It’s a God awful small affair, to the girl with the mousy hair
Deviating somewhat from the standard theme of my blog, but it’s almost life-science related. Allusions to biochemistry and all that. Anyway, I’m sure most of you have heard the tantalising news of data emerging from the Curiosity Rover on Mars, suggesting that Mars had an environment conducive to life in it’s ancient past. I’ve had about a day to let that news sink in but it’s still exciting.
On facebook I follow a page called ‘The Universe’. It is probably my favourite page on that website. It doesn’t dumb things down, it keeps very true to themes about the universe and it’s not in your face and obnoxious like ‘I fucking love science’ sometimes gets (though it’s still a fun page to follow).
Regarding the recent data from Mars (the scientist in me is telling me to wait on confirmation data from the next set of experiments), ‘The Universe’ posted one of the most brilliant, beautiful summaries of the discovery on facebook. I felt it a bit of shame that it only went up on facebook, to me it bettered NASA’s own delivery of the gravity and implications of the discovery. Now let’s just hope the data presented by NASA isn’t anomalous (though all the cumulative data from Mars expeditions would make this somewhat unlikely)!
I like to keep the majority of the stuff I post on here original, and only reblog/quote in exceptional circumstances - and this is one of those circumstances. This is the excellent summary of the journey to find out if Mars could once support life, Copied from here. -
- “To tell that story, we have to go back to before the Mars Exploration Rover mission. When MER went to Mars, we sent 2 rovers, and we sent them to 2 different sites, both hunting for evidence of water. One went to a site that looked like a lake in the geomorphology, the other went to a site where orbital spectra indicated the presence of hematite, a mineral which likely formed in the presence of water. When we got to the two sites, we found the geomorphology site was filled with basalt, and the hematite-site was filled with sediments derived from a water-bearing environment. Eventually, Spirit caught up, and found evidence of a hydrothermal system, but really, the rover sent to the mineralogy site found the water first.
The Curiosity rover selection process was one of the most difficult decisions I’ve seen NASA make. Instead of 2 rovers, this time, they only had 1. They couldn’t miss. They basically had the same decision; picking between a mineralogical site and a couple geomorphology sites. The geomorphology sites resemble river deltas from orbit. The mineralogical site, a place called Gale Crater, had the spectral signature of clay minerals.
Clay minerals imply an environment we’ve never seen before on Mars. In very wet environments on Earth, clay minerals are the most important product. When a rock erodes in the presence of lots of water, the soluble elements are removed, and only the most insoluble elements remain. The 2 most insoluble elements in water are iron(III) and aluminum.
On Earth, the continents are made of rocks like granodiorite and granite. These rocks don’t contain much iron, so Earth makes minerals that contain aluminum and water; aluminum-rich clays. Minerals like Kaolinite, aluminum clays. If you go to the Amazon River on Earth, coming out of a rainforest where water is abundant, the mineral you find coming out along with the water is kaolinite; water rich aluminum-clay. Clays tell you that the environment had a lot of water. They form in areas that have lakes and have oceans. They don’t form in dry settings, they don’t form in deserts, and they don’t form when water is only around for a short time.
Mars isn’t a granite world; it’s a basalt world. Compared to Earth, the rocks on Mars have much more iron. When you try to make clays out of these iron-rich basalts, the end result is an iron-rich clay called nontronite, rather than aluminum-clays. Seeing clay minerals implies not only that water was present, it implies a lot of water. It implies that so much water was present that all of the other soluble elements in the rocks were stripped out by water. This is a setting none of the other rovers saw, and this clay mineral was detected from orbit in abundance at Gale Crater. Quite simply, clay minerals are the #1 reason why the landing site was chosen. Last time, the mineralogical site found what it was looking for and the geomorphology site did not. So, with only 1 landing site, the mineralogical site, showing evidence of clay minerals and large amounts of water, was chosen.
The single biggest goal of this rover is assessing the rocks that contain clay minerals, the environment they formed in, and what that tells us about the environment on Mars when there was a large amount of water present.
