A Model of Outflow Generation by Hydrothermal Underpressure Drainage in Volcano–Tectonic Environment, Shalbatana Vallis (Mars)

The Evolution of Lacustrine Environments on Mars: Is Mars Only Hydrologically Dormant?

“…17). Carr (1995) and Cabrol et al (1997) proposed that the source of water for Shalbatana Vallis was a lake located further south in Ganges Chasma. The passage between the Ganges lake and Shalbatana Vallis was created by groundwater conducts which collapsed.…”

Ma'adim Vallis Evolution: Geometry and Models of Discharge Rate

“…It is more likely that subsurface aquifer drainage was episodic over the esti-the valley. There are no other traces of subsequent erosion: thus, we assume that the discharge of this intravalley lake mated two Gyr activity of Ma'adim Vallis Grin and Cabrol, 1997;Cabrol et al, 1997). was the last active episode of Ma'adim Vallis.…”

“…The resolution covering Ma'adim and Squyres, 1991;Cabrol, 1991;Cabrol et al, 1997). The Vallis region varies: for example, the average spatial reso-1.2.…”

Proximal Analysis of Regolith Habitats and Protective Biomolecules in Situ by Laser Raman Spectroscopy: Overview of Terrestrial Antarctic Habitats and Mars Analogs

“…Pumice washload and pumilith of volcanic and meteoritic origin would have been introduced into the sediment by underground drainage processes. Based on analyses of the Shalbatana Vallis region of Tharsis, Cabrol et al (1997) developed a model of volcano-tectonic strains generating crossing fault systems to produce hot spots. This would have allowed hydrothermal drainage of confined aquifers within an ice-saturated cryosphere.…”