Emplacement of a Debris Ocean on Mars by Regional-Scale Collapse and Flow at the Crustal Dichotomy

Details Emplacement of a Debris Ocean on Mars by Regional-Scale Collapse and Flow at the Crustal Dichotomy Emplacement of a Debris Ocean on Mars by Regional-Scale Collapse and Flow at the Crustal Dichotomy

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1584h&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1584

Astronomy and Astrophysics

Astrophysics

Scientific paper

Giant debris flows could have filled the northern lowlands with ~2km of
sediment in 10^3 to 10^5 years by catastrophic regional terrain
collapse. The outburst floods and chaos zones are probably the waning
stage of this process.

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