That’s the backstory of this press release. Today, the Curiosity team announced the results of drilling into a rock called “John Klein” (drill hole pictured). The rover has been driving on what appears to be an alluvial fan deposit fed by a channel on the Gale Crater rim. The rover landed on coarse grained fan rocks, and drove to a place where the rocks appeared finer grained. These fine grained rocks are the rocks they drilled.
They fed this first drilled sample into the CheMin instrument and the SAM instrument. CheMin is an X-Ray diffraction system. It is spectacular at identifying minerals. If you wanted to identify clay minerals, it’s exactly what you’d want. They fed the drilled sample into CheMin, and…it turned out to be made of iron-bearing, smectite clays. Also known as; nontronite.
They also fed the sample into the SAM instrument, a mass spectrometer. SAM can measure abundances of elements like carbon and sulfur, and hopefully also measure isotopes on those samples. They didn’t give us the isotope compositions in the press release, suggesting that they’re still working on those, but they did announce the presence of carbon and sulfate bearing minerals.
Put all this together, and the most important part of today’s results is this sentence; we found what we were looking for. In the other 2 sites on Mars, we found evidence of some water, but not large amounts of water. Spirit found a hydrothermal environment, where small amounts of water circulated through the rocks. Opportunity found an oasis in a desert, where small amounts of water had moved through rocks and precipitated minerals like hematite.
Curiosity went to a place where the orbital spectra say there should have been a lot of water. Clay minerals aren’t made when there is only a small amount of water; it takes a lot of water to make clay. It takes a lake, or an ocean, or at least long-lived water bodies. The other rovers found small amounts of water and the signatures of acidic environments.
To create a habitable environment, as we understand it, you don’t just need small amounts of water, you need a lot of water. You need enough water to drown the rocks, to move most of the elements around. The end result of this amount of water should be clay minerals. If that kind of environment ever existed on Mars, the signature should be nontronite clays. Those clay minerals could be trapped in mudrocks, like shales and siltstones on Earth, and if we’re lucky, they’d have carbon, sulfur, and other elements that life could make use of trapped within them that could be analyzed.
That rock type is…exactly what Curiosity drilled. We went to Gale crater hunting for clays. We picked Gale Crater because orbital spectra said there was clay. We wanted to see the rocks that hosted the clay, measure the chemistry of clay-bearing rocks, and interpret what the environment was that formed them.
There are a lot of other interesting details about this rock. It appears less-oxidized than the surface. It isn’t fully red; when they drilled the rock, they found it looked dark; meaning some of the iron hadn’t oxidized. It wasn’t fully altered. They also found olivine, an easily-erodible mineral, in the mudrocks. These results suggest that the clays were laid down with sediment that wasn’t as highly altered, because olivine and reduced minerals wouldn’t survive that much exposure to water. They also found both sulfates and sulfides, indicating partial reaction of the sulfur-bearing minerals, but not complete consumption of them. These details will take time to figure out, and I’m sure the team will target a whole lot of effort to figuring them out, as chemical reactions involving reduced minerals and sulfide minerals on earth provide energy that life can use to sustain itself.
All of these are important and the team will keep working on them. But the message you should take from today’s press release is this; we went to Gale Crater looking for clay minerals like nontronite in the rocks, because those minerals would tell us that there was a very large amount of water when they formed. Today, they announced…they found what they are looking for. Curiosity is where it was supposed to be. We sent an organic chemistry laboratory to Mars to look at clay-bearing rocks. We now have an organic chemistry laboratory sitting on clay-bearing rocks. We found what we are looking for.
-JBB
Image credit: NASA/JPL-Caltech/Cornell/MSSS
http://www.nasa.gov/mission_pages/msl/news/msl20130312.html
The image compares rocks seen by NASA’s Opportunity rover and Curiosity rover in two different areas of Mars. On the left is “Wopmay” rock, in Endurance Crater, Meridiani Planum, studied by the Opportunity rover; on the right are the rocks of the “Sheepbed” unit in Yellowknife Bay, in Gale Crater, which Curiosity has been studying. The images have been white balanced to show roughly what they would look like if they were on Earth. ” -




















































