Saturn's
moon Enceladus. Credit: NASA
What are the chances of finding
extraterrestrial life in our solar system? Frank Postberg, a professor of
planetary science at Freie Universität Berlin, has published a study in Science Advances with an international team of researchers. They
present new evidence that it is easier to determine the constituents of the
ocean hidden beneath Enceladus's icy surface than previously assumed.
Postberg also contributed to a
second study published the same day. In that study, he and another planetary
scientist from Freie Universität, Dr. Nozair Khawaja, helped show that certain
microorganisms could tolerate the conditions in Enceladus's ocean better than
previously thought. The results increase the likelihood of finding evidence of
life on Saturn's moon.
What makes Enceladus so attractive in the search for life in space?
Enceladus is considered one of the
most promising places to search for extraterrestrial life in our solar system.
Researchers suspect that a global ocean of liquid water lies beneath the moon's
icy crust, with a rocky core farther below. Due to cryovolcanic activity,
gigantic plumes break through cracks in the crust at the moon's south pole,
ejecting ice particles hundreds of kilometers into space.
NASA's Cassini spacecraft passed
through these plumes multiple times to analyze their composition. Enceladus's
ocean is the only extraterrestrial "body of water" from which
scientists have been able to directly analyze samples. The samples revealed
traces of various salts and organic compounds. Previous analyses by Cassini
also indicated hydrothermal processes on the seafloor and other conditions that could support life.
Enceladus ice plumes separate and sort the ocean's components
Postberg's study, "Cassini CDA
Observes Compositional Segregation of Enceladus' Ice Grains from Slow Freezing
and Fragmentation of Oceanic Spray," includes surprising findings about
what happens to the ocean water on its way into space. The international team
used Cassini data, long-term laboratory experiments and theoretical models to
reconstruct the process.
Droplets form at the ocean's
surface as gas-filled bubbles rise and pop. Water vapor then carries the
droplets through cracks in the ice shell and out into space. Scientists
previously believed the droplets froze instantaneously. The new findings reveal
that they freeze slowly, allowing most components (including dissolved ones) to
separate from each other. Salts and organic materials are thus distributed in
different locations inside each freezing droplet. Various types of previously
dissolved salts also separate; for example, sodium chloride (table salt)
separates from sodium carbonate.
On their way up, the frozen
droplets accelerate to speeds of up to 1,000 km/h (620 miles per hour). If they
hit the walls of the icy cracks, they break into fragments only a few
micrometers in size before shooting into space. As a result, ice particles often
consist of just one highly concentrated, previously segregated substance.
"Enceladus actually does a lot
of the work for us in preparing samples for analysis that usually take a lot of
effort in chemical labs on Earth," says Postberg, who led the study.
"The oceanic constituents are separated from each other and simultaneously
concentrated into individual ice particles."
Making it easier to find signs of life
This mechanism helps researchers
characterize the ocean as a potential habitat for life. It is also particularly
useful in the search for biosignatures, or measurable indications of life. If an ocean
droplet contained components from alien microbes, those components could
separate from others as the droplet froze. After fragmentation, the microbial
material might be found in only a small fraction of ice particles. In those
particles, however, it would be highly concentrated and relatively pure.
"That is great news in the
search for life," says Postberg. "Future spacecraft will have to
analyze many individual ice particles in the plume. But if they come across one
with microbial material in it, they could identify biosignatures in the
particle relatively easily with already available technology."
The discovery could have important
implications for future space missions to Enceladus, such as the ESA's L4
mission, which is being planned. The mission will specifically look for signs
of life on Saturn's moon. Postberg's lab at Freie Universität Berlin has
previously conducted laboratory studies demonstrating that specialized
instruments can detect microbial cellular material in individual particles from
the ice plumes.
Could life really exist on Enceladus?
A recent study offers new insight
into this question. On the same day Postberg's article appeared in Science Advances, scientists at
Ludwig-Maximilians-Universität München (LMU) published another article in the
journal: "Enceladus-Like Geochemistry Fuels Methanogenesis under Extreme
CO₂-Limitation." Postberg and
Khawaja contributed to the study.
The scientists reproduced the
conditions of Enceladus's ocean in a laboratory. The ocean has a very low
concentration of oxygen, a very high concentration of carbonate and is very alkaline (with pH values of 10 or 11). After recreating these
conditions, including the ocean's hydrothermal interaction with its rocky
floor, they introduced Methanothermococcus okinawensis into the simulated
environment.
This microorganism is a
methane-producing archaean that normally lives near deep-sea hydrothermal vents
on Earth. It does not need oxygen, which is rare on Enceladus, to survive. Its
metabolism requires only hydrogen and carbon dioxide.
The results were surprising: The
organism failed to grow in an optimal laboratory medium at such a high pH
because it lacked dissolved carbon dioxide. By contrast, it continued to grow
in the Enceladus simulant, producing methane using hydrogen generated by
water-rock reactions. Under the simulated conditions, the microorganisms were
even able to adapt their metabolism to the low amounts of carbon dioxide.
"This was really a surprise to us," Khawaja said. "This was an
experiment for which we did not expect such a successful outcome."
Taken together, the two studies in Science Advances shed new light on the search for extraterrestrial life. "On Enceladus the specific geochemical conditions might allow one of the oldest known metabolic systems on Earth to work, even in very alkaline environments," Postberg says. "While that doesn't mean that there is life on Saturn's moon, our first study shows that—in the event that there is—future space missions might have a good chance of finding traces if they analyze individual ice grains from Enceladus's plume."
Provided by Free University of Berlin
Source: Great news from Saturn's moon Enceladus in the search for life in space

