Exhumed rocks reveal Mars water ran deep
Focusing on the chemistry of rocks embedded in martian crater walls, rims, and central uplifts, scientists identified 175 sites bearing minerals formed in the presence of water.
By
ESA, Noordwijk, Netherlands —
Published:
June 28, 2012 Excavating water-rich rocks. Credits: Mars Express HRSC, ESA/DLR/FU Berlin (G. Neukum); NASA/MOLA Science Team; D. Loizeau et al.
Impact craters are natural windows into the history of planetary surfaces — the deeper the crater, the further back in time you can probe.
In addition, rocks blasted out during the impact offer a chance to study material that once lay hidden beneath the surface.
In a new study, ESA’s Mars Express and NASA’s Mars Reconnaissance Orbiter zoomed in on craters in a 620- by 1,240-mile (1,000 by 2,000 kilometers) region of the ancient southern highlands, called Tyrrhena Terra, to learn more about the history of water in this area.
Focusing on the chemistry of rocks embedded in the crater walls, rims, and central uplifts, as well as the surrounding exhumed material, scientists identified 175 sites bearing minerals formed in the presence of water.
“The large range of crater sizes studied from less than 1 kilometer to 84 kilometers (0.6 to 52 miles) wide indicate that these hydrated silicates were excavated from depths of tens of meters to kilometers,” said Damien Loizeau from ESA. “The composition of the rocks is such that underground water must have been present here for a long period of time in order to have altered their chemistry.”
While the material excavated by impacts appears to have been in close contact with water, there is little evidence for rocks on the surface lying between the craters in Tyrrhena Terra having been altered by water.
“Water circulation occurred several kilometers deep in the crust some 3.7 billion years ago, before the majority of craters formed in this region,” said Nicolas Mangold from the Laboratory of Planetology and Geodynamics in France. “The water generated a diverse range of chemical changes in the rocks that reflect low temperatures near the surface to high temperatures at depth, but without a direct relationship to the surface conditions at that time.”
By comparison, Mawrth Vallis, one of the largest identified clay-rich regions of Mars, displays a more uniform aqueous mineralogy that indicates a closer link with surface processes.
“The role of liquid water on Mars is of great importance for its habitability, and this study using Mars Express describes a very large zone where groundwater was present for a long time,” said Olivier Witasse from ESA.
|