Astronomy
1st Edition
ISBN: 9781938168284
Author: Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher: OpenStax
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Textbook Question
Chapter 11, Problem 3E
Explain why visual observation of the gas giants is not sufficient to determine their rotation periods, and what evidence was used to deduce the correct periods.
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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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- Why would the astronomically short lifetime of gas and dust disks around protostars pose a problem in understanding how the Jovian planets formed? What modification of the solar nebula theory might solve this problem?arrow_forwardWhich of the gas giants has the largest icy/rocky core compared to its overall size?arrow_forwardAre the Gas giants only made out of gas?arrow_forward
- Did hydrogen gas condense from the nebula as the nebula cooled? What about helium gas? How do you know?arrow_forwardHow does the CNO cycle differ from the protonproton chain? How is it similar?arrow_forwardConsider the differentiated meteorites. We think the irons are from the cores, the stony-irons are from the interfaces between mantles and cores, and the stones are from the mantles of their differentiated parent bodies. If these parent bodies were like Earth, what fraction of the meteorites would you expect to consist of irons, stony-irons, and stones? Is this consistent with the observed numbers of each? (Hint: You will need to look up what percent of the volume of Earth is taken up by its core, mantle, and crust.)arrow_forward
- Explain the role of impacts in planetary evolution, including both giant impacts and more modest ones.arrow_forwardWhat was the solar nebula like? Why did the Sun form at its center?arrow_forwardConsider the attached light curve for a transiting planet observed by the Kepler mission. If the host star is identical to the sun, what is the radius of this planet? Give your answer in terms of the radius of Jupiter. Brightness of Star Residual Flux 0.99 0.98 0.97 0.006 0.002 0.000 -8-881 -0.06 -0.04 -0.02 0.00 Time (days) → 0.02 0.04 0.06arrow_forward
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