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Nasa scientist Daniel Glavin described the results from the first “wet chemistry” experiment carried out by Curiosity.
A long-chain carboxylic acid, or fatty acid, was a good fit for one of the data peaks detected in a mudstone called Cumberland, he told an audience at the meeting. A form of alcohol molecule may also be among the compounds analysed.
The preliminary result will excite scientists because fatty acids are key components of the cell membranes found in all life forms, including microbial organisms.
Dr Glavin told an audience that the result was “provocative”, and said the link to biology was the “million-dollar question”. But he explained that a non-biological origin was equally plausible at this stage of the research.
One scientist commenting on the presentation suggested that contamination could not be ruled out as a cause of the signal.
The SAM team have been working to address the leak of a pre-existing chemical called MTBSTFA within the instrument.
The fact this is also an organic molecule has complicated the search for indigenous carbon-containing compounds in Martian rocks.
However, team members say they have turned the leak into an advantage, using their understanding of how MTBSTFA reacts with other compounds to identify Martian organics.
The dust cloud surrounds Mars and reaches altitudes more than 1,000 kilometers (621 miles) from the planet’s surface, said MAVEN lead scientist Bruce Jakosky, also with University of Colorado.
“We think the source is the (Martian) atmosphere, however we have no process to take dust from low altitude to bring it up to 200 kilometers (124 miles). So if the source is the atmosphere, we don’t understand which process is moving them up,” Andersson said.
The dust also could have come from Mars’ moons, Phobos and Deimos, from dust in the solar wind or from comet dust that fills interplanetary space.
“If our hypothesis for Mount Sharp holds up, it challenges the notion that warm and wet conditions were transient, local, or only underground on Mars,” said Ashwin Vasavada, Curiosity deputy project scientist at NASA’s Jet Propulsion Laboratory in Pasadena, California. “A more radical explanation is that Mars’ ancient, thicker atmosphere raised temperatures above freezing globally, but so far we don’t know how the atmosphere did that.”
Why this layered mountain sits in a crater has been a challenging question for researchers. Mount Sharp stands about 3 miles (5 kilometers) tall, its lower flanks exposing hundreds of rock layers. The rock layers – alternating between lake, river and wind deposits – bear witness to the repeated filling and evaporation of a Martian lake much larger and longer-lasting than any previously examined close-up.
“We are making headway in solving the mystery of Mount Sharp,” said Curiosity Project Scientist John Grotzinger of the California Institute of Technology in Pasadena. “Where there’s now a mountain, there may have once been a series of lakes.”
Curiosity currently is investigating the lowest sedimentary layers of Mount Sharp, a section of rock 500 feet (150 meters) high, dubbed the Murray formation. Rivers carried sand and silt to the lake, depositing the sediments at the mouth of the river to form deltas similar to those found at river mouths on Earth. This cycle occurred over and over again.
“The great thing about a lake that occurs repeatedly, over and over, is that each time it comes back it is another experiment to tell you how the environment works,” Grotzinger said. “As Curiosity climbs higher on Mount Sharp, we will have a series of experiments to show patterns in how the atmosphere and the water and the sediments interact. We may see how the chemistry changed in the lakes over time. This is a hypothesis supported by what we have observed so far, providing a framework for testing in the coming year.”
After the crater filled to a height of at least a few hundred yards, or meters, and the sediments hardened into rock, the accumulated layers of sediment were sculpted over time into a mountainous shape by wind erosion that carved away the material between the crater perimeter and what is now the edge of the mountain.
On the 5-mile (8-kilometer) journey from Curiosity’s 2012 landing site to its current work site at the base of Mount Sharp, the rover uncovered clues about the changing shape of the crater floor during the era of lakes.Read more
Just as water-based snowfalls occur during winter in Mars’ northern hemisphere, carbon dioxide snowfalls occur in the planet’s southern hemisphere during the south pole’s own winter. Frozen CO2 persists in the southern region all year round, but how it got there is still a mystery. (via Does it snow on Mars? | Spaceanswers.com)Read more
A drive of 157 feet (48 meters) on July 27 put Opportunity’s total odometry at 25.01 miles (40.25 kilometers).This month’s driving brought the rover southward along the western rim of Endeavour Crater. The rover had driven more than 20 miles (32 kilometers) before arriving at Endeavour Crater in 2011, where it has examined outcrops on the crater’s rim containing clay and sulfate-bearing minerals. The sites are yielding evidence of ancient environments with less acidic water than those examined at Opportunity’s landing site.
If the rover can continue to operate the distance of a marathon — 26.2 miles (about 42.2 kilometers) — it will approach the next major investigation site mission scientists have dubbed “Marathon Valley.” Observations from spacecraft orbiting Mars suggest several clay minerals are exposed close together at this valley site, surrounded by steep slopes where the relationships among different layers may be evident.Read more
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See also:Read more "USGS Scientific Investigations Map 3292: Geologic Map of Mars "