The Hydrological Cycle in the Last 80% of Mars History: Sources, Locations, Residence Times, Stability, Duration and Evolution of H2O

Details The Hydrological Cycle in the Last 80% of Mars History: Sources, Locations, Residence Times, Stability, Duration and Evolution of H2O The Hydrological Cycle in the Last 80% of Mars History: Sources, Locations, Residence Times, Stability, Duration and Evolution of H2O

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1724h&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1724

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Scientific paper

Geological evidence indicates that the Mars hydrologic cycle has
consisted of a globally continuous cryosphere for the last 80% of its
history, with liquid water occasionally emerging to the surface during
magmatic events that cracked the cryosphere.

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