LONDON: Mineral veins seen on Mars were formed by the evaporation of ancient martian lakes, scientists have found, providing evidence for long and varied history of water on the red planet.
The research used NASA’s Mars Curiosity rover to explore Yellowknife Bay in Gale Crater on Mars, examining the mineralogy of veins that were paths for groundwater in mudstones.
The study suggests that the veins formed as the sediments from the ancient lake were buried, heated to about 50 degrees Celsius and corroded.
“The taste of this martian groundwater would be rather unpleasant, with about 20 times the content of sulphate and sodium than bottled mineral water for instance,” said Professor John Bridges from University of Leicester in the UK.
“However, some microbes on Earth do like sulphur and iron rich fluids, because they can use those two elements to gain energy. Therefore, for the question of habitability at Gale Crater the taste of the water is very exciting news,” said Bridges.
The researchers, including those from The Open University in the UK, suggest that evaporation of ancient lakes in the Yellowknife Bay would have led to the formation of silica and sulphate-rich deposits.
Subsequent dissolution by groundwater of these deposits which the team predict are present in the Gale Crater sedimentary succession led to the formation of pure sulphate veins within the Yellowknife Bay mudstone.
The study predicts the original precipitate was likely gypsum, which dehydrated during the lake’s burial.
The team compared the Gale Crater waters with fluids modelled for martian meteorites shergottites, nakhlites and the ancient meteorite ALH 84001, as well as rocks analysed by the Mars Exploration rovers and with terrestrial ground and surface waters.
The aqueous solution present during sediment alteration associated with mineral vein formation at Gale Crater was found to be high in sodium, potassium and silicon, but had low magnesium, iron and aluminium concentrations and had a near neutral to alkaline pH level.
The mudstones with sulphate veins in the Gale Crater were also found to be close in composition to rocks in Watchet Bay in North Devon in the UK, highlighting a terrestrial analogue which supports the model of dissolution of a mixed silica and sulphate-rich shallow horizon to form pure sulphate veins.
“These result provide further evidence for the long and varied history of water in Gale Crater. Multiple generations of fluids, each with a unique chemistry, must have been present to account for what we find in the rock record today,” said Ashwin Vasavada, Curiosity Project Scientist from the NASA Jet Propulsion Laboratory in the US.