The origin of the Martian intercrater plains - The role of liquefaction from impact and tectonic-induced seismicity

Details The origin of the Martian intercrater plains - The role of liquefaction from impact and tectonic-induced seismicity The origin of the Martian intercrater plains - The role of liquefaction from impact and tectonic-induced seismicity

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..241c&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 241.

Computer Science

Mars Craters, Plains, Hypervelocity Impact, Tectonics, Seismology, Liquefaction, Mars Surface, Meteoritic Composition

Scientific paper

The nature of liquefaction-induced seismicity is briefly reviewed. The
possibility that this mechanism can account for the origin of the
Martian intercrater plains is briefly assessed.

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