The selfie was taken on 11 October 2019 (Sol 2,553) in a location named “Glen Etive” (pronounced “glen EH-tiv”), which is part of the “clay-bearing unit”, a region the team has eagerly awaited reaching since before Curiosity launched.
Visible in the left foreground are two holes Curiosity drilled named Glen Etive 1 (right) and Glen Etive 2 (left) by the science team.
The rover can analyse the chemical composition of rock samples by powderising them with the drill, then dropping the samples into a portable lab in its belly called Sample Analysis at Mars (SAM).
About 984 feet (300 metres) behind the rover is Vera Rubin Ridge, which Curiosity departed nearly a year ago. Beyond the ridge, you can see the floor of Gale Crater and the crater’s northern rim. Curiosity has been ascending Mount Sharp, a 3-mile-tall (5-kilometre-tall) mountain inside the crater.
SAM principal investigator Paul Mahaffy of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, explained, “We’ve been eager to find an area that would be compelling enough to do wet chemistry. Now that we’re in the clay-bearing unit, we’ve finally got it.”
The special chemistry experiment occurred on 24 September 2019, after the rover placed the powderised sample from Glen Etive 2 into SAM. The portable lab contains 74 small cups used for testing samples.
Most of the cups function as miniature ovens that heat the samples; SAM then “sniffs” the gases that bake off, looking for chemicals that hold clues about the Martian environment billions of years ago, when the planet was friendlier to microbial life.
But nine of SAM’s 74 cups are filled with solvents the rover can use for special “wet chemistry” experiments. These chemicals make it easier for SAM to detect certain carbon-based molecules important to the formation of life, called organic compounds.
Because there’s a limited number of wet chemistry cups, the science team has been saving them for just the right conditions. In fact, the experiment at Glen Etive is only the second time Curiosity has performed wet chemistry since touching down on Mars in August 2012.
Clay-based rocks are good at preserving chemical compounds, which break down over time and when bombarded by radiation from space and the sun. The science team is intrigued to see which organic compounds, if any, have been preserved in the rocks at Glen Etive. Understanding how this area formed will give them a better idea of how the Martian climate was changing billions of years ago.
While this marks Curiosity’s second wet chemistry experiment, it is the rover’s first on a drilled sample. In December 2016, when Curiosity’s drill malfunctioned, the rover still had a bit of sand that had been scooped up in a place called “Ogunquit Beach”.
It wasn’t a drilled sample, but the team wasn’t sure whether they’d get the drill working and be able to perform wet chemistry in the future. So, they delivered the Ogunquit Beach sand into one of SAM’s wet chemistry cups since there was still science to be gained.
“SAM’s data is extremely complex and takes time to interpret. But we’re all eager to see what we can learn from this new location, Glen Etive,” said Mahaffy.
Scientists consider Glen Etive a strategic location that will reveal more about how the clay-bearing unit formed. They built upon the valuable dress rehearsal at Ogunquit Beach to make adjustments that improved the recent experiment.
MAHLI was built by Malin Space Science Systems in San Diego.
The SAM instrument suite was built at Goddard Space Flight Center, with significant elements provided by industry, university, and national and international NASA partners. NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Science Laboratory Project for the NASA Science Mission Directorate in Washington. JPL designed and built the project’s Curiosity rover.
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