Compositional trend within the lunar highland crust

Details Compositional trend within the lunar highland crust Compositional trend within the lunar highland crust

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..802o&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.802

Computer Science

Scientific paper

In this study we investigated spatial and vertical compositional (modal abundance) trends of the high plagioclase abundance anorthosite rocks over the entire lunar surface within the upper crust by using continuous reflectance spectra derived by the SELENE Spectral Profiler (SP) [3] and images derived by the SELENE Multiband Imager (MI) [1]. We also investigated compositional trend within the deeper area than a central peak excavation depth (possibly lower crust) based on a composition of Orientale ejecta. Orientale is selected because it is young and least disturbed by later impact event.

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