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East side of Cape York, Sol 3040 - 3056
fredk
post Aug 29 2012, 01:50 PM
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QUOTE (Tesheiner @ Aug 29 2012, 11:55 AM) *
The name of some imaging sequences from today say something about it.
Those should have been taken before the 3056 drive, when we were still at the 3053 location surrounded by all the pretty veins. Since we've moved inland tosol, I'm guessing that we're going after the putative clays, since we're now halfway along CY. I know who I'm rooting for to reach the clays first!
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Stu
post Aug 29 2012, 02:05 PM
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QUOTE (fredk @ Aug 29 2012, 02:50 PM) *
I'm guessing that we're going after the putative clays, since we're now halfway along CY. I know who I'm rooting for to reach the clays first!


Well, she's heading towards these...

Attached Image


... so maybe it's prospecting time... smile.gif


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walfy
post Aug 29 2012, 08:28 PM
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The rock from sol 3049 makes for a nice 3D.

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Tesheiner
post Aug 29 2012, 09:12 PM
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QUOTE (fredk @ Aug 29 2012, 03:50 PM) *
Those should have been taken before the 3056 drive, when we were still at the 3053 location surrounded by all the pretty veins.

Checked it and the pancam shot was taken at the previous site but the navcam was shot "mid-drive" more or less around the 35km mark.
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dvandorn
post Aug 29 2012, 10:17 PM
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Just have a curiosity (small C) -- if we do get to some phyllosilicates, what does Oppy have left to bring to bear for examination?

I imagine we can at least brush the rock surface and the APXS should still give us some good data. And we can take some MI images. But is the Mossbauer capable of getting good spectra anymore? And if not, how much info can we get with what we got left?

Again, just curious.

-the other Doug


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“The trouble ain't that there is too many fools, but that the lightning ain't distributed right.” -Mark Twain
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fredk
post Aug 29 2012, 11:27 PM
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After the attempt at a looooong MB integration at Greeley this winter, they decided that it was no longer useful, IIRC.
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marsophile
post Aug 30 2012, 12:40 AM
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QUOTE (dvandorn @ Aug 29 2012, 02:17 PM) *
if we do get to some phyllosilicates, what does Oppy have left to bring to bear for examination?


The APXS will give elemental composition, and the MI morphology, but that may not be enough for a definitive identification. In the long run, comparison of the weak signature at Cape York with the strong signature at Cape Tribulation may be very suggestive, i.e., If there is some distinctive feature at Cape York, and a lot more of it at Cape Tribulation, then Oppy may have identified something that is correlated with the phyllosilicates. Curiosity can then investigate similar features with its full complement of instruments.
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Eutectic
post Aug 30 2012, 06:08 AM
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Tesheiner's map from post #89 overlaid with the CRISM data from http://www.planetary.org/blogs/emily-lakda.../2011/3134.html .

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Phil Stooke
post Aug 30 2012, 07:36 AM
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The full set of filters in mutispectral images will help as well, though I don't know how much in this context.

Phil


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Tesheiner
post Aug 30 2012, 12:13 PM
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A 12m "bump" was executed on sol 3057.
Here's the "post-drive" navcam mosaic.
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belleraphon1
post Aug 30 2012, 02:09 PM
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QUOTE (dvandorn @ Aug 29 2012, 05:17 PM) *
Just have a curiosity (small C) -- if we do get to some phyllosilicates, what does Oppy have left to bring to bear for examination?

I imagine we can at least brush the rock surface and the APXS should still give us some good data. And we can take some MI images. But is the Mossbauer capable of getting good spectra anymore? And if not, how much info can we get with what we got left?

Again, just curious.

-the other Doug


See this post from Stu's excellent 'Road To Endeavour' blog....
http://roadtoendeavour.wordpress.com/2011/...g-to-cape-york/

Craig
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centsworth_II
post Aug 30 2012, 02:37 PM
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For the hard core data geeks (of which I am not one), The below paper describes in detail Spirit's evidence for phyllosilicates in Gusev.

Evidence of phyllosilicates in Wooly Patch, an altered rock encountered at West Spur, Columbia Hills, by the Spirit rover in Gusev crater, Mars
"On its traverse to Columbia Hills, the Mars Exploration Rover Spirit investigated an outcrop designated ''Wooly Patch'' .... The major-element composition and Fe-mineralogy, as determined by the Alpha-Particle X-ray Spectrometer and Mossbauer Spectrometer, are inconsistent with any reasonable assemblage of basaltic minerals in that there is an excess of Si and Al. The combined data are best explained by the presence of 14–17% phyllosilicate minerals."

It will be interesting to see how Opportunity's evidence for phyllosilicates at Endeavour matches up. Minus the Mossbauer data of course.
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Stu
post Aug 30 2012, 08:56 PM
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Having briefly surrendered the dancefloor it to her big, sexier sister, Oppy is definitely jumping back into the spotlight as she advances upon some fascinating geology at Cape York. Some gorgeous rock formations here, and some fascinating science to come too, I'm sure...

Attached Image



Attached Image



Colour view of the rocks around Oppy now - just a simple 4,5,6 combo; no magic spells, SKYNET supercomputer or goat sacrifices needed to make it from the raw images... rolleyes.gif

Attached Image


Can't wait to see what Oppy does here!


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ngunn
post Aug 30 2012, 09:21 PM
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I had already started to hope, and your anaglyph increases my anticipation, that these outcrops could be (at last) the everted crater rim strata we were expecting to see (but didn't) at Morris Hill. If this is the material the clays originate from then there could be a sub-Crism-resolution patch of clays right here.
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serpens
post Aug 30 2012, 11:46 PM
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QUOTE (ngunn @ Aug 30 2012, 09:21 PM) *
... that these outcrops could be (at last) the everted crater rim strata ......


What bends my mind is how we could differentiate between ballistically emplaced Endeavour impact ejecta / condensate and uplift rim, which would be the Miyamoto ejecta field materiel. Even if we can identify clays did they develop within the rim or were they formed in the pre Endeavour impact environment?
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