Physical Science
11th Edition
ISBN: 9780077862626
Author: Bill Tillery, Stephanie J. Slater, Timothy F. Slater
Publisher: McGraw-Hill Education
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Textbook Question
Chapter 15, Problem 2QFT
What are the basic differences between the terrestrial planets and the giant planets? Describe how the protoplanet nebular model accounts for these differences.
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What is the frost line in the solar nebula? Explain how temperature differences led to the formation of two distinct types of planets.
Compare and contrast the terrestrial planets to the gas giant planets. Be sure to include differences in size, density, and any special information about any of the planets.
Question #4:
According to the nebular theory, which planet is most likely to be
gaseous rather than rocky?
A. Venus, because it is the warmest planet and so is more likely
to be gaseous
B. Mercury, because planets closer to the solar nebula are more
likely to be made of gas, like the nebula
C. Earth, because the atmosphere consists of nitrogen, oxygen,
and other gases, so it is a gaseous planet
D. Neptune, because as the planets get farther from the solar
nebula, their composition is more icy and gaseous
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Chapter 15 Solutions
Physical Science
Ch. 15 -
1. The mass of the Sun is how much larger than...Ch. 15 -
2. The distance from Earth to the Sun is called a...Ch. 15 -
3. What type of planets are Mercury, Venus,...Ch. 15 -
4. Which of the following is most likely found on...Ch. 15 -
5. What is the outermost...Ch. 15 -
6. The planet that was named after the mythical...Ch. 15 -
7. A day on which planet is longer than a year on...Ch. 15 -
8. The day on which planet is about the same time...Ch. 15 -
9. Mars has distinct surface feature-related...Ch. 15 -
10. How many moons orbit...
Ch. 15 -
11. What is the largest planet in our solar...Ch. 15 -
12. Callisto, Europa, Ganymede, and Io...Ch. 15 -
13. The density of Jupiter is
a. 50 percent...Ch. 15 -
14. The only moon in the solar system with a...Ch. 15 -
15. Saturn’s rings are thought to be
a. composed...Ch. 15 -
16. The planet with the lowest average density,...Ch. 15 -
17. The planet that is not a giant...Ch. 15 -
18. What planets are considered...Ch. 15 -
19. Area of the solar system where long-period...Ch. 15 -
20. Short-period comets have orbital periods...Ch. 15 -
21. Remnants of comets and asteroids found in...Ch. 15 -
22. Meteorites are classified into all of the...Ch. 15 -
23. The most widely accepted theory on the origin...Ch. 15 -
24. The belt of asteroids between Mars and...Ch. 15 -
25. Which of the following planets would be...Ch. 15 -
26. Which of the following planets probably still...Ch. 15 -
27. Venus appears the brightest when it is in...Ch. 15 -
28. The small body with a composition and...Ch. 15 -
29. A small body from space that falls on the...Ch. 15 -
30. Planets in our solar system are classified...Ch. 15 -
31. What separates the terrestrial planets from...Ch. 15 -
32. The planet that has the shortest “year” among...Ch. 15 -
33. What planet is called the morning star and...Ch. 15 -
34. Venus “shines” because it is
a. composed of...Ch. 15 -
35. On Venus, the sun rises in the west. This is...Ch. 15 -
36. The “sister” planet to Earth...Ch. 15 -
37. What feature on Mars was considered by some...Ch. 15 -
38. Jupiter radiates twice as much energy as it...Ch. 15 -
39. The Great Red Spot is thought to be
a. a...Ch. 15 -
40. The metallic hydrogen that surrounds the core...Ch. 15 -
41. A shooting star is a...Ch. 15 -
1. Describe the protoplanet nebular model of the...Ch. 15 -
2. What are the basic differences between the...Ch. 15 -
3. Describe the surface and atmospheric...Ch. 15 -
4. What evidence exists that Mars at one time had...Ch. 15 -
5. Describe the internal structure of Jupiter and...Ch. 15 -
6. What are the rings of Saturn?
Ch. 15 -
7. Describe some of the unusual features found on...Ch. 15 -
8. What are the similarities and the differences...Ch. 15 -
9. Give one idea about why the Great Red Spot...Ch. 15 -
10. What is so unusual about the motions and...Ch. 15 -
11. What evidence exists today that the number of...Ch. 15 -
12. Using the properties of the planets other...Ch. 15 -
13. What are “shooting stars”? Where do they come...Ch. 15 -
14. What is an asteroid? What evidence indicates...Ch. 15 -
15. Where do comets come from? Why are...Ch. 15 -
16. What is a meteor? What is the most likely...Ch. 15 -
17. What is a meteorite? What is the most likely...Ch. 15 -
18. Technically speaking, what is wrong with...Ch. 15 -
19. What are the primary differences between the...Ch. 15 -
1. What are the significant similarities and...Ch. 15 - Prob. 2FFACh. 15 -
