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Distribution of Methane and Carbide in Apollo 11 Fines

Abstract

METHANE (up to 5 µg g−1 carbon), and material behaving as carbide (releasing up to 23 µg g−1 carbon as CD4) on deuterated acid dissolution, are ubiquitous components of lunar fines1–4. The abundances of both components correlate with a number of parameters related to the extent of exposure of the samples on the lunar surface2,3. Also, location studies show that the CH4 and carbide are apparently concentrated at particle surfaces4,5. We have suggested therefore that the principal origins for each species involve processes occurring directly at the lunar surface, notably solar wind implantation for formation of CH4 and both solar wind implantation and meteorite impact for the formation of carbide1–4.

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CADOGAN, P., EGLINTON, G., MAXWELL, J. et al. Distribution of Methane and Carbide in Apollo 11 Fines. Nature Physical Science 241, 81–83 (1973). https://doi.org/10.1038/physci241081a0

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