Inside NASA’s Bold Moonshot to Find Life Orbiting Saturn

Photo Illustration by Thomas Levinson/The Daily Beast/Getty
Photo Illustration by Thomas Levinson/The Daily Beast/Getty

PASADENA, Calif.—From the snow-white Saturnian moon of Enceladus to the brown sludge of your local sewage treatment plant, a new piece of technology from NASA’s Jet Propulsion Laboratory might get the chance to do it all.

JPL’s scientists have designed a package of instruments dubbed the Ocean Worlds Life Surveyor (OWLS) to remotely and autonomously look for signs of life on the solar system’s water-laden bodies. Enceladus is a prime destination to search, as it’s known to have the chemical potential to host microbes—and therefore life.

But the same system that can probe water samples at the molecular and cellular levels some 746 million miles from Earth can do the same here—and wouldn’t it be valuable to have devices independently working 24/7 to remove pollution and contaminants from our waters? Or, while attached to a buoy far out to sea, on the watch for harmful algae blooms? A version is already wanted on the International Space Station to help monitor the orbital lab’s drinking water cleanliness, says the scientist leading the OWLS team.

“I think in time, this will be one of those NASA success stories where we invented something for a very specific extraterrestrial-type application and have found a lot of applications here on Earth as well,” OWLS co-principal investigator and science lead Peter Willis told The Daily Beast.

<div class="inline-image__caption"><p>NASA’s Cassini captured this image of the surface of Enceladus on Oct. 9, 2008.</p></div> <div class="inline-image__credit">NASA/JPL/Space Science Institute</div>

NASA’s Cassini captured this image of the surface of Enceladus on Oct. 9, 2008.

NASA/JPL/Space Science Institute

What makes OWLS groundbreaking is how it combines automation with innovative technologies such as microscopes with no moving parts and the ability to test liquids in zero gravity. Wind it up and let it run—and that’s exactly what makes it so lucrative for research on terra firma.

“Science, right now, is limited by graduate students. There are only so many of them, and you need them to stare at all the data all the time,” Lukas Mandrake, an instrument autonomy system engineer, told The Daily Beast. “Everything is shockingly manual… and that is limiting our ability to make discoveries. So this software has applications all over the place to alleviate that particular bottleneck.”

Mandrake comments came on the same day recent rains across Los Angeles flushed harmful bacteria into Santa Monica Bay. “That determination [of danger] is made by a human looking through a microscope for certain things moving in certain ways,” he explained. “If they don’t see it, they say it’s not dangerous. Wouldn’t it be nice if we could systematize that process?”

Following five years of development, Willis and his team ran OWLS through field testing at California’s Mono Lake earlier this summer. The equipment, currently the size of a few filing cabinets, successfully found chemical and cellular evidence of life in the salty water. Next steps, Willis said, are shrinking down the instruments and customizing them for specific missions.


Despite its promise, the timeline for the OWLS mission is a big question mark. “[I] don't think we would have data back in less than 15-ish years—and that's if everything goes perfectly,” Chris Lindensmith, the program’s microscope lead, told The Daily Beast.

Unfortunately, the slow pace of discoveries is just how space exploration works—especially when it comes to Enceladus. In fact, the Saturnian moon wasn’t discovered until 1789 by William Herschel (who later discovered Uranus). Nearly 200 years passed before the two Voyager spacecraft flew by on their tours of the outer solar system. In between, little knowledge was gained beyond specifics of the moon’s orbit, mass, density and reflectivity of light. And relative to the rest of the solar system, it’s tiny; Earth is more than 25 times larger.

But then Enceladus’ potential for harboring life was discovered in 2005, when the Cassini probe buzzed the moon—one of 83 in Saturn’s orbit not embedded in its signature rings. In a dramatic moment backlit by the sun, Cassini witnessed geysers on its surface shooting up more than 300 miles, spurting what later was determined to be mostly salty water vapor and ice, as well as sand. Some ejected material fell back to the surface like snow, explaining why Enceladus is the most reflective body in our solar system, but much of the spray traveled far enough to be ensnared by Saturn’s gravity to help form an outer ring.

