J
JonClarke
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<p class="MsoNormal">For some reason nobody seems to have commented on nthis story, despite its importance. So, better late than never, here it is.</p><p class="MsoNormal"><font face="Arial" size="2"><span style="font-size:10pt;color:black;font-family:Arial"><font color="#0000ff">http://www.space.com/includes/iab.html?url=/scienceastronomy/081218-agu-mro-carbonte.html</font></span></font></p><p class="MsoNormal"><font face="Arial" size="2"><span style="font-size:10pt;color:black;font-family:Arial">It is important for lots of reasons.</span></font></p><p class="MsoNormal"><font face="Arial" size="2"><span style="font-size:10pt;color:black;font-family:Arial">It shows evidence for intense weathering on Mars in the Early Hesperian, which means lots of liquid water interaction with the rock.</span></font></p><p class="MsoNormal"><font face="Arial" size="2"><span style="font-size:10pt;color:black;font-family:Arial">It shows evidence for extensive non-acidic weathering.</span></font></p><p class="MsoNormal"><font face="Arial" size="2"><span style="font-size:10pt;color:black;font-family:Arial">The magnesite (magnesium carbonate) occurs in qaulities that on Earth would be considered ore grade, This is of interest for those interested in Mars settlement as magnesium is a very useful metal.</span></font></p> <div class="Discussion_UserSignature"> <p><em>Whether we become a multi-planet species with unlimited horizons, or are forever confined to Earth will be decided in the twenty-first century amid the vast plains, rugged canyons and lofty mountains of Mars</em> Arthur Clarke</p> </div>