Lunar mare basalts - Conference summary

Details Lunar mare basalts - Conference summary Lunar mare basalts - Conference summary

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976eostr..57..823m&link_type=abstract

EOS, vol. 57, Nov. 1976, p. 823-829.

Mathematics

Logic

Basalt, Lunar Composition, Lunar Maria, Apollo 17 Flight, Chemical Composition, Earth Crust, Gamma Rays, Geological Surveys, Lunar Rocks, Metamorphic Rocks, Spectroscopy, Titanium

Scientific paper

Compositionally, lunar mare basalts are similar to some very young subalkaline basalts from terrestrial mid-ocean ridges and to very old pods of basaltic material incorporated into ancient metamorphic rocks. Basalt flows in Mare Imbrium are considered, taking into account the results of orbital gamma ray spectroscopic studies. The results of the analyses of lunar samples obtained from the Apollo missions are evaluated and various models are discussed in connection with an interpretation of the observed conditions.

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