Difference between revisions of "Lunar Atmosphere"
(lunar outgassing events.) |
(adding superscripts) |
||
| (4 intermediate revisions by one other user not shown) | |||
| Line 8: | Line 8: | ||
Diurnal temperature range: >100 K to <400 K (roughly -250 F to +250 F) | Diurnal temperature range: >100 K to <400 K (roughly -250 F to +250 F) | ||
Total mass of atmosphere: ~25,000 kg | Total mass of atmosphere: ~25,000 kg | ||
| − | Surface pressure (night): 3 x 10-15 bar (2 x 10-12 torr) | + | Surface pressure (night): 3 x 10<sup>-15</sup> bar (2 x 10<sup>-12</sup> torr) |
| − | Abundance at surface: 2 x | + | Abundance at surface: 2 x 10<sup>5</sup> particles/cm3 |
Estimated Composition (particles per cubic cm): | Estimated Composition (particles per cubic cm): | ||
| Line 31: | Line 31: | ||
Although the Moon is relatively inert geologically, the lunar atmosphere continues to replenished by [[lunar outgassing]] events. | Although the Moon is relatively inert geologically, the lunar atmosphere continues to replenished by [[lunar outgassing]] events. | ||
| + | |||
| + | == See also == | ||
| + | |||
| + | [[Lunar Settlement Artifical Atmosphere]] | ||
[[Category:Mining]] | [[Category:Mining]] | ||
Latest revision as of 13:50, 19 October 2011
Public domain info obtained from NASA:
Moon Fact Sheet
http://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html
Lunar Atmosphere Diurnal temperature range: >100 K to <400 K (roughly -250 F to +250 F) Total mass of atmosphere: ~25,000 kg Surface pressure (night): 3 x 10-15 bar (2 x 10-12 torr) Abundance at surface: 2 x 105 particles/cm3
Estimated Composition (particles per cubic cm):
- Helium 4 (4He) - 40,000
- Neon 20 (20Ne) - 40,000
- Hydrogen (H2) - 35,000
- Argon 40 (40Ar) - 30,000
- Neon 22 (22Ne) - 5,000
- Argon 36 (36Ar) - 2,000
- Methane - 1000
- Ammonia - 1000
- Carbon Dioxide (CO2) - 1000
Trace Oxygen (O+), Aluminum (Al+), Silicon (Si+) Possible Phosphorus (P+), Sodium (Na+), Magnesium (Mg+)
Composition of the tenuous lunar atmosphere is poorly known and variable, these are estimates of the upper limits of the nighttime ambient atmosphere composition. Daytime levels were difficult to measure due to heating and outgassing of Apollo surface experiments.
Although the Moon is relatively inert geologically, the lunar atmosphere continues to replenished by lunar outgassing events.
