Trace element identification of three chemically distinct very low titanium (VLT) basalt glasses from Apollo 17

Details Trace element identification of three chemically distinct very low titanium (VLT) basalt glasses from Apollo 17 Trace element identification of three chemically distinct very low titanium (VLT) basalt glasses from Apollo 17

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994gecoa..58.1367l&link_type=abstract

Geochimica et Cosmochimica Acta, vol. 58, p. 1367

Computer Science

9

Trace Elements, Basalt, Regolith, Titanium, Abundance, Lunar Rocks, Apollo 17 Flight, Igneous Rocks, Electron Probes, Glass

Scientific paper

Small VLT samples from Apollo 17 soils were analyzed for trace elements using newly developed high sensitivity INAA techniques. Three distinct groups of VLT compositions are identified. Cobalt contents clearly delineate the HICo, MECo, and LOCo groups, which are also clearly identifiable by their major and minor element compositions. The results allow conclusions to be drawn concerning the sequence of events that produced the regolith at the Apollo 17 landing site.

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