Saturday 28 September 2013

MARS CURIOSITY ROVER'S ANALYSIS

Evidence that water once existed on Martian soil found

A mosaic of images taken by the telephoto right-eye camera of the Mast Camera (Mastcam), Curiosity shows a cluster of dark rocks in the


Ø In the first series of the Curiosity rover’s analysis of fine Martian soil samples, scientists have found that two per cent of it is water by weight. They have also found other evidence that hint at liquid water having once existed on the planet.

Ø Soil samples were picked up from a patch of sand, silt and dust called Rocknest. They were heated to 835 degrees Celsius and studied by instruments onboard the rover.

Ø “The major gases released were water – about 2 per cent by weight of the sample – and carbon dioxide, oxygen and sulphur dioxide,”

Ø Analysis by the rover’s instruments found that, locked up in every cubic foot of Martian dirt, there were almost two pints of water. “That’s a real resource for future explorers. We can access it with just a little bit of heating,” 

Ø It was  also found carbonates, which are formed in the presence of water, and alumino-silicates, ferric compounds, and sulphates.

Ø Scientists notes that oxygen could have come from the breakdown of a perchlorate mineral. Perchlorates are markers of past climate and could have participated in the transformation of Martian organic matter. Because of similarities between the compounds in the soil and the atmosphere, the ‘dirt’ collected by the rover seems to have acted as a sponge for the atmosphere, which is where the volatile materials could be derived from.

Hydrogen
Ø “We can see that especially in the amount of the different types, or isotopes, of hydrogen. We know that the atmosphere contains extra heavy hydrogen, called deuterium. And we see that same thing in the water bound in the soil,”
Ø Thus, these minerals are constantly blown around by winds, and they mix with dust from other parts of the planet. This finding is supported by other papers in the report, which found most minerals to be of basaltic origins.
Ø There was a notable exception. A lone, loose rock dubbed Jake M, found on the plains along Curiosity’s path from its landing point, had a chemical composition unlike any other encountered on Mars.
Ø Scientists think it could have originated from a water-rich environment based on its similarities to rocks found in Earth’s rift zones. 

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