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Shards of pure ice might snow upwards beneath the ice shell of Europa

The moons Europa and Enceladus probably have global oceans buried beneath their frozen shells, and those seas may be home to a strange kind of ice called frazil ice
Original Caption Released with Image: The puzzling, fascinating surface of Jupiter's icy moon Europa looms large in this newly-reprocessed color view, made from images taken by NASA's Galileo spacecraft in the late 1990s. This is the color view of Europa from Galileo that shows the largest portion of the moon's surface at the highest resolution. The view was previously released as a mosaic with lower resolution and strongly enhanced color (see PIA02590). To create this new version, the images were assembled into a realistic color view of the surface that approximates how Europa would appear to the human eye. The scene shows the stunning diversity of Europa's surface geology. Long, linear cracks and ridges crisscross the surface, interrupted by regions of disrupted terrain where the surface ice crust has been broken up and re-frozen into new patterns. Color variations across the surface are associated with differences in geologic feature type and location. For example, areas that appear blue or white contain relatively pure water ice, while reddish and brownish areas include non-ice components in higher concentrations. The polar regions, visible at the left and right of this view, are noticeably bluer than the more equatorial latitudes, which look more white. This color variation is thought to be due to differences in ice grain size in the two locations. Images taken through near-infrared, green and violet filters have been combined to produce this view. The images have been corrected for light scattered outside of the image, to provide a color correction that is calibrated by wavelength. Gaps in the images have been filled with simulated color based on the color of nearby surface areas with similar terrain types. This global color view consists of images acquired by the Galileo Solid-State Imaging (SSI) experiment on the spacecraft's first and fourteenth orbits through the Jupiter system, in 1995 and 1998, respectively. Image scale is 1 mile (1.6 kilometers) per pixel. North on Europa is at right. The Galileo mission was managed by NASA's Jet Propulsion Laboratory in Pasadena, California, for the agency's Science Mission Directorate in Washington. JPL is a division of the California Institute of Technology, Pasadena. Additional information about Galileo and its discoveries is available on the Galileo mission home page at http://solarsystem.nasa.gov/galileo/. More information about Europa is available at http://solarsystem.nasa.gov/europa. Image Credit: NASA/JPL-Caltech/SETI Institute
The surface of Jupiter’s moon Europa is an icy shell
NASA/JPL-Caltech/SETI Institute

Beneath the frozen shell of Europa, flakes of ice may float upwards like strange underwater snow. The sparkling landscape formed by this process on the underside of the shell could be a favourable environment for alien life.

On Earth, the ice shelves in Antarctica are the closest analogue to the ice shells of Jupiter’s moon Europa and Saturn’s moon Enceladus, which are both thought to host global oceans beneath their frozen surfaces. There are two types of ice in the ice shelves: congelation ice, which starts in one spot and then spreads out as water freezes onto its edges, and frazil ice, which forms when supercooled water turns into ice crystals that then float up to settle beneath the shelf.

at the University of Texas at Austin and her colleagues compared measurements of Antarctic ice with observations and models of the ice on Enceladus and Europa to figure out which sort of ice we should expect there. They found that frazil ice could be common on both worlds, especially in areas where the ice shell is fractured, such as Enceladus’ famous “tiger stripes”.

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Both frazil and congelation ice are generally less salty than the ocean water from which they form, but frazil ice tends to be particularly pure at around 0.1 per cent of the salinity of the underlying water. “How the ice freezes matters a lot for how salty the ice would be,” says Wolfenbarger. “There’s a chance that the ice could be a lot more pure than has been previously estimated.”

Understanding the relationship between the salinity of the ice and that of the water could help us understand the conditions in the oceans of Enceladus and Europa, even if we can’t drill down to sample them directly. The salinity of these oceans is crucial for the possibility of microbial life there, because any organisms may not be able to survive if the water is too salty.

The likely presence of frazil ice is particularly intriguing because it is porous and could bring nutrients from deep underwater up to the bottom of the ice as it snows onto the underside of the shell. “At the bottom of the ice shelf it could be pretty mushy, and that’s an environment that organisms like to inhabit,” says Wolfenbarger. “We have actually seen protists in these environments on Earth, which hints that these might be good environments to look for life – assuming we can get to them.”

Astrobiology

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Topics: Moons