A Comparison of Terrestrial and Martian Gravity Conditions on the Behavior of CO2-driven Aqueous Flow

Details A Comparison of Terrestrial and Martian Gravity Conditions on the Behavior of CO2-driven Aqueous Flow A Comparison of Terrestrial and Martian Gravity Conditions on the Behavior of CO2-driven Aqueous Flow

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2011l&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2011

Physics

Scientific paper

Exsolution of small amounts of volatiles from discharging water can
cause pulsing flow (geysering) on Mars (forming streamlined mesas in the
Cerberus Plains). Martian gravity changes the properties of the pulses
from terrestrial conditions.

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