|
Size: 2671
Comment:
|
Size: 2853
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 9: | Line 9: |
|| speed || C || H energy ||<-2> Conditions in Local Cloud || || m/s || || || Pressure || || 25k || 8e-5 || 4 eV || Pascals || || 30k || 1e-4 || 5 eV || || || 100k || 3e-4 || 50 eV || || || 300k || 1e-3 || 500 eV || || || 1M || 3e-3 || 5 keV || 500μ || || 1.4M || 5e-3 || 10 keV || || low energy ion implantation || || 3M || 1e-2 || 50 keV || 1.4m || low energy van Allen belt || || 10M || 3e-2 || 500 keV || 0.5 || high energy ion implantation || || 30M || 0.10 || 5 MeV || 14 || 7 W/m^2^ particle power || || 100M || 0.33 || 50 MeV || 500 || || || 200M || 0.67 || 380 MeV || 4K || highest energy van Allen belt, 1e12 more flux || || 250M || 0.83 || 500 MeV || 26K || 11 KW/m^2^ particle power || |
|| speed || C || H energy ||<-3> Conditions in Local Cloud, 3e5 H/m^3^ || || m/s || || || flux || Pressure || || || 25k || 8e-5 || 4 eV || H/s-m^2^ || Pascals || || || 30k || 1e-4 || 5 eV || || || || || 100k || 3e-4 || 50 eV || || || || || 300k || 1e-3 || 500 eV || || || || || 1M || 3e-3 || 5 keV || 3e11 || 500μ || || || 1.4M || 5e-3 || 10 keV || || || low energy ion implantation || || 3M || 1e-2 || 50 keV || || 1.4m || low energy van Allen belt || || 10M || 3e-2 || 500 keV || 3e12 || 0.5 || high energy ion implantation || || 30M || 0.10 || 5 MeV || || 14 || 7 W/m^2^ particle power || || 100M || 0.33 || 50 MeV || || 500 || || || 200M || 0.67 || 380 MeV || 6e13 || 4K || highest energy van Allen belt, 1e12 more flux || || 250M || 0.83 || 500 MeV || || 26K || 11 KW/m^2^ particle power || |
Star Travel and the Interstellar Medium particle effects
The interstellar medium - the coronal gas - forms a column between locations in space. The sun is 4 light years from one edge of a 60 light-year-across cloud with a density of 0.3 hydrogens per cubic centimeter, or 3e5 H/m3, encountering the sun as it moves towards Scorpio at 25 km/s. Around that cloud is the Local Bubble, 300 LY across with a density of 50 H/m3. A light year is 9.5e15 meters, so for the first 4 light years in one direction, and more than 50 LY in the opposite direction, we encounter a column of hydrogen atoms with a density of about 1e21 H/m2-LY. That is the density of a layer of liquid water 30 nm thick per light year. 100 light years, 3 micrometers.
These protons will implant themselves in the surface of any object passing through them. At a mere 25 km/s, the energy per proton is 3.6 electron volts - many will bounce off. Approaching the speed of light, the energy approaches multiples of the mass energy of the proton, 938 MeV/c2. That will damage solid structure to the implant depth.
I don't know how much. A particle physicist can tell you how deep.
speed |
C |
H energy |
Conditions in Local Cloud, 3e5 H/m3 |
||
m/s |
|
|
flux |
Pressure |
|
25k |
8e-5 |
4 eV |
H/s-m2 |
Pascals |
|
30k |
1e-4 |
5 eV |
|
|
|
100k |
3e-4 |
50 eV |
|
|
|
300k |
1e-3 |
500 eV |
|
|
|
1M |
3e-3 |
5 keV |
3e11 |
500μ |
|
1.4M |
5e-3 |
10 keV |
|
|
low energy ion implantation |
3M |
1e-2 |
50 keV |
|
1.4m |
low energy van Allen belt |
10M |
3e-2 |
500 keV |
3e12 |
0.5 |
high energy ion implantation |
30M |
0.10 |
5 MeV |
|
14 |
7 W/m2 particle power |
100M |
0.33 |
50 MeV |
|
500 |
|
200M |
0.67 |
380 MeV |
6e13 |
4K |
highest energy van Allen belt, 1e12 more flux |
250M |
0.83 |
500 MeV |
|
26K |
11 KW/m2 particle power |
