Lots of good info on the last
MER Monthly Report, including details on the problems with the Mossbauer Spectrometer and its expected use on hydrated rocks / clay:
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Why is the overnight cold bothering it now, when spring is warming Mars in the southern hemisphere? “We’re still talking Mars,” noted Nelson. “In middle of Martian day, it’s warm enough that this thing is still working properly, but late in the afternoon or evenings, we don’t get it to work right.”
That may seem really unfortunate for many who have been following this mission since lot of the Mössbauer integrations occurred overnight. “But we’re not going to do extensive Mössbauer investigations for a while, and by the time we get to these hydrated rocks and the rim of Endeavour, we’ll be beyond the real cold temperatures at night,” Arvidson pointed out. “The power source of the instrument is so depleted. Cobalt-57 has a half-life is 271.8 days, so we’re down many half-lives and we have to spend days and days making measurements now. We won’t do take that time anymore unless there’s something extraordinary. The next big campaigns will be when we see the hydrated rocks detected by CRISM, possibly as close at Santa Maria, and then when we get to the clay minerals at the rim.”
And some info re Santa Maria.
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And, yes, they are planning for the rover to stop at Santa Maria, just a short jag off the route. On this fairly “fresh” crater, it appears that the impact has “punctured through the bedrock,” as Arvidson put it. Now about 2.7 kilometers away, Santa Maria is luring the team for another reason.
“As we get close to Endeavour, there’s a change in the characteristics observed by CRISM [onboard MRO] and we start to see hydrated rock that’s exposed, which we don’t see where we are today,” explained Arvidson. “Santa Maria might be close enough so that when it formed, it did so in those hydrated rocks. That’s one of the reasons we’re stopping.” Added Squyres: “We’ll see when we get there.”