Computer Science
Scientific paper
Apr 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976lpsc....7..493h&link_type=abstract
In: Lunar Science Conference, 7th, Houston, Tex., March 15-19, 1976, Proceedings. Volume 1. (A77-34651 15-91) New York, Pergamon
Computer Science
Atmospheric Models, Carbon, Ion Implantation, Lunar Atmosphere, Lunar Soil, Solar Wind, Abundance, Carbon Dioxide, Carbon Monoxide, Escape, Methane
Scientific paper
About 8 tons of solar-wind carbon is implanted in the lunar soil each year. This inflow is adequate to supply the present regolith carbon abundance (about 100 ppm) in 1-m thickness of soil per billion years. However, the present meteor flux is only capable of mixing to a depth of 10 cm over a billion-year period. As a result, soil mixing cannot act to assimilate the total influx of carbon in the soil. It is necessary that most of the carbon influx be balanced by escape. Model atmospheres for three candidate gases, CH4, CO, and CO2, have been computed. Each model is sized to provide the needed escape rate.
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