An Introduction to Physical Science
14th Edition
ISBN: 9781305079137
Author: James Shipman, Jerry D. Wilson, Charles A. Higgins, Omar Torres
Publisher: Cengage Learning
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Chapter 16, Problem 7MC
To determine
The physical characteristics of terrestrial planet.
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What is the range of density for the outer planets (in g/cm3)?
1.2 to 5.5
2.2 to 5.5
2.2 to 6.5
3.3 to 7.2
none of these
100%
Normal text
Arlal
12.5
| I1 1 | 2 | 3
3. Fill out this data table with information you have collected about the solar system planets.
Characteristics
Unit
Mercury
Venus
Earth
330
4,870
5,970
Mass
1024 g
61
928
1,083
Volume
1024 cm3
5.4
5.4
50
Density
g/cm3
58
106 km
100
100
Distance from Sun
Radius
km
Crust Thickness
km
Atmosphere Height
km
Fill out this data table with information you have collected about the solar system planets.
Characteristics
Unit
Mercury
Venus
Earth
330
10 g
4,870
5,970
Mass
61
928
1,083
Volume
1024 cm
5.4
5.4
50
Density
g/cm
Distance from Sun
58
10° km
100
100
Radius
km
Crust Thickness
km
Atmosphere Height
km
Axial Tilt
degrees
Force of Gravity on
a1 kg test mass
N
Length of Day
4223
4,223
88
hours
225
365
Length of Orbit
Earth days 88
167
464
15
Mean Temperature
° C
ТЕВОС
Mars
Jupiter
Saturn
Uranus
Neptune
102,000
642
| 1,898,000
568.000
86,800
Chapter 16 Solutions
An Introduction to Physical Science
Ch. 16.1 - What is the difference between the geocentric...Ch. 16.1 - Prob. 2PQCh. 16.1 - Calculate the period of a planet whose orbit has a...Ch. 16.2 - Prob. 1PQCh. 16.2 - Prob. 2PQCh. 16.3 - Which has the greater albedo, the Earth or the...Ch. 16.3 - Prob. 2PQCh. 16.4 - What makes a planet terrestrial, or pertaining to...Ch. 16.4 - What is the most abundant molecule in the...Ch. 16.5 - Prob. 1PQ
Ch. 16.5 - Prob. 2PQCh. 16.6 - Prob. 1PQCh. 16.6 - Prob. 2PQCh. 16.7 - Prob. 1PQCh. 16.7 - Prob. 2PQCh. 16.8 - Prob. 1PQCh. 16.8 - Prob. 2PQCh. 16 - Prob. AMCh. 16 - Prob. BMCh. 16 - Prob. CMCh. 16 - Prob. DMCh. 16 - Prob. EMCh. 16 - Prob. FMCh. 16 - Prob. GMCh. 16 - Prob. HMCh. 16 - Prob. IMCh. 16 - Prob. JMCh. 16 - Prob. KMCh. 16 - Prob. LMCh. 16 - Prob. MMCh. 16 - Prob. NMCh. 16 - Prob. OMCh. 16 - Prob. PMCh. 16 - Prob. QMCh. 16 - Prob. RMCh. 16 - Prob. SMCh. 16 - Prob. TMCh. 16 - Prob. UMCh. 16 - Prob. VMCh. 16 - Prob. WMCh. 16 - Prob. XMCh. 16 - Prob. 1MCCh. 16 - Which of Keplers laws gives the most direct...Ch. 16 - Which of Keplers laws gives an indication of the...Ch. 16 - Prob. 4MCCh. 16 - Which of the following is abundant on the Earth...Ch. 16 - Prob. 6MCCh. 16 - Prob. 7MCCh. 16 - Which of the following statements concerning the...Ch. 16 - Which of the following is not a physical...Ch. 16 - What are the primary constituents of the Jovian...Ch. 16 - Which of the following is not a physical...Ch. 16 - Which planet has a ring system made of mostly...Ch. 16 - Which Jovian planet revolves on its side and has...Ch. 16 - Which one of the following criteria disqualifies...Ch. 16 - Which statement about the dwarf planet Ceres is...Ch. 16 - Prob. 16MCCh. 16 - Prob. 17MCCh. 16 - Which of the following is not a very useful method...Ch. 16 - ___ is the study of the universe. (Intro)Ch. 16 - Prob. 2FIBCh. 16 - Prob. 3FIBCh. 16 - Prob. 4FIBCh. 16 - Prob. 5FIBCh. 16 - Prob. 6FIBCh. 16 - Prob. 7FIBCh. 16 - The albedo of the Earth is about ___. (16.3)Ch. 16 - Prob. 9FIBCh. 16 - Prob. 10FIBCh. 16 - Prob. 11FIBCh. 16 - Prob. 12FIBCh. 16 - The Jovian planet with retrograde rotation is ___....Ch. 16 - Prob. 14FIBCh. 16 - Prob. 15FIBCh. 16 - Prob. 16FIBCh. 16 - Prob. 17FIBCh. 