QUOTE (Marcel @ Apr 28 2005, 10:29 AM)
My first reaction was: get back! But now Oppy is in there, they might as well take the opportunity (
) to investigate the soil on composition (and then get back!). Maybe the lighter coloration doesn't have to do so much with outcrops (like orbital imagery suggests), but with a lighter toned (higher salt content?) material. Salt is lower in density than rock, which could be an explanation for the different mechanical properties Oppy is facing now.
Maybe there aren't any outcrops at all between here and Victoria! Maybe the lighter colour isn't a rocky rim of Erebus cropping out, but completely eroded and fragmented "mothermaterial" of the ancient crater, presenting itself just by a lighter soil.....
In that case, reaching Victoria will only be possible by avoiding the light stuff and find a route on the darker soil....very interesting !
Hmmm... when you look at the highest-resolution MOC imagery, it's true that you can't tell for certain if the "outcrop" is really outcrop or if it's just piles of lighter-colored sand. But if you zoom out a bit and look at a slightly bigger picture, the "outcrop" organizes itself (at least to my eye) into impact-related landforms -- ancient crater rims and "splash pattern" ejecta texturing. That argues for the areas that appear to be outcrop to actually reflect ridges in the local landform.
As has been discussed elsewhere, the blueberries seem to provide a natural cover to prevent further erosion of the evaporite layer out on the plains... and as we advance into the lighter-colored soils and dunes, the blueberries seem to be diminishing in abundance. Maybe we're getting into an area of evaporite that developed a lot fewer concretions? That would mean the evaporite would erode primarily, with no cover of concretions to stop the erosion process.
A good lesson we can learn from both terrestrial and lunar geology is that a vastly large majority of the materials at any given location on the surface of a planet originated(*) within a kilometer or two of that location. I think that argues for the lighter soils and dunes to be the eroded dust from the evaporite layer. I bet the IDD work will show these soils and sands to be very similar in composition to the evaporite layers.
-the other Doug
(*) -- when I say "originate," I'm talking relative to the local landforms. Obviously, large-scale cratering tossed a lot of the original crust around, especially in the ancient cratered southern highlands. But ever since the last of the great impacts and the last of the great floods, I'd bet that nothing much has moved more than a few kilometers in any given direction, with the exception of a very thin layer of dust. DVD