J
JonClarke
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There is a very exciting image at http://qt.exploratorium.edu/mars/opportunity/pancam/2004-11-03/1P152775622EFF37K5P2439L2M1.JPG<br /><br />It shows an angular relationship between units at the bootm of the cliff and those higher up. There are three possibilities:<br /><br />1) Faulting, although in this case the faulting is very low angle to parallel to layering whereas faults typically associated with cratering are very steep. Therefore I don't prefer this option.<br /><br />2) Angular unconformity between steeply dipping older and sub horizontal younger rocks. This would be very exciting as it is concslive evidence for deformation and erosion cycles on mars. However, the evidence from orbital imagery is that Endurance crater is not situated near the bottom of the succession so again, I don't prefer this option.<br /><br />3) Large scale cross bedding. The scale of this and the evidence for lacustrine processes in other sediments would suggest wither a) aeolian dunes or b) fluvial cross bedding.<br /><br />I can see Opportunity spending another month or two in this area!<br /><br />Cheers<br /><br />Jon <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>