3. Evaluate the statement that Venus is Earth's...Ch. 15 -
4. Describe the possibility and probability of...Ch. 15 -
5. Provide arguments that Pluto should be...Ch. 15 -
6. Explain why is it difficult to count the...Ch. 15 - Prob. 1IICh. 15 -
1. Based on the density and diameter in km...Ch. 15 - Prob. 2PEBCh. 15 -
3. A scale model of the solar system is being...Ch. 15 -
4. How many times has Uranus rotated on its axis...Ch. 15 -
5. An elementary school class is building a scale...Ch. 15 -
6. A class is building scale models of the...Ch. 15 - Prob. 7PEBCh. 15 -
8. A 1 cm thick piece of lead with a surface area...Ch. 15 -
9. Assume an astronaut at a space station on Mars...Ch. 15 -
10. What is the mass of the Sun, in kilograms,...Ch. 15 -
11. What is the mass of the Sun, in kilograms,...Ch. 15 -
12. Based on Kepler’s third law, what is the...Ch. 15 -
13. Based on Kepler’s third law, what is the...Ch. 15 - Prob. 14PEBCh. 15 -
15. Assuming a circular orbit, what is the...
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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
- Describe the solar nebula, and outline the sequence of events within the nebula that gave rise to the planetesimals.arrow_forwardExplain our ideas about why the terrestrial planets are rocky and have less gas than the giant planets.arrow_forwardPresent 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_forward
- Order the following steps in the formation of a Terrestrial planet chronologically: gravitational collapse, accretion, out-gassing, condensation, and differentiation.arrow_forwardWhere would you look for some “original” planetesimals left over from the formation of our solar system?arrow_forwardGiven what you've learned about the solar nebula idea, what do you believe the likelihood is of discovering livable planets in other solar systems? Learn more about this search by visiting NASA's Kepler mission and writing a half-page overview of the project.arrow_forward
- 1. Which of the outer planets have compositions dominated by the "ices" ingredient? Check the correct two. 2. Which of the outer planets have compositions dominated by the "gases" ingredient? Check the correct two. 3. Most of the spaceflight missions to the outer planets have been flyby missions, but two of them were orbiters. Which of these two spacecraft orbited giant planets? Check the correct two. (Hint: An orbiter might do a flyby of one planet and then go on to orbit a different planet.) 4. Jupiter's mass is how many times larger than the Earth's? Just type a number, no words or any other extra stuff. 5. Which of the outer planets has extreme seasons, with its rotational axis being tilted so much that it is practically in the plane of its orbit?arrow_forwardWhich is these facts is NOT explained by the nebular theory? There are two main types of planets: terrestrial and jovian Existance of comets and asteroids Planets orbit in the same direction and plane Number of planets of each type (4 terrestrial and 4 jovian)arrow_forwardWe think the terrestrial planets formed around solid “seeds” that later grew over time through the accretion of rocks and metals. a) Suppose the Earth grew to its present size in 1 million years through the accretion of particles averaging 100 grams each. On average, how many particles did the Earth capture per second, given that the mass of the Earth is = 5.972 × 10 ^24 kg ? b) If you stood on Earth during its formation and watched a region covering 100 m^2, how many impacts would you expect to see in one hour. Use the impact rate you calculated in part a. You’ll need the following as well: the radius of the Earth is = 6.371 × 10 ^6 m and the surface area of the Earth is 4??^2Eartharrow_forward
- Which of the following statements is correct? a. The formation of planets stopped because the solar nebula got cooler c. The formation of planets stopped because the solar nebula ran out of planetesimals d. The formation of planets stopped because the solar nebula spinning was slowing down e. The formation of planets stopped because the young Sun's strong solar wind swept away material not yet accreted onto the planetsarrow_forwardHow many impacts would you expect to strike a 100m2 region in one hour during Earth’s formation, assuming that Earth grew to its present size in 10 million years from particles averaging 100 grams each? (Hint: Assume that Earth had its current radius of 6378km.) (Notes: The surface area of a sphere is 4pir2 ; 1yr=3.2x107 .) a. About 1300. b. About 13 . c. About 13,000. d. About 130arrow_forwardGiven what you know about the solar nebula theory, how likely is it that additional solar systems will yield inhabited planets? Visit NASA's Kepler mission and write a half-page description of the project.arrow_forward
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