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Expeditions Story Searching for Life Where the Sun Don’t Shine (part 5): Explorations to the Seafloors of Earth and Europa
Searching for Life Where the Sun Don’t Shine (part 5): Explorations to the Seafloors of Earth and Europa
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Extreme Life
Posted:   02/07/13
Author:    Garret Fitzpatrick

Summary: This series follows an oceanographic expedition to the Mid-Cayman Rise and NASA's efforts to plan a future mission to Jupiter's moon, Europa. In part five, scientists use high-tech submersibles to explore the seafloor and bring intriguing samples up to the surface.

 

Chris German explains the dive plan. Credit: Woods Hole Oceanographic Institution (WHOI)

This is Part 5 of a 6-part series telling the story of humankind’s efforts to understand the origins of life, by looking for it in extreme environments where life thrives without relying on the Sun as an energy source. It follows an oceanographic expedition to the Mid-Cayman Rise led by Chris German of the Woods Hole Oceanographic Institution, and NASA’s efforts to plan a future mission to Jupiter’s moon, Europa. By understanding how life can live without the Sun we may discover how life began on our planet, and whether or not Earth is the only place in the universe capable of supporting a biosphere.



As he watched Florida recede in the distance, thoughts of the journey behind and the one lying before Chris German filled a hopeful mind. “Deep joy,” describes German, reflecting on his outlook at the start of the expedition. “The mystery (of the existence of the vent sites) had already been removed by the 2009 & 2011 expeditions so we knew exactly where to go, I had the best kit on the planet to sample with in ROV Jason and in my NASA/NSF team I had assembled some of the best experts in the world, who have also become my friends along the way, to take out and sample the site with,” says German. “It couldn't get much better.”

This voyage to the Mid-Cayman Rise (MCR) was planned to last 22 days. In 28 years of exploring since he began his PhD studies at the University of Cambridge, German has spent around a thousand days at sea, about on par for a modern day oceanographer. It’s a life of discovery and adventure but it also demands sacrifices—while at sea he’s missed his wife’s birthday (twice), his older son Martin’s 18th birthday, and his daughter Helen’s 16th birthday (while in the Antarctic).

Jason returns from its last dive of the expedition. Credit: WHOI
Now on Atlantis, bearing down on potentially the most significant sampling of hydrothermal vent sites on the planet, German hoped real discoveries would be waiting for the team somewhere about 400 miles south of Havana.

In addition to grabbing temperature readings, biological samples and close-up shots of the vents, German and his colleagues wanted to study the MCR for what it can tell us about Earth’s history. Since the MCR is an ultraslow spreading ridge, it acts differently than its faster counterparts. Usually rocks get older the farther you go from the spreading center of a mid-ocean ridge. That’s because new seafloor is being created by magma erupting and then cooling and molding together with the older surrounding seafloor. But at ultraslow spreading ridges, the rate of magma generation doesn’t always keep pace with the rate at which tectonic plates are being pulled apart by subduction processes. These processes may be nearby or many thousands of miles distant at the far end of the plate, where older, colder, and more dense sections of ocean crust sink back into the underlying mantle.

Along key sections of the MCR, this movement of tectonic plates resembles a condition you may find on your bookshelf. Imagine removing a bookend to allow a row of books to tilt over on their sides. The upper face of a book cover that slides up and into view is like the rock that formed deep beneath the seafloor but has now slid up to be exposed at the seafloor where seawater-rock interactions can give rise to unusual hydrothermal systems. Importantly, even though these rocks were formed relatively recently in geologic time, they very closely resemble the compositions of the lavas that used to erupt at the seafloor back during the first 2-2.5 billion years of Earth history. Here we find a system in the modern world that may be very close to what hydrothermal systems were like during the brief but legendary lifetime of our good friend, Earth Life Form #1.

Jason sampling a hydrothermal plume. Credit: WHOI
At 9:45 p.m. on January 8, Atlantis reached her destination above a hydrothermal vent site called Von Damm—named after the late geochemist Karen Von Damm. After two and a half days in transit, the ship rocked in the calm waves, keeping relatively stationary by use of one bow thruster and the stern propellers since her anchors couldn’t reach the seafloor, 7,500 feet below.

On the deck beneath two 42,000-pound capacity cranes sat the Remotely Operated Vehicle (ROV) Jason, named after an ancient Greek mythological hero famous for leading a group of adventurers called the Argonauts. Jason is the most capable U.S. academic research vessel roaming the seas today, able to reach 99% of the world’s seafloor at depths down to 21,000 feet.

The vehicle is also nearly indefatigable. It can work 24 hours a day with the help of a pilot, navigator, engineer, and three scientists. That means teams of six rotate through four-hour shifts, allowing Jason to remain submerged for many days at a time for continuous imaging, observation and sampling.

Tethered to Jason is it’s partner vehicle Medea, which serves as something of a shock absorber for the Greek hero. Any yanks on the line from Atlantis are transferred down to Medea, which maintains enough slack in the fiberoptic cable to allow Jason to roam around within 115 feet of Medea. (In Greek mythology, Medea was Jason’s wife.)

Tubeworms. Credit: WHOI
Chris German is thankful for his robotic helpers and their human watchmen. He relies heavily on the engineering team for real-time adjustments to the dive plan and troubleshooting the Jason/Medea vehicles. Without the team’s constant attention to the robots, there are no photos of vents, samples of tubeworms, or up-close sonar mapping of the seafloor. He recalls a saying from Captain Dale of his 2009 expedition, who said, “Robots are like dogs: they’ll do their best, but neither one is any better than the person who trained them.”

