The largest moon in our solar system, a companion to Jupiter named Ganymede,
might have ice and oceans stacked up in several layers like a club sandwich,
according to new NASA-funded research that models the moon's makeup.
Previously, the moon was thought to harbor a thick ocean sandwiched between
just two layers of ice, one on top and one on bottom.
"Ganymede’s ocean might be organized like a Dagwood sandwich," said Steve
Vance of NASA's Jet Propulsion Laboratory in Pasadena, Calif., explaining the
moon's resemblance to the "Blondie" cartoon character's multi-tiered sandwiches.
The study, led by Vance, provides new theoretical evidence for the team's "club
sandwich" model, first proposed last year. The research appears in the journal
Planetary and Space Science.
The results support the idea that primitive life might have possibly arisen
on the icy moon. Scientists say that places where water and rock interact are
important for the development of life; for example, it's possible life began on
Earth in bubbling vents on our sea floor. Prior to the new study, Ganymede's
rocky sea bottom was thought to be coated with ice, not liquid -- a problem for
the emergence of life. The "club sandwich" findings suggest otherwise: the first
layer on top of the rocky core might be salty water.
"This is good news for Ganymede," said Vance. "Its ocean is huge, with
enormous pressures, so it was thought that dense ice had to form at the bottom
of the ocean. When we added salts to our models, we came up with liquids dense
enough to sink to the sea floor."
NASA scientists first suspected an ocean in Ganymede in the 1970s, based on
models of the large moon, which is bigger than Mercury. In the 1990s, NASA's
Galileo mission flew by Ganymede, confirming the moon's ocean, and showing it
extends to depths of hundreds of miles. The spacecraft also found evidence for
salty seas, likely containing the salt magnesium sulfate.
Previous models of Ganymede's oceans assumed that salt didn't change the
properties of liquid very much with pressure. Vance and his team showed, through
laboratory experiments, how much salt really increases the density of liquids
under the extreme conditions inside Ganymede and similar moons. It may seem
strange that salt can make the ocean denser, but you can see for yourself how
this works by adding plain old table salt to a glass of water. Rather than
increasing in volume, the liquid shrinks and becomes denser. This is because the
salt ions attract water molecules.
The models get more complicated when the different forms of ice are taken
into account. The ice that floats in your drinks is called "Ice I." It's the
least dense form of ice and lighter than water. But at high pressures, like
those in crushingly deep oceans like Ganymede’s, the ice crystal structures
become more compact. "It's like finding a better arrangement of shoes in your
luggage -- the ice molecules become packed together more tightly," said Vance.
The ice can become so dense that it is heavier than water and falls to the
bottom of the sea. The densest and heaviest ice thought to persist in Ganymede
is called "Ice VI."
By modeling these processes using computers, the team came up with an ocean
sandwiched between up to three ice layers, in addition to the rocky seafloor.
The lightest ice is on top, and the saltiest liquid is heavy enough to sink to
the bottom. What's more, the results demonstrate a possible bizarre phenomenon
that causes the oceans to "snow upwards." As the oceans churn and cold plumes
snake around, ice in the uppermost ocean layer, called "Ice III," could form in
the seawater. When ice forms, salts precipitate out.
The heavier salts would
thus fall downward, and the lighter ice, or "snow," would float upward. This
"snow" melts again before reaching the top of the ocean, possibly leaving slush
in the middle of the moon sandwich.
“We don’t know how long the Dagwood-sandwich structure would exist," said
Christophe Sotin of JPL. "This structure represents a stable state, but various
factors could mean the moon doesn't reach this stable state.
Sotin and Vance are both members of the Icy Worlds team at JPL, part of the
multi-institutional NASA Astrobiology Institute based at the Ames Research
Center in Moffett Field, Calif.
The results can be applied to exoplanets too, planets that circle stars
beyond our sun. Some super-Earths, rocky planets more massive than Earth, have
been proposed as "water worlds" covered in oceans. Could they have life? Vance
and his team think laboratory experiments and more detailed modeling of exotic
oceans might help find answers.
Ganymede is one of five moons in our solar system thought to support vast
oceans beneath icy crusts. The other moons are Jupiter's Europa and Callisto and
Saturn's Titan and Enceladus.
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