Type 2 Terrain: Compositional Constraints on the Martian Lowlands

Details Type 2 Terrain: Compositional Constraints on the Martian Lowlands Type 2 Terrain: Compositional Constraints on the Martian Lowlands

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1230n&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1230

Computer Science

5

Scientific paper

The presence of glass and/or weathering products can alter the mid-IR
spectral properties of a basaltic surface to mimic a more silicic
composition.

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