New model could explain icy blast from Jupiter’s moon

A new model could explain hypothesized icy eruptions coming from Jupiter’s moon Europa.

On Europa, powerful eruptions may spew into space, raising questions among hopeful astrobiologists on Earth: What would blast out from miles-high plumes? Could they contain signs of extraterrestrial life? And where in Europa would they originate?

The new explanation now points to a source closer to the frozen surface than might be expected.

Rather than originating from deep within Europa’s oceans, some eruptions may originate from water pockets embedded in the icy shell itself, according to new evidence.

Using images collected by the NASA spacecraft Galileo, the researchers developed a model to explain how a combination of freezing and pressurization could lead to a cryovolcanic eruption, or a burst of water.

The results in Geophysical Research Letters have implications for the habitability of Europa’s underlying ocean—and may explain eruptions on other icy bodies in the solar system.

Signs of life?

Scientists have speculated that the vast ocean hidden beneath Europa’s icy crust could contain elements necessary to support life. But short of sending a submersible to the moon to explore, it’s difficult to know for sure. That’s one reason Europa’s plumes have garnered so much interest: If the eruptions are coming from the subsurface ocean, the elements could be more easily detected by a spacecraft like the one planned for NASA’s upcoming Europa Clipper mission.

But if the plumes originate in the moon’s icy shell, they may be less hospitable to life, because it is more difficult to sustain the chemical energy to power life there. In this case, the chances of detecting habitability from space are diminished.

“Understanding where these water plumes are coming from is very important for knowing whether future Europa explorers could have a chance to actually detect life from space without probing Europa’s ocean,” says lead author Gregor Steinbrügge, a postdoctoral researcher at Stanford University’s School of Earth, Energy & Environmental Sciences.

The researchers focused their analyses on Manannán, an 18-mile-wide crater on Europa that was created by an impact with another celestial object some tens of millions of years ago. Reasoning that such a collision would have generated a tremendous amount of heat, they modeled how melting and subsequent freezing of a water pocket within the icy shell could have caused the water to erupt.

“The comet or asteroid hitting the ice shell was basically a big experiment which we’re using to construct hypotheses to test,” says coauthor Don Blankenship, senior research scientist at the University of Texas Institute for Geophysics (UTIG) and principal investigator of the Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) instrument that will fly on Europa Clipper. “The polar and planetary sciences team at UTIG are all currently dedicated to evaluating the ability of this instrument to test those hypotheses.”

The model indicates that as Europa’s water transformed into ice during the later stages of the impact, pockets of water with increased salinity could be created in the moon’s surface. Furthermore, these salty water pockets can migrate sideways through Europa’s ice shell by melting adjacent regions of less brackish ice, and consequently become even saltier in the process.

“We developed a way that a water pocket can move laterally—and that’s very important,” Steinbrügge says. “It can move along thermal gradients, from cold to warm, and not only in the down direction as pulled by gravity.”

Freezing brine pocket on Europa

The model predicts that when a migrating brine pocket reached the center of Manannán crater, it became stuck and began freezing, generating pressure that eventually resulted in a plume, estimated to have been over a mile high. The eruption of this plume left a distinguishing mark: a spider-shaped feature on Europa’s surface that was observed by Galileo imaging and incorporated in the researchers’ model.

“Even though plumes generated by brine pocket migration would not provide direct insight into Europa’s ocean, our findings suggest that Europa’s ice shell itself is very dynamic,” says co-lead author Joana Voigt, a graduate research assistant at the University of Arizona, Tucson.

The relatively small size of the plume that would form at Manannán indicates that impact craters probably can’t explain the source of other, larger plumes on Europa that have been hypothesized based on Hubble and Galileo data, the researchers say. But the process modeled for the Manannán eruption could happen on other icy bodies—even without an impact event.

“Brine pocket migration is not uniquely applicable to Europan craters,” Voigt says. “Instead the mechanism might provide explanations on other icy bodies where thermal gradients exist.”

The study also provides estimates of how salty Europa’s frozen surface and ocean may be, which in turn could affect the transparency of its ice shell to radar waves. The calculations, based on imaging from Galileo from 1995 to 1997, show Europa’s ocean may be about one-fifth as salty as Earth’s ocean—a factor that will improve the capacity for the Europa Clipper mission’s radar sounder to collect data from its interior.

The findings may be discouraging to astrobiologists hoping Europa’s erupting plumes might contain clues about the internal ocean’s capacity to support life, given the implication that plumes do not have to connect to Europa’s ocean. However, the new model offers insights toward untangling Europa’s complex surface features, which are subject to hydrological processes, the pull of Jupiter’s gravity and hidden tectonic forces within the icy moon.

“This makes the shallow subsurface—the ice shell itself—a much more exciting place to think about,” says coauthor Dustin Schroeder, an assistant professor of geophysics at Stanford. “It opens up a whole new way of thinking about what’s happening with water near the surface.”

Additional coauthors are from the University of Texas at Austin; the University of Arizona, Tucson; and NASA’s Jet Propulsion Laboratory.

Support for the research came from the G. Unger Vetlesen Foundation. A portion of the work was carried out by the Jet Propulsion Laboratory at Caltech under a contract with NASA.

Source: Stanford University

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