The next day, the engineering team had Jason ready to go by noon, but a few technical difficulties pushed the inaugural dive back a few hours. By 4:30 p.m., Jason was on the ocean bottom with all systems running. Its first photos from the deep were of weathered rock outcrops, a few fish and shrimp, mussels and tubeworms. Data were displayed in an operations van—a mobile boxcar of screens and instrument displays for monitoring Jason’s progress that shared the deck of Atlantis with a host of equipment. Using its manipulator arms, Jason collected five tubeworms, a clam, and a sea cucumber.

The science teams started working their round-the-clock shifts. Twenty-three people from nine institutions in three countries made up seven science teams. There was the Carbon Team made of Max Coleman and Sarah Bennett from NASA’s JPL. They wanted to track the state of carbon as it exits from the vent sites and how it gets altered through the food chain. “We’re looking at the whole carbon cycle, from abiotic carbon production deep within the crust, to biotic carbon production through chemosynthesis,” says Bennett. “If hydrothermal systems were to exist on Europa, it’s studies like this that may help us to calculate the biomass that may exist.”

Just about everything seems to revolve around carbon. It’s an organic element, so the biologists study it because it tells you something about how life has evolved there. It’s preserved in rocks, so the geologists want to measure it to figure out the ages of their samples. It gets spouted from superheated vents, so the chemists want to know what it mixes with.

View from the ROV operations van. Credit: WHOI
That’s why Coleman and Bennett are part of each of the other teams as well—the Plume, Biology, Geology, Fluids and Microbiology Teams—in order to get at the bigger picture of all things carbon in and around the vent systems.

After Jason’s first dive was declared a success, the crew of Atlantis brought the ROV back up to the surface. Securing Jason and Medea to the deck and distributing samples among eager science teams, Atlantis made for the second target, named the Piccard vent site (named after late undersea explorer Jacques Piccard), merely two hours’ drive away.

******



By the time Jason submerged for its tenth and final dive of the expedition, Chris German and his team could already declare this mission a success. The team had returned to the Von Damm site for a final look at the rocks surrounding the hydrothermal system.

In the operations van aboard Atlantis, the Geology Team looked on—Guy Evans and Frieder Klein from Woods Hole and Matt Hodgkinson from the University of Southampton in the U.K. Unless you have the right rocks yielding the right chemistry, you won’t get the right conditions for life, regardless of what planet you’re on. At least as far as life as we know it goes. We’ve been wrong before.

Geologist Frieder Klein from WHOI with a tough chunk of basalt. Credit: WHOI
“There are some conditions you need to understand when thinking about the origin of life," says Klein. "The key components are pH, hydrogen concentration, methane, CO2, and temperature, which we try to constrain using the rock record.”

A particularly interesting rocky outcrop north of the vent site appeared on the screens at around 9:00 p.m. The ROV pilot reached out with Jason’s robotic arms to grab hold of the rock and pull. The rock didn’t budge. He tried again, maneuvering Jason’s arms to try a different angle. Still, nothing moved. After an hour-long struggle and with more biology and fluid samples to collect, Chris German called off the assault. The team dubbed the outcropping ‘kryptonite.’

By 4:00 a.m., Jason and Medea were still at work and Evans, Klein, and Hodgkinson came back to the operations van to resume the rock hunt after a brief rest. At 6:00 a.m. Jason returned to the area where it had wrestled with the “kryptonite”. A near-identical outcrop once again filled the screens and the team resumed the attack. Thirty minutes later, Jason’s strength was still no match for the rock. With another thirty minutes left of the team’s final dive, the Geology Team decided to move on to look for a more pliable sample.

Thus far, samples of mantle rocks—the ancient seafloor thought to be dragged up by the sliding-book-on-the-bookshelf tectonic plate at this ultraslow spreading ridge—had not been collected. If found, these rocks would help tell the story of the early ocean seafloor and, potentially, the environment surrounding the original genesis of life. The Geology Team wondered if Jason was wrestling with a primordial clue.

Beebe vents 1 - 4. Credit: WHOI
Fifteen minutes before the end of the dive, the team found a third outcropping—similar in composition but slightly more weathered than the previous two. They decided to let their robotic friend engage in one final boulder brawl.

With three minutes left on the clock, Jason, leader of the Argonauts, broke free a chunk of the “kryptonite” the size of a Thanksgiving turkey-serving platter.

Back on deck, it didn’t turn out to be kryptonite at all! Only basalt. Tough, tough, layered basalt—a common form of volcanic deposit on the seafloor. Interesting, but not the clue they were looking for.

Maybe the sought-after mantle rocks were covered in sediment. Maybe they weren’t there after all. Or maybe they were still buried beneath the seafloor—shallow enough to interact with the circulating seawater but not exposed at the seabed. That, along with a continuous stream of unresolved questions reflecting the eternal curiosity and resiliency of the human spirit, will be up to future explorers to battle.


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Searching for Life Where the Sun Don’t Shine (part 1): Explorations to the Sea Floors of Earth and Europa
Searching for Life Where the Sun Don’t Shine (part 2): Explorations to the Sea Floors of Earth and Europa
Searching for Life Where the Sun Don’t Shine (part 3): Explorations to the Seafloors of Earth and Europa
Searching for Life Where the Sun Don’t Shine (part 4): Explorations to the Seafloors of Earth and Europa
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