A new study published in the Astrobiology journal (April
2021) suggests that the Martian sub-surface (below the crust) might be a good
place to look for possible present-day life on the Red planet. The study looked
at the chemical composition of Martian meteorites that landed on the Earth and
was found that these rocks in contact with water would produce enough chemical
energy that is required to support microbial life. This is similar to the
existence of microbial life in the depth of Earth. In recent decades,
scientists have discovered that Earth's depths are home to a vast bloom of life that
exists largely separated from the world above. These creatures survive using
the byproducts of the chemical reactions produced when rocks come into contact
with water.
The most important of the chemical reactions is radiolysis,
where the radioactive elements within rocks react with water and break these
water molecules into hydrogen and oxygen. Hydrogen is dissolved in groundwater
whereas oxygen gets soaked up with minerals like pyrite etc to form sulphate
minerals. These microbes use Hydrogen as fuel and use the oxygen preserved in
sulphates to burn the fuel.
The project named 'Earth-4D Subsurface Science and
Exploration' is supported by the Canadian Institute for Advanced Research is
looking for similar microbial habitats on Mars and elsewhere in the solar
system. The study found that in several different types of Martian meteorites,
all the ingredients are present in adequate quantities to support Earth-like
habitats.
Unlike Earth, Mars lacks tectonic movement that constantly
brings out the inner rocks to the surface. Prior research has found evidence of
an active groundwater system on Mars in the past. The lead author says,
"If we want to think about the possibility of present-day life, the
subsurface is going to be where the action is".

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