Table 15.2 Planetary Data Mean Distance from Sun Orbital Velocity Planet 1 Planet 2 Planet 3 1.2 15,000 52,000 1.4 4.8 0.01 Millions of Millions of Inclination of Relative Mass (Earth = 1) Diameter (km) Mean Distance from Star (AU) Density (g/cm3) Orbital Eccentricity 15 0.1 5000 35 5.3 0.23 Planet Symbol AU* Miles Kilometers Orbital Period Orbit mi's km/s Mercury 0.39 36 58 88 days 7°00' 29.5 47.5 17 1.22 0.05 우 245 days Venus 0.72 67 108 3°24' 21.8 35.0 Earth 1.00 93 150 365.25 days 0°0' 18.5 29.8 Mars 1.52 142 248 687 days 1°51 14.9 24.1 Jupiter 24 12 years 5.20 483 778 1°18' 8.1 13.1 Saturn 9.54 886 1427 30 years 2°29' 6.0 9.6 Uranus 19.18 1783 2870 84 years 0°46' 4.2 6.8 Neptune 30.06 2794 4497 165 years 1°46' 3.3 5.3 Diameter Period of Rotation Relative Mass Average Density (g/cm³) Flattening (%) | Eccentricity* Polar Number of Known Planet Around Axis Miles Kilometers (Earth = 1) Satellitestt Mercury 59 days 3015 4878 0.06 5.4 0.0 0.206 Venus 243 days 7526 12,104 0.82 5.2 0.0 0.007 Earth 23h56m045 7920 12,756 1.00 5.5 0.3 0.017 1 Mars 24h37m235 4216 6794 0.11 3.9 0.5 0.093 2 Jupiter gh56m 88,700 143,884 317.87 1.3 6.7 0.048 67 Saturn 10 30m 75,000 120,536 95.14 0.7 10.4 0.056 62 Uranus 17h14m 29,000 51,118 14.56 1.2 2.3 0.047 27 Neptune 16*07m 28,900 50,530 17.21 1.7 1.8 0.009 14 *AU = astronomical unit, Earth's mean distance from the Sun. 'Eccentricity is a measure of the amount an orbit deviates from a circular shape. The larger the number, the less circular the orbit. fIncludes all satellites discovered as of July 2015. Satellites are celestial bodies that orbit a planet rather than orbiting a star like the Sun.

Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
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Question

Assume that a solar system has been discovered in a nearby region of
the Milky Way Galaxy. The accompanying table shows data that have
been gathered about three of the planets orbiting the central star of
this newly discovered solar system. Using Table 15.2 as a guide, classify
each planet as Jovian, terrestrial, or neither. Explain your reasoning. 

Table 15.2 Planetary Data
Mean Distance from Sun
Orbital Velocity
Planet 1 Planet 2 Planet 3
1.2
15,000 52,000
1.4
4.8
0.01
Millions of
Millions of
Inclination of
Relative Mass (Earth = 1)
Diameter (km)
Mean Distance from Star (AU)
Density (g/cm3)
Orbital Eccentricity
15
0.1
5000
35
5.3
0.23
Planet
Symbol
AU*
Miles
Kilometers
Orbital Period
Orbit
mi's
km/s
Mercury
0.39
36
58
88 days
7°00'
29.5
47.5
17
1.22
0.05
우
245 days
Venus
0.72
67
108
3°24'
21.8
35.0
Earth
1.00
93
150
365.25 days
0°0'
18.5
29.8
Mars
1.52
142
248
687 days
1°51
14.9
24.1
Jupiter
24
12 years
5.20
483
778
1°18'
8.1
13.1
Saturn
9.54
886
1427
30 years
2°29'
6.0
9.6
Uranus
19.18
1783
2870
84 years
0°46'
4.2
6.8
Neptune
30.06
2794
4497
165 years
1°46'
3.3
5.3
Diameter
Period of Rotation
Relative Mass
Average
Density (g/cm³) Flattening (%) | Eccentricity*
Polar
Number of Known
Planet
Around Axis
Miles
Kilometers
(Earth = 1)
Satellitestt
Mercury
59 days
3015
4878
0.06
5.4
0.0
0.206
Venus
243 days
7526
12,104
0.82
5.2
0.0
0.007
Earth
23h56m045
7920
12,756
1.00
5.5
0.3
0.017
1
Mars
24h37m235
4216
6794
0.11
3.9
0.5
0.093
2
Jupiter
gh56m
88,700
143,884
317.87
1.3
6.7
0.048
67
Saturn
10 30m
75,000
120,536
95.14
0.7
10.4
0.056
62
Uranus
17h14m
29,000
51,118
14.56
1.2
2.3
0.047
27
Neptune
16*07m
28,900
50,530
17.21
1.7
1.8
0.009
14
*AU = astronomical unit, Earth's mean distance from the Sun.
'Eccentricity is a measure of the amount an orbit deviates from a circular shape. The larger the number, the less circular the orbit.
fIncludes all satellites discovered as of July 2015. Satellites are celestial bodies that orbit a planet rather than orbiting a star like the Sun.
Transcribed Image Text:Table 15.2 Planetary Data Mean Distance from Sun Orbital Velocity Planet 1 Planet 2 Planet 3 1.2 15,000 52,000 1.4 4.8 0.01 Millions of Millions of Inclination of Relative Mass (Earth = 1) Diameter (km) Mean Distance from Star (AU) Density (g/cm3) Orbital Eccentricity 15 0.1 5000 35 5.3 0.23 Planet Symbol AU* Miles Kilometers Orbital Period Orbit mi's km/s Mercury 0.39 36 58 88 days 7°00' 29.5 47.5 17 1.22 0.05 우 245 days Venus 0.72 67 108 3°24' 21.8 35.0 Earth 1.00 93 150 365.25 days 0°0' 18.5 29.8 Mars 1.52 142 248 687 days 1°51 14.9 24.1 Jupiter 24 12 years 5.20 483 778 1°18' 8.1 13.1 Saturn 9.54 886 1427 30 years 2°29' 6.0 9.6 Uranus 19.18 1783 2870 84 years 0°46' 4.2 6.8 Neptune 30.06 2794 4497 165 years 1°46' 3.3 5.3 Diameter Period of Rotation Relative Mass Average Density (g/cm³) Flattening (%) | Eccentricity* Polar Number of Known Planet Around Axis Miles Kilometers (Earth = 1) Satellitestt Mercury 59 days 3015 4878 0.06 5.4 0.0 0.206 Venus 243 days 7526 12,104 0.82 5.2 0.0 0.007 Earth 23h56m045 7920 12,756 1.00 5.5 0.3 0.017 1 Mars 24h37m235 4216 6794 0.11 3.9 0.5 0.093 2 Jupiter gh56m 88,700 143,884 317.87 1.3 6.7 0.048 67 Saturn 10 30m 75,000 120,536 95.14 0.7 10.4 0.056 62 Uranus 17h14m 29,000 51,118 14.56 1.2 2.3 0.047 27 Neptune 16*07m 28,900 50,530 17.21 1.7 1.8 0.009 14 *AU = astronomical unit, Earth's mean distance from the Sun. 'Eccentricity is a measure of the amount an orbit deviates from a circular shape. The larger the number, the less circular the orbit. fIncludes all satellites discovered as of July 2015. Satellites are celestial bodies that orbit a planet rather than orbiting a star like the Sun.
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