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Meridiani has a very strange feature.
There are craters and no ejecta. Is the ejecta all covered by some recent event? If so, why is the surface surrounding the craters not lumpy? Are the craters not impact events but sinkholes? The bottom of Eagle crater had horizontal sedimentary rock the was cracked parallel to the layering. This would make sense if the ground had sunk. Opportunity is aproaching endurance crater which is pretty large, but the surface looks smooth all the way to the drop off. |
#2
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Mike Herron wrote in message ...
Meridiani has a very strange feature. There are craters and no ejecta. Is the ejecta all covered by some recent event? If so, why is the surface surrounding the craters not lumpy? Are the craters not impact events but sinkholes? The bottom of Eagle crater had horizontal sedimentary rock the was cracked parallel to the layering. This would make sense if the ground had sunk. Opportunity is aproaching endurance crater which is pretty large, but the surface looks smooth all the way to the drop off. Craters age and change. Over time they lose their ejecta blankets and slump. This is true even on the Moon where impacts of various sizes (ranging upwards from near continuous bombardment by micrometeoroids) disturb the surface. On Mars there is also the wind, wind-borne dust, and, potentially for older craters, water. In fact, the lack of an ejecta blanket is not at all an unusual feature for craters on Mars, it merely indicates it is an old crater that has lost its ejecta blanket due to weathering. More so, a sink hole that would be so nearly circular and otherwise mimic the appearance of a crater so closely would be tremendously unusual. |
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