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Lunar atmosphere measurements.Cold cathode ionization gauges were left on the lunar surface during Apollo missions 14 and 15 to measure the amount of lunar gas. The observed nighttime concentration is very low, about 200,000 per cu cm, which is less than the neon concentration that might be expected from the solar wind. This suggests that the lunar surface is not saturated with solar wind neon, and hence that less neon is being released from the surface than impinges upon it. The low nighttime concentration shows that contaminant gases from the Apollo operations freeze out at night or become adsorbed on the cold lunar surface. Observed daytime concentrations have been two orders of magnitude greater than the nighttime values and appear to be due mainly to contamination in the landing area. The rate at which the contamination is decreasing is characterized by a time constant of a few months. Gas clouds have been seen at times and these appear to have been released from Apollo hardware left on the lunar surface.
Document ID
19730035028
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Johnson, F. S.
Carroll, J. M.
(Texas, University Dallas, Tex., United States)
Evans, D. E.
(NASA Manned Spacecraft Center Houston, Tex., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1972
Subject Category
Space Sciences
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: January 10, 1972
End Date: January 13, 1972
Accession Number
73A19830
Funding Number(s)
CONTRACT_GRANT: NAS9-5964
Distribution Limits
Public
Copyright
Other

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