Wednesday, December 1, 2021

Clays, Not Water, Are Likely Source of Lakes on Mars

Lakes on Mars might not be lakes after all. Three studies published in the past month have cast doubt on the premise of there being subsurface lakes below the Martian south pole. Where there’s water, there’s life. That’s the case on Earth, at least, and also why scientists remain tantalized by any evidence suggesting there’s liquid water on cold, dry Mars.

The Red Planet is a difficult place to look for liquid water. While water ice is plentiful, any water warm enough to be liquid on the surface would last for only a few moments before turning into vapor in Mars’ wispy air. Hence, the interest generated in 2018 when a team, led by Roberto Orosei of Italy’s Istituto Nazionale di Astrofisica, announced they had found evidence of subsurface lakes on Mars deep below the ice cap at Mars’ south pole. The evidence they cited came from a radar instrument aboard the ESA (European Space Agency) Mars Express orbiter.

What appears to be lakes on Mars may actually be reflections from clay.
This image taken by NASA’s Mars Reconnaissance Orbiter shows ice sheets at Mars’ south pole. The spacecraft detected clays nearby this ice; scientists have proposed such clays are the source of radar reflections that have been previously interpreted as liquid water. (Image: NASA / JPL-Caltech /University of Arizona / JHU)

Radar signals, which can penetrate rock and ice, change as they’re reflected off different materials. In this case, they produced especially bright signals beneath the polar cap that could be interpreted as liquid water. The possibility of a potentially habitable environment for microbes was exciting. But after taking a closer look at the data, along with experiments in a cold laboratory here on Earth, some scientists now think clays, not water, might be creating the signals. In the past month, a trio of new papers have unraveled the mystery — and may have dried up the hypothesis about lakes on Mars.

A scientific ecosystem

Martian polar scientists belong to a small, tight-knit community. Not long after the lakes paper was published, about 80 of those scientists met for the International Conference on Mars Polar Science and Exploration in Ushuaia, a seaside village at the southern tip of Argentina.

The colored dots represent sites where bright radar reflections have been spotted by ESA’s Mars Express orbiter at Mars’ south polar cap. Such reflections were previously interpreted as subsurface liquid water, but their prevalence and proximity to the frigid surface suggest they may be something else. (Image: ESA / NASA / JPL-Caltech)

Gatherings like these provide an opportunity to test new theories and challenge each other’s perspectives. Jeffrey Plaut of NASA’s Jet Propulsion Laboratory, who is also the co-principal investigator, along with Orosei, of the instrument behind the intriguing radar signals, called MARSIS, or the Mars Advanced Radar for Subsurface and Ionospheric Sounding, said:

“Communities can generate their own little scientific ecosystems. These communities can be self-sustaining, because you bounce a question off someone and maybe a year or two later they help you figure out an answer.”

Subsurface lakes on Mars

Lots of talk centered on the subsurface lakes on Mars. How much heat would it take to keep water liquid under all that ice? Could brine be lowering the freezing point of the water enough to keep it liquid? Of course, it wouldn’t be the first time an exciting water-related hypothesis set off a flurry of investigations. In 2015, NASA’s Mars Reconnaissance Orbiter found what looked like streaks of damp sand running down slopes, a phenomenon called “recurring slope lineae.” But repeated observations using the spacecraft’s HiRISE — or High-Resolution Imaging Science Experiment — camera have since revealed this is more likely the result of sand flows.

A paper released earlier this year found many recurring slope lineae after a global dust storm on Mars in 2018. The finding suggested that dust settling on slopes triggers sand flows, which, in turn, expose the darker subsurface materials that give the lineae their distinctive coloration. As with the damp-sand hypothesis, several scientists began thinking up ways to test the hypothesis regarding subsurface lakes on Mars. Isaac Smith of York University in Toronto, who led the most recent study showing that clays can explain the observations, said:

“There was a feeling that we should try to address this.”

Too cold for lakes on Mars

Among those scientists was Plaut. He and Aditya Khuller, an Arizona State University doctoral student who was interning at JPL, analyzed 44,000 radar echoes from the base of the polar cap across 15 years of MARSIS data. They turned up dozens more bright reflections like the ones in the 2018 study. But in their recent paper published in Geophysical Research Letters, they found many of these signals in areas close to the surface, where it should be too cold for water to remain liquid, even when mixed with perchlorates, a kind of salt commonly found on Mars that can lower the freezing temperature of water.

Isaac Smith of Toronto’s York University bundled up while working in a lab, freezing smectite clays with liquid nitrogen to test how they respond to radar signals. The results have challenged the hypothesis that subsurface lakes can be found at Mars’ south pole. (Image: York University / Craig Rezza)

Two separate teams of scientists then analyzed the radar signals to determine whether anything else could be producing those signals. Carver Bierson of ASU completed a theoretical study suggesting several possible materials that could cause the signals, including clays, metal-bearing minerals, and saline ice. But York University’s Isaac Smith, knowing that a group of clays called smectites were present all over Mars, went further in a separate, third paper: He measured smectite properties in a lab.

Smectites look like ordinary rocks, but they were formed by liquid water long ago. Smith put several smectite samples into a cylinder designed to measure how radar signals would interact with them. He also doused them with liquid nitrogen, freezing them to minus 58°F (minus 50°) — close to what they would be at the Martian south pole. Smith said:

“The lab was cold. It was winter in Canada at the time, and pumping liquid nitrogen into the room made it colder. I was bundled up in a hat, jacket, gloves, scarf, and a mask because of COVID-19. It was pretty uncomfortable.”

After freezing the clay samples, Smith found their response nearly perfectly matched the MARSIS radar observations. Then, he and his team checked for clays present on Mars near those radar observations. They relied on data from MRO, which carries a mineral mapper called the Compact Reconnaissance Imaging Spectrometer, or CRISM. Bingo. While CRISM can’t peer through ice, Smith found smectites scattered in the vicinity of the south pole’s ice cap.

Smith’s team demonstrated that frozen smectite can make the reflections — no unusual amounts of salt or heat are required — and that they’re present at the south pole. There’s no way to confirm what the bright radar signals are without landing at Mars’ south pole and digging through miles of ice. But the recent papers have offered plausible explanations that are more logical than liquid water. Plaut said:

“In planetary science, we often are just inching our way closer to the truth. The original paper didn’t prove it was water, and these new papers don’t prove it isn’t. But we try to narrow down the possibilities as much as possible in order to reach consensus.”

Provided by: NASA [Note: Materials may be edited for content and length.]

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Troy Oakes
Troy was born and raised in Australia and has always wanted to know why and how things work, which led him to his love for science. He is a professional photographer and enjoys taking pictures of Australia's beautiful landscapes. He is also a professional storm chaser where he currently lives in Hervey Bay, Australia.
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