Researchers have long known that there was water in the form of ice on Mars. Now, new research on data from Curiosity shows that it is possible that there is liquid water close to the surface of Mars.
The explanation is that the substance perchlorate has been found in the soil, which lowers the freezing point so the water does not freeze into ice, but is liquid and present in very salty salt water - a brine.
"Our measurements from the Curiosity rover's weather monitoring station show that these conditions exist at night and just after sunrise in the winter. Based on measurements of humidity and the temperature at a height of 1.6 meters and at the surface of the planet, we can estimate the amount of water that is absorbed," said Madsen.
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"The soil is porous, so what we are seeing is that the water seeps down through the soil. Over time, other salts may also dissolve in the soil and now that they are liquid, they can move and precipitate elsewhere under the surface," said Madsen.
Observations by the Mars probe's stereo camera have previously shown areas characteristic of old riverbed that clearly show that a long time ago there was flowing, running water with a depth of up to one meter.
"These kind of deposits are formed when large amounts of water flow down the slopes of the crater and these streams of water meet the stagnant water in the form of a lake. When the stream meets the surface, the solid material carried by the stream falls down and is deposited in the lake just at the lakeshore.
Gradually, a slightly inclined slope is built up just below the surface of the water and traces of such slanting deposits were found during the entire trip to Mount Sharp.
"The sediment plates on the bottom are level, so everything indicates that the entire Gale Crater may have been a large lake," Madsen added.
The research was published in the scientific journal Nature.