<div class="inline-image__caption"><p>NASA’s Cassini captured this image of Enceladus on Nov. 30, 2010. The shadow of the body of Enceladus on the lower portions of the jets is clearly visible</p></div> <div class="inline-image__credit"> NASA/JPL-Caltech/Space Science Institute</div>

NASA’s Cassini captured this image of Enceladus on Nov. 30, 2010. The shadow of the body of Enceladus on the lower portions of the jets is clearly visible

NASA/JPL-Caltech/Space Science Institute

Molecular hydrogen, and nitrogen- and oxygen-bearing compounds were also discovered on the plumes. On Earth, similar compounds are part of chemical reactions producing amino acids, which are the building blocks of life. And found under the geysers at the south pole’s rocky interior was a source of heat that has yet to be fully explained.

By the time Cassini’s mission ended in 2017, it sent back home enough data for NASA to announce Enceladus’ external shell of frozen water, 25 miles thick in some places, floats atop a subsurface ocean with depths up to 19 miles.

Water. Heat. Rock. If you’re looking for extraterrestrial life, you could do far worse than start there.

“Then it was like, what more do you need? You’ve got this evidence of a habitable environment underneath a crust of ice,” Willis said.

Once on the scene, OWLS will look for life despite no one knowing what form life might take on in an ocean world. This makes it essential to include the broadest possible array of instruments, capable of measuring sizes ranging from single molecules to microorganisms.

That’s why the project combined two subsystems: chemical analysis techniques and microscopes. The chemical analysis system looks for biosignatures in the organic compounds, while the microscopes seek cells and their tell-tale motions.

To find chemical evidence of life, OWLS uses its Organic Capillary Electrophoresis Analysis System (OCEANS), which essentially pressure-cooks liquid samples and feeds them to instruments that search for amino acids, fatty acids, and other signs of microbial life. For example, microorganisms found on Earth called methanogens can use molecular hydrogen and carbon dioxide as a source of energy, combining them in a metabolism that generates methane—one of many chemical compounds also found in the plumes.

The OCEANS system is so sensitive, Willis compared it to a shark that can smell just one molecule of blood in a billion molecules of water—and then identify the blood type.

<div class="inline-image__caption"><p>The OWLS extractor uses pressure and temperature to perform subcritical water extraction, breaking cells down to their constituent organic molecules for chemical analysis.</p></div> <div class="inline-image__credit">NASA/JPL-Cal Tech</div>

The OWLS extractor uses pressure and temperature to perform subcritical water extraction, breaking cells down to their constituent organic molecules for chemical analysis.

NASA/JPL-Cal Tech

OWLS’ three microscopes—a system named ELVIS [Extant Life Volumetric Imaging System]—uses machine-learning algorithms to both home in on lifelike movement as well as detect objects lit up by fluorescent molecules, whether naturally occurring in living organisms or by added dyes.

Of course, these tests will generate a galactic amount of data, which must be transmitted back home at rates that make the chintziest dial-up modems of the primordial internet age look like optical fiber. In fact, it’s so tedious a task that it’s been compared to looking for a refrigerator’s light that’s orbiting Saturn while you’re on Earth.

Luckily, OWLS has “onboard science instrument autonomy,” which greatly compresses the data by selecting only the most valuable biosignatures to send back. It also keeps a manifest of what wasn’t sent in case something unexpected prompts further review. This way 10 gigabytes collected every minute can be condensed to five essential megabytes received daily on Earth.

“Scientists don't want to send a Roomba to space and say, ‘I hope you do a great job,’” Mandrake said. “They need summarization and prioritization of what to look at first and what is there, and then they want to dialogue with the spacecraft.”

Saturn May Have Gotten Its Rings by Murdering One of Its Moons

It was more than 40 years after NASA’s first up-close look at Enceladus before the space agency found clues that might lead to the discovery of extraterrestrial life there. And, as Lindensmith said, it’ll be at least another 15 before we receive data to confirm that hypothesis or shoot it down.

But in the near term, the technology of OWLS may soon appear in biomedical diagnostics, and the monitoring of water quality, and food or pharmaceutical processes. “We envision it being an open-source kind of instrument,” said Willis. “We don’t work for a company; we’re not trying to commercialize these things or make a profit off them.”

There may be no undertaking at JPL more ambitious than looking for extraterrestrial life, and answering the timeless question of whether we’re alone in the universe. OWLS should be a valuable tool in that lofty pursuit.

But in earthier matters, we down here need clean water to drink and safe food to eat. OWLS can help with that, too.

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