[dropcap style=”font-size:100px; color:#992211;”]A[/dropcap]cid fog on Mars. It’s a genuine meteorological phenomenon of sizeable scientific import.
Even if it does sound a bit like a blues-rock/Oasis covers band set up by engineering students hoping to look wacky and meet drunk girls.
Or a particularly nasty strain of sativa.
Planetary scientist Shoshanna Cole has pieced together a compelling story about how acidic vapors may have eaten at the rocks in a 100-acre area on Husband Hill in the Columbia Hills of Gusev Crater on Mars. She used a variety of data gathered by multiple instruments on the 2003 Mars Exploration Rover Spirit to tease out information from exposures of the ancient bedrock. She will be presenting her work on Monday, Nov. 2, in Baltimore, Maryland, at the annual meeting of the Geological Society of America.
The work focused on the ‘Watchtower Class’ outcrops on Cumberland Ridge and the Husband Hill summit, said Cole, who is an assistant professor at Ithaca College and began studying the area for her Ph.D. thesis at Cornell University.
“The special thing about Watchtower Class is that it’s very widespread and we see it in different locations. As far as we can tell, it’s part of the ground there,” which means that these rocks record environments that existed on Mars billions of years ago.
By combining data from previous studies of the area on Mars, Cole saw some intriguing patterns emerge. Spirit examined Watchtower Class rocks at a dozen locations spanning about 200 meters along Cumberland Ridge and the Husband Hill summit. The chemical composition of these rocks, as determined by Spirit’s Alpha Proton X-ray Spectrometer (APXS), is the same, but the rocks looked different to all of the other instruments.
Across Cumberland Ridge — which is about 1/3 the size of a football field — the Mössbauer Spectrometer showed there was a surprisingly wide range in the proportion of oxidized iron to total iron, as if something had reacted with the iron in these rocks to different degrees. This iron oxidation state ranges from 0.43 to 0.94 across a span of only 30 meters. Meanwhile, data from both the Mössbauer Spectrometer and the Miniature Thermal Emission Spectrometer (Mini-TES) showed that the minerals within the rocks changed and lost their structure, becoming less crystalline and more amorphous. And these trends match the size of small bumps, which Cole calls agglomerations, seen in Pancam and Microscopic Imager pictures of the rocks.
“So we can see the agglomerations progress in size from west to east and the iron changes in the same way,” Cole said. “It was super cool.”
But the fact that the rocks were otherwise the same in composition indicates that they were originally identical. “That makes us think that they were made of the same stuff when they started out. Then something happened to make them different from each other.”
Cole hypothesizes that the rocks were exposed to acidic water vapor from volcanic eruptions, similar to the corrosive volcanic smog, or “vog,” that poses health hazards in Hawaii from the eruptions of Kilauea. When the Martian vog landed on the surface of the rocks it dissolved some minerals, forming a gel. Then the water evaporated, leaving behind a cementing agent that resulted in the agglomerations.
“So nothing is being added or taken away, but it was changed,” Cole said. “This would have happened in tiny amounts over a very long time. There’s even one place where you see the cementing agent healing a fracture. It’s pretty awesome. I was pretty happy when I found that one.”
More support of this idea comes from a 2004 study in which scientists conducted laboratory experiments exposing mock martian basalt rocks (based on data from the Mars Pathfinder mini-rover) to sulfuric and hydrochloric acids. The results indicated that as these rocks are exposed to acids, they lose their crystalline structure — just like what Cole sees in varying degrees across the Watchtower Class exposures.
As for why there is a trend in the iron and the degree to which the rocks were changed, the answer is microclimates, similar to those in different areas of your home garden. The time that the gel was present on the rocks depended on how much sunshine and wind the rocks got. The more altered rocks, which have larger agglomerations, are on very steep slopes facing away from the Sun, which makes them shadier. The least altered rocks are on sunnier and gentler slopes, according to Cole.
Piecing together this Martian vog puzzle underscores the story of Spirit’s success.
“Spirit’s the rover who always had to try harder,” she said. “She was sent to Gusev Crater to look for lake deposits, but landed in lava field. She had to make a long trek to the Columbia Hills to find evidence of ancient watery environments. There’s still tons of data to analyze there, and that’s really nifty.”
Source: Eurekalert/Geological Society of America
Image: mage from S. Cole, PhD thesis; background image: NASA/JPL/Cornell/Arizona State University; Moessbauer values from Morris et al. 2008 (doi: 10.1029/2008JE003201).
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