Light element geochemistry of the Apollo 15 site

Details Light element geochemistry of the Apollo 15 site Light element geochemistry of the Apollo 15 site

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976lpsc....7..481k&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

5

Apollo 15 Flight, Chemical Composition, Geochemistry, Light Elements, Lunar Landing Sites, Lunar Rocks, Abundance, Carbon Isotopes, Iron Isotopes, Lunar Composition, Nitrogen Isotopes, Sulfur Isotopes

Scientific paper

Abundances of C, N, S, and He and contents of CH4 and metallic Fe at Hadley-Apennine are typical of a mixed mare and highland environment. Isotopic compositions of C, N, and S similarly conform in most cases to patterns observed elsewhere on the moon. Systematic relationships between S abundance and total Fe content are apparent for crystalline rocks from most landing sites but their full significance is not yet understood.

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