QUOTE (WindyT @ Apr 25 2007, 01:05 PM)
Are fines coming out of the crater responsible for the apparent layering (dark and light layers) in the dunes we saw on the way to Victoria?
QUOTE (atomoid @ Apr 25 2007, 06:32 PM)
dune layering on the plains consisting of fines blowing in from the whole planet in general to mix unevenly with the larger local grains i think...
..which brings me back to: did anyone ever hear of any research trying to link the dune layering with any sort of seasonal/epochal timeline? if we could count tree-rings, then we'd know what were looking at. i dont know if anyone has even submitted a theory arguing whether the sand dunes are fossils or not.
QUOTE (WindyT @ Apr 26 2007, 12:58 AM)
I used to think that as well, but I went back over the dune pictures, and it looked like the layering became more distinctive as Oppy approached the crater annulus. I starting thinking about what fines could come out of the crater and what that additional deposition might look like.
With the recent statement, I revived these quotes from the thread. It sorta all fits together:
When deposition>removal, you get a layer.
Dark sand out of crater blows out from crater/dark streak on annulus and goes all over plain = dark zone in sequence.
Light dust from all over Mars filters down from atmosphere = light dust buildup makes light zone in sequence.
There's probably a pretty tiger stripe sequence of altenating dark layers and light layers as you dig down in the streaks. I'd expect dark streaks when more wind is present, and light streaks all other times.
Just like tree rings. Everybody wins.
Any imagemeisters got any patterns from image analysis of dunes near the annulus? Might give a clue as to the seasonality....
-Mike