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Revision 7 as of 2015-10-13 04:56:38
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|| speed || C || H energy || Pressure ||
|| m
/s || || || Pa     ||
|| 25k || 8e-5 || 4 eV ||
||
|| 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 in Local Cloud ||
|| 100M || 0.33 || 50 MeV || 500 || high energy van Allen belt   ||
||
200M || 0.67 || 380 MeV || 4K || relativistic ||
|| 250M || 0.83 || 500 MeV || 26K || 11 KW/m^2^ particle power in Local Cloud ||
|| 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 || 500&mu; || ||
|| 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

https://upload.wikimedia.org/wikipedia/commons/7/74/Local_Interstellar_Clouds_with_motion_arrows.jpg

InterstellarMedium (last edited 2015-10-14 02:24:00 by KeithLofstrom)