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Researchers model source of eruption on Jupiter's moon Europa by Staff Writers Stanford CA (SPX) Nov 11, 2020
On Jupiter's icy moon 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? A 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 from researchers at Stanford University, the University of Arizona, the University of Texas and NASA's Jet Propulsion Laboratory. 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, published Nov. 10 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.
Harbingers of life? 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," said lead author Gregor Steinbrugge, a postdoctoral researcher at Stanford's School of Earth, Energy and Environmental Sciences (Stanford Earth). The researchers focused their analyses on Manannan, 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," said co-author 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," Steinbrugge said. "It can move along thermal gradients, from cold to warm, and not only in the down direction as pulled by gravity."
A salty driver "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," said 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 Manannan 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 Manannan eruption could happen on other icy bodies - even without an impact event. "Brine pocket migration is not uniquely applicable to Europan craters," Voigt said. "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," said co-author 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."
Radiation Does a Bright Number on Jupiter's Moon Pasadena CA (JPL) Nov 10, 2020 As the icy, ocean-filled moon Europa orbits Jupiter, it withstands a relentless pummeling of radiation. Jupiter zaps Europa's surface night and day with electrons and other particles, bathing it in high-energy radiation. But as these particles pound the moon's surface, they may also be doing something otherworldly: making Europa glow in the dark. New research from scientists at NASA's Jet Propulsion Laboratory in Southern California details for the first time what the glow would look like, and wha ... read more
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