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To partially etch the hematite core, the above silica-encapsulated hematite nanoparticles were suspended in 180 mL distilled water with 1.8 g PVP and 11.34 g oxalic acid (0.5 M) and incubated at 60 °C for 10.5 h.
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The hematite ore assays over 65percentnt iron.
From orbit, however, scientists could not tell which rocks contained the hematite or how the hematite got there.
Because of the hematite, Meridiani Planum is expected to look unlike other landscapes seen to date on Mars, perhaps with shiny hematite outcrops jutting out of the ground.
It is also possible that the hematite formed without water in oxygen-rich lavas.
From orbit, the Mars Odyssey spacecraft spotted a deposit of hematite the size of Oklahoma blanketing Meridiani Planum, but it could not tell whether the hematite was in the soil or the rocks or elsewhere.
The hematite model flowsheet precipitates iron as hematite (Fe2O3) downstream from the leach in a dedicated autoclave.
In solution, the hematite splits oxygen away from hydrogen.
The hematite spheres (or 'Martian blueberries') as imaged by the Mars Exploration Rover.
The hematite probably formed from reactions with oxygen molecules in the oceans.
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