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originally posted by: funbox
a reply to: Soylent Green Is People
interesting stuff on the phoenix lander , as ArMaP pointed out ,but is this really comparable to the picture were seeing from curiosity.. 7 minuets is quite a short time for seeing the movement we are seeing
originally posted by: Phage
There can be no dew on Mars. The air pressure is to low to allow liquid water to condense. Frost is possible in the Martian winter, but no dew. And no possibility of liquid water (unless it's very, very salty) except for a few regions (of which Gale Crater is not one).
originally posted by: Aleister
But this find is not just something that could be picked out of a Curiosity landscape picture - it had to be noticed, checked, then photographic evidence of the movement presented. So if it turns out to be what funbox and Blue Shift are surmising, at least one of the probable surmises, ATS should be very proud. imnho.
After our successful drill last week, the main event in today’s sol 765 plan is dropping off the drilled sample in CheMin, which will tell us what minerals are in the rocks of Pahrump Hills. CheMin works by shining a beam of X-rays through the sample and recording how the X-rays reflect off of the structure of the crystals in the sample. To make sure that every possible orientation of the crystals is measured, the sample holder vibrates, causing the powdered rock to mix around in the sample cell.
After our successful drill last week, the main event in today’s sol 765 plan is dropping off the drilled sample in CheMin, which will tell us what minerals are in the rocks of Pahrump Hills. CheMin works by shining a beam of X-rays through the sample and recording how the X-rays reflect off of the structure of the crystals in the sample. To make sure that every possible orientation of the crystals is measured, the sample holder vibrates, causing the powdered rock to mix around in the sample cell.
The drill sample has been sieved so that only particles smaller than 150 microns will go to CheMin. The rover will dump out the particles that are coarser than 150 microns, take pictures of them with Mastcam and MAHLI, and measure their composition with APXS. Not all of the fine-grained sample will go to CheMin: some will be saved for analysis by SAM, and in case we want to re-analyze it with CheMin.
originally posted by: wildespace
And here's the info on what Cury has been doing on that Sol: astrogeology.usgs.gov...
"After our successful drill last week, the main event in today’s sol 765 plan is dropping off the drilled sample in CheMin, which will tell us what minerals are in the rocks of Pahrump Hills. CheMin works by shining a beam of X-rays through the sample and recording how the X-rays reflect off of the structure of the crystals in the sample. To make sure that every possible orientation of the crystals is measured, the sample holder vibrates, causing the powdered rock to mix around in the sample cell."
[Emphasis mine]