Cassini discovered the water-ice plumes on Enceladus in 2005. These plumes, emitted from fractures near its south pole, expel tiny ice grains