|
Size: 2623
Comment:
|
Size: 2986
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 7: | Line 7: |
| ||<-2> ||<-3> Velocity km/s || || Object || Mass kg || Orbit || Escape || Center || Temp K || Composition || |
||<-2> ||<:-3> Velocity km/s || ||<:> Object || Mass kg || Orbit || Escape || Center || Temp K || Composition || |
| Line 11: | Line 11: |
| || Asteroids || 3.xxe19 || 16-20 || < 0.51 || 16-20 || 85-270 || some iron, silicates || | ||<)> Asteroids || 3.xxe19 || 16-20 || < 0.51 || 16-20 || 85-270 || some iron, silicates || ||''' Jupiter '''|| 1.90e27 || 13.1 || 59.5 || 74.0 || 112+ || H, He, some core rock || ||<)> Callisto || 1.08e23 || 8.2 || 2.0 || 15.6 || 80-165 || H₂O and rock || |
| Line 13: | Line 15: |
| || Titan || 1.34e23 || 5.6 || 2.6 || 11.6 || 94 || H₂O and rock || | ||<)> Titan || 1.34e23 || 5.6 || 2.6 || 11.6 || 94 || H₂O and rock || |
| Line 15: | Line 17: |
| || Titania || 3.53e21 || | ||<)> Titania || 3.53e21 || 3.6 || 0.8 || 7.8 || 60-89 || H₂O, organics, rock || |
| Line 17: | Line 19: |
| || Triton || 2.14e22 || 4.4 || 1.5 || 7.2 || 38 || H₂O and rock || | ||<)> Triton || 2.14e22 || 4.4 || 1.5 || 7.2 || 38 || H₂O and rock || |
| Line 19: | Line 21: |
| The energy to escape from the center of the planet is 1.5 times the surface escape velocity, assuming (incorrectly) uniform density. | The energy to escape from the center of the planet is 1.5 times the surface escape velocity, assuming (incorrectly) uniform density. "Center" is the escape velocity from the center of the planet to solar escape. |
Stady Materials
Materials in solar system for Stapledon-Dyson Static-Dynamic 50 AU Shell, 60K
Source Planets and Moons
|
Velocity km/s |
|||||
Object |
Mass kg |
Orbit |
Escape |
Center |
Temp K |
Composition |
Mercury |
3.30e23 |
47.4 |
4.25 |
47.7 |
85-700 |
iron core, silicate mantle |
Venus |
4.87e24 |
35.0 |
10.4 |
37.3 |
737 |
? |
Asteroids |
3.xxe19 |
16-20 |
< 0.51 |
16-20 |
85-270 |
some iron, silicates |
Jupiter |
1.90e27 |
13.1 |
59.5 |
74.0 |
112+ |
H, He, some core rock |
Callisto |
1.08e23 |
8.2 |
2.0 |
15.6 |
80-165 |
H₂O and rock |
Saturn |
5.68e26 |
9.7 |
35.5 |
44.5 |
84-134 |
H, He, some core rock |
Titan |
1.34e23 |
5.6 |
2.6 |
11.6 |
94 |
H₂O and rock |
Uranus |
8.68e25 |
6.8 |
21.3 |
27.0 |
47-76 |
H, He, 2.3% methane |
Titania |
3.53e21 |
3.6 |
0.8 |
7.8 |
60-89 |
H₂O, organics, rock |
Neptune |
1.02e26 |
5.4 |
23.5 |
29.3 |
55-72 |
H, He, trace methane |
Triton |
2.14e22 |
4.4 |
1.5 |
7.2 |
38 |
H₂O and rock |
The energy to escape from the center of the planet is 1.5 times the surface escape velocity, assuming (incorrectly) uniform density. "Center" is the escape velocity from the center of the planet to solar escape.
Although the usual Dyson Sphere literature dotes on taking apart planets - particularly Earth for some reason, perhaps sociopathic authors - planets are hard, especially if the good stuff is deep inside, and not beneficiated by plate tectonics and ocean/biological chemistry. Asteroids are prefractured planetesimals, and many are threats to the Earth and ought to be removed. Uranus is better than Neptune as a source of carbon, more carbon (in methane), easier to get to, 60% more solar energy.
Abundance
Element |
ppm by weight |
Oxygen |
10,000 |
Carbon |
4,600 |
Iron |
1,000 |
Silicon |
650 |
Resistivity
https://en.wikipedia.org/wiki/Electrical_resistivity_and_conductivity
http://www.bnl.gov/magnets/Staff/Gupta/cryogenic-data-handbook/Section10.pdf
Element |
e-8 Ω-m, imprecise estimates |
Graph |
||||
|
300 K |
TC /K |
≃ 80 K |
73 K |
53 K |
60 K |
Silver |
1.6 |
|
0.33 |
0.28 |
0.15 |
0.19 |
Copper |
1.7 |
0.004 |
|
|
|
0.11 |
Aluminum |
2.8 |
0.004 |
0.28 |
0.33 |
0.20 |
0.22 |
Iron |
10.0 |
0.005 |
0.74 |
0.62 |
0.27 |
0.35 |