Difference between revisions of "Argon"

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Most of the volatiles have been deposited in the top layers of the Moon's surface by the solar wind over geologic time. A notable exception to this is Argon. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of Potassium and/or Krypton deep within the lunar mantle or core, and that the Argon-40 seeps out to the surface via fissures. This vented Argon enter the [[lunar atmosphere]]; then the Argon is implanted into the [[regolith]] by interactions with ions from the solar wind.  
 
Most of the volatiles have been deposited in the top layers of the Moon's surface by the solar wind over geologic time. A notable exception to this is Argon. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of Potassium and/or Krypton deep within the lunar mantle or core, and that the Argon-40 seeps out to the surface via fissures. This vented Argon enter the [[lunar atmosphere]]; then the Argon is implanted into the [[regolith]] by interactions with ions from the solar wind.  
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Public domain info obtained from NASA:
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 +
Moon Fact Sheet
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http://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html
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Lunar Atmosphere Estimated Composition (particles per cubic cm):
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Helium 4 (4He) - 40,000
 +
Neon 20 (20Ne) - 40,000
 +
Hydrogen (H2) - 35,000
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Argon 40 (40Ar) - 30,000
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Neon 22 (22Ne) - 5,000
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Argon 36 (36Ar) - 2,000
  
 
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Revision as of 06:13, 31 August 2007

Argon
Ar
In situ availability:
Necessity:
Atomic number: 18
Atomic mass: 39.948
group: 18
period: 3
normal phase: Gas
series: Noble gases
density: 1.784 g/L
melting point: 83.80K,
-189.35°C,
-308.83°F
boiling point: 87.30K,
-185.85°C,
-302.53°F
FNeN/A
Cl ← Ar → K
BrKrN/A
Atomic radius (pm): 71
Bohr radius (pm): 71
Covalent radius (pm): 97
Van der Waals radius (pm): 188
ionic radius (pm): -
1st ion potential (eV): 15.76
Electron Configuration
1s2
2s2 2p6
3s2 3p6
Electrons Per Shell
2, 8, 8
Electronegativity:
Electron Affinity: Unstable anion
Oxidation states: -
Magnetism: Nonmagnetic
Crystal structure: Face centered cubic

Argon is a Noble gas in group 18. It has a Face centered cubic crystalline structure. This element has 3 stable isotopes: 36, 38, and 40.

Most of the volatiles have been deposited in the top layers of the Moon's surface by the solar wind over geologic time. A notable exception to this is Argon. the concentration of Argon in lunar soil is much higher than found in the solar wind, so must come from a different source. Especially, the isotope Argon-40. It is presently believed that the Argon-40 comes from radioactive decay of Potassium and/or Krypton deep within the lunar mantle or core, and that the Argon-40 seeps out to the surface via fissures. This vented Argon enter the lunar atmosphere; then the Argon is implanted into the regolith by interactions with ions from the solar wind.

Public domain info obtained from NASA:

Moon Fact Sheet

http://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html

Lunar Atmosphere 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


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