUNE VENUS EARTH ROCK ROCK ROCK ROCK INNER CORE INNER CORE CORE SIren/ Nickel CORE Iron/ WATER WATER WATER Nickel OUTER CORE OUTER CORE METALLIC U HYDROGEN METALLIC WATER MANTLE Reck HYDROGEN MANTLE Rock MANTLE Reck CORE SIren/ Silicates Silicates Silicates Nickel HYDROGEN GAS HYDROGEN GAS HYDROGEN HYDROGEN GAS GAS SURFACE SURFACE SURFACE SURFACE O The gas giants do not have solid surfaces. O The gas giants have an iron core. O The gas giants lack hydrogen gas. O The gas giants do not contain water.arrow_forward
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