Horizons: Exploring the Universe (MindTap Course List)
14th Edition
ISBN: 9781305960961
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
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Chapter 16, Problem 2LTL
To determine
The reason that Earth’s view is unusual among planets in general.
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In the previous lab, we calculated the area in between Mars' and Jupiter's orbit to be ~1.6e18 km2. Since there are roughly 750,000 asteroids, how much area (in km2) is available for one asteroid? Use this calculation to argue whether you are likely (or not) to hit an asteroid while flying through the asteroid belt.
(Hint: To answer the first part of the question, find the area per asteroid)
Chapter 16 Solutions
Horizons: Exploring the Universe (MindTap Course List)
Ch. 16 - Why would you include the Moon in a comparison of...Ch. 16 - In what ways is Earth unique among the Terrestrial...Ch. 16 - What are the four stages of planetary development?Ch. 16 - How do you know that Earth differentiated?Ch. 16 - How are earthquakes in Hawaii different from those...Ch. 16 - Prob. 6RQCh. 16 - How do island chains located in the centers of...Ch. 16 - Prob. 8RQCh. 16 - H does the increasing abundance of CO2 in Earth’s...Ch. 16 - Why would a decrease in the density of the ozone...
Ch. 16 - Prob. 11RQCh. 16 - Prob. 12RQCh. 16 - Prob. 13RQCh. 16 - How Do We Know? Why is heat flow the key to...Ch. 16 - How Do We Know? In what ways have scientists been...Ch. 16 - Prob. 1DQCh. 16 - Prob. 2DQCh. 16 - Assume P waves travel at 10 km/s and S waves...Ch. 16 - Earth’s metallic core has about 55% of the...Ch. 16 - Prob. 3PCh. 16 - Prob. 4PCh. 16 - Prob. 5PCh. 16 - Earth is four times lager in diameter than its...Ch. 16 - The smallest detail visible through Earth-based...Ch. 16 - Prob. 1LTLCh. 16 - Prob. 2LTLCh. 16 - Prob. 3LTLCh. 16 - Prob. 4LTLCh. 16 - Prob. 5LTL
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- Look at the right top and bottom images in Figure 20-2. Count the number of craters in each image. Based on your result, which portion of the Moons surface do you judge to be relatively older, and why? Figure 202 Details visible in photographs show that meteorite impacts covered the Moon with craters long ago, and then lava flooded out and filled the largest basins, covering the craters there with smooth plains.arrow_forwardWhy do astronomers conclude that the surface of Mercury, shown in Figure UN 15-4, is old? When did the majority of those craters form?arrow_forwardHow Do We Know? How can the flow of energy out of a planets interior affect its surface and atmosphere?arrow_forward
- What is the smallest-diameter crater you can identify in the photo of Mercury in Figure 2 of the Concept Art: Terrestrial and Jovian Planets? (Hint: See Appendix Table A-10, Properties of the Planets, to find the radius of Mercury in kilometers for scale.)arrow_forwardHow does the solar nebula theory explain the significant density difference between the Terrestrial and Jovian planets?arrow_forwardWe believe that chains of comet fragments like Comet Shoemaker-Levy 9’s have collided not only with the jovian planets, but occasionally with their moons. What sort of features would you look for on the outer planet moons to find evidence of such collisions? (As an extra bonus, can you find any images of such features on a moon like Callisto? You can use an online site of planetary images, such as the Planetary Photojournal, at photojournal.jpl.nasa.gov.)arrow_forward
- Look at Figure 21-1. Compare temperature profiles of Venuss and Earths atmospheres. Describe the differences between the two profiles. Figure 21-1 (a) Image of Venus made from an approaching spacecraft using a UV filter designed to bring out small contrast differences in the clouds that completely hide the planets surface. None of these details would be visible to an unaided human eye. (b) The four main cloud layers in the atmosphere of Venus are more than ten times higher above the surface than ordinary Earth clouds. If you could insert thermometers into Venuss atmosphere at different levels, you would find that the lower atmosphere is much hotter than that of Earth, as indicated by the red line in the graph, but temperatures in the two planets upper atmospheres are quite similar.arrow_forwardWhat is the wavelength of the most intense radiation emitted from the surface of Mercury at high noon? In which band of the electromagnetic spectrum is that wavelength? (Hints: Use Wiens law, Eq. 7-2, and examine Figure 6-3.)arrow_forwardExplain how high-speed impacts form circular craters. How can this explanation account for the various characteristic features of impact craters?arrow_forward
- Why isnt the crust of Mars broken into mobile plates as Earths crust is? How do you know?arrow_forwardCalculate the mass of Callisto using a value for its density of 1.8 g/cm3. Convert your answer to units of kg, and compare to the mass of Ganymede given in Problem 5. (Notes: Density is mass divided by volume, and the volume of a sphere is 43r3. Necessary data are given in Appendix Table A-11.) 4. What is the escape velocity from the surface of Ganymede? Ganymedes mass is 1.5 1023 kg and its radius is 2.6 103 km. (Hint: Use the formula for escape velocity, Eq. 5-1b. The formula requires input quantities in kg and m.)arrow_forward
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