Months after scientists announced "the strongest evidence yet" of liquid water on Mars, a study today said there was none at least in the valleys carved into numerous Red Planet slopes.
Months after scientists announced “the strongest evidence yet” of liquid water on Mars, a study today said there was none at least in the valleys carved into numerous Red Planet slopes.
Rather than water flows like those on Earth, these Martian gullies were likely created by dry ice defrosting, a duo of French scientists wrote in the journal Nature Geoscience.
“The role of liquid water in gully formation should… be reconsidered, raising the question of the importance of its occurrence in Mars’ recent past,” wrote Francois Forget and Cedric Pilorget of the French national research institute CNRS.
They said their findings held no implications for the headline-making announcement in September that dark lines running down slopes in the tropics of Mars in summer, may be streaks of super-salty brine — hinting at the presence of life-sustaining water.
Monday’s paper dealt with unrelated geological features in a different part of the planet, mainly in the mid-latitude range between 30 and 60 degrees, on pole-facing cold slopes, said the French team.
They had set out to explain the origins of small channels carved into crater walls, hills and other martian protrusions.
When first discovered, these gullies were interpreted as runoff from melting water ice or groundwater leaks that occurred hundreds of thousands of years ago.
Then, in recent years, it was discovered that gully formation was ongoing, in spite of Mars being too cold for liquid water to exist.
Pilorget and Forget looked for answers in a thin layer of frozen carbon dioxide (CO2) observed to be present in periods that gullies were being formed.
They used computer simulations to show that thawed and trapped CO2 gas building up beneath the surface ice layer would eventually break through the soil and trigger flows of gas and debris.
No similar processes are known to occur on Earth.