Martian-soil density map - Comparison with albedo, topography, and geology

Details Martian-soil density map - Comparison with albedo, topography, and geology Martian-soil density map - Comparison with albedo, topography, and geology

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..611e&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, July-Aug. 1979, p. 611-621. In Russian.

Mathematics

Logic

Astronomical Maps, Geology, Mars Surface, Topography, Albedo, Correlation, Histograms

Scientific paper

Various maps of Mars are compared, including soil density, albedo, hypsometric, and geological. A major finding is the presence of two types of fines: dark and light, with predominance of the light component. Age-dependent variations of mantle density and albedo are identified. The geologically younger regions have a higher concentration of fines and are lighter.

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