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As the discovery of so-called SLiMEs (Science, 20 October 1995) on
Earth have shown, non-photosynthetic-based ecosystems exist on Earth. The idea is that hot water reacts with basalt to produce hydrogen, that can be used by thermophilic micro-organisms in methanogenesis or sulfate-reduction. I think if we will ever find life on Mars it will probably be something of this nature. Do we know if there is basalt or related iron(II)containing rocks under the Martian surface (I would guess so, since the surface material is mostly iron(III) and there is probably a core of liquid iron too)? Are Spirit and Opportunity capable to detect deep underground reservoirs of liquid water? And if we can localize these, would it be technologically feasible to equip future unmanned missions with some means to drill up samples (probably several hundreds of metres deep) and examine them? Would fixation of radioactive carbon in these samples provide sufficient proof of metabolic activity? |
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