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Question 62 - Problems - Chapter 1¶Problem:¶The table below shows the masses and the diameters of the different planets in our solar system.
Out[1]:
|
DistanceSun |
OrbitalPeriod |
Mass |
Radius |
Gravity |
RotationPeriod |
PlanetName |
|
|
|
|
|
|
Mercury |
5.790000e+07 |
0.241 |
3.300000e+23 |
2439 |
0.380 |
58.600 |
Venus |
1.080000e+08 |
0.615 |
4.870000e+24 |
6052 |
0.910 |
243.000 |
Earth |
1.500000e+08 |
1.000 |
5.980000e+24 |
6378 |
1.000 |
0.997 |
Mars |
2.280000e+08 |
1.880 |
6.420000e+23 |
3393 |
0.380 |
1.026 |
Jupiter |
7.780000e+08 |
11.900 |
1.900000e+27 |
71399 |
2.530 |
0.410 |
Saturnus |
1.430000e+09 |
29.500 |
5.670000e+26 |
60000 |
1.070 |
0.430 |
Uranus |
2.870000e+09 |
84.000 |
8.700000e+25 |
25400 |
0.920 |
0.650 |
Neptunus |
4.500000e+09 |
165.000 |
1.030000e+26 |
24300 |
1.190 |
0.770 |
Pluto |
5.890000e+09 |
248.000 |
1.500000e+22 |
1500 |
0.045 |
6.390 |
Question:¶
a) Calculate the average density of each plannet and make a list of the planets in order of decreasing densities.
b) Is there a corelation between the density of the planet and the distance to the sun?
Solution:¶To calcculate density Rho, we use the formula:
$$
\textrm{Density}\;\varrho =\;\frac{\textrm{Weight}\;\left(\textrm{in}\;\textrm{kg}\right)}{\textrm{Volume}\;\left(\textrm{in}\;m^3 \right)}
$$
Therfore, we need the volume of each planet
$$
\textrm{Volume}\;v\;=\frac{4}{3}*\pi \;r^3
$$
For planet Mercury the density is 5.4 g/cm3
For planet Venus the density is 5.2 g/cm3
For planet Earth the density is 5.5 g/cm3
For planet Mars the density is 3.9 g/cm3
For planet Jupiter the density is 1.2 g/cm3
For planet Saturnus the density is 0.63 g/cm3
For planet Uranus the density is 1.3 g/cm3
For planet Neptunus the density is 1.7 g/cm3
For planet Pluto the density is 1.1 g/cm3
Out[2]:
|
DistanceSun |
OrbitalPeriod |
Mass |
Radius |
Gravity |
RotationPeriod |
Volume |
Density |
PlanetName |
|
|
|
|
|
|
|
|
Earth |
1.500000e+08 |
1.000 |
5.980000e+24 |
6378 |
1.000 |
0.997 |
1.086781e+21 |
5.502487 |
Mercury |
5.790000e+07 |
0.241 |
3.300000e+23 |
2439 |
0.380 |
58.600 |
6.077487e+19 |
5.429876 |
Venus |
1.080000e+08 |
0.615 |
4.870000e+24 |
6052 |
0.910 |
243.000 |
9.285074e+20 |
5.244977 |
Mars |
2.280000e+08 |
1.880 |
6.420000e+23 |
3393 |
0.380 |
1.026 |
1.636214e+20 |
3.923691 |
Neptunus |
4.500000e+09 |
165.000 |
1.030000e+26 |
24300 |
1.190 |
0.770 |
6.010456e+22 |
1.713680 |
Uranus |
2.870000e+09 |
84.000 |
8.700000e+25 |
25400 |
0.920 |
0.650 |
6.864197e+22 |
1.267446 |
Jupiter |
7.780000e+08 |
11.900 |
1.900000e+27 |
71399 |
2.530 |
0.410 |
1.524632e+24 |
1.246202 |
Pluto |
5.890000e+09 |
248.000 |
1.500000e+22 |
1500 |
0.045 |
6.390 |
1.413717e+19 |
1.061033 |
Saturnus |
1.430000e+09 |
29.500 |
5.670000e+26 |
60000 |
1.070 |
0.430 |
9.047787e+23 |
0.626673 |
b) Density is decresing if planets are further from the sun but not in a linear way so this can be a coincidence.
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