16 - Prob. 1SACh. 16 - What is the main difference between the...Ch. 16 - Prob. 3SACh. 16 - Prob. 4SACh. 16 - Describe the orientation and the shape of the...Ch. 16 - Prob. 6SACh. 16 - Prob. 7SACh. 16 - Prob. 8SACh. 16 - Prob. 9SACh. 16 - Prob. 10SACh. 16 - Prob. 11SACh. 16 - Prob. 12SACh. 16 - Explain the differences between the Grand Canyon...Ch. 16 - Prob. 14SACh. 16 - Prob. 15SACh. 16 - Which planets axis of rotation is a peculiarity,...Ch. 16 - Prob. 17SACh. 16 - Prob. 18SACh. 16 - Why is Pluto not considered a major planet, and...Ch. 16 - Prob. 20SACh. 16 - Prob. 21SACh. 16 - What was the major influence in the formation of...Ch. 16 - What is astrometry?Ch. 16 - Prob. 24SACh. 16 - Prob. 1VCCh. 16 - Give some reasons our knowledge of the solar...Ch. 16 - A Foucault pendulum suspended from the ceiling of...Ch. 16 - Prob. 3AYKCh. 16 - Explain how the scientific method was used to...Ch. 16 - How does the solar nebula theory explain the...Ch. 16 - Calculate the period T of a planet whose orbit has...Ch. 16 - Calculate the period T of a dwarf planet whose...Ch. 16 - Calculate the length R of the semimajor axis of a...Ch. 16 - Calculate the length R of the semimajor axis of a...Ch. 16 - Determine what the period of revolution of the...Ch. 16 - Determine what the period of revolution of the...Ch. 16 - Asteroids are believed to be material that never...Ch. 16 - Show that the asteroid belt lies between Mars and...Ch. 16 - Use Keplers third law to show that the closer a...Ch. 16 - Prob. 10ECh. 16 - Prob. 11ECh. 16 - List the Jovian planets in order of increasing...
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- What are the primary constituents of the Jovian planets? (16.5) (a) hydrogen and helium (b) hydrogen and carbon dioxide (c) methane and oxygen (d) nitrogen and oxygenarrow_forwardDescribe the solar nebula, and outline the sequence of events within the nebula that gave rise to the planetesimals.arrow_forwardQuestion #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 e Education TM Inc. RK12arrow_forward
- What are two differences between the terrestrial (rocky) planets and the Gas giants?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_forwardMiller’s Planet part I: This planet is described as having 130% Earth gravity What is the acceleration due to gravity on the surface of this planet? 7 m/s2 130 m/s2 13 m/s2 Miller’s Planet part II: What is the source of the waves on this planet? Wind Tidal stress due to proximity of Gargantua Plate tectonic driven Miller-quakes Miller’s Planet Part III: Why would it be unlikely that this planet could sustain an atmosphere let alone liquid water on its surface. Gargantua’s accretion disk likely emits X-rays, UV rays and possibly gamma radiation Miller’s planet’s surface gravity is too small Miller’s planet has no magnetic fieldarrow_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_forwardThe cores of terrestrial planets are mostly metal because: The entire planets are mostly metal Metals are denser and so sank to the centres of planets when they were still molten Metals condensed first in the formation of the Solar System Radioactivity created metals in the core of planets from the decay of uraniumarrow_forwardWhat is the difference between a planetesimal and a protoplanet?arrow_forward
- Describe four characteristics in common among all four Jovian planets. (Hint: Review Celestial Profiles for all of these planets.)arrow_forwardDescribe the four stages of Terrestrial planet development.arrow_forwardWhy is Pluto not considered a major planet, and what other peculiarity distinguishes it from the major planets?arrow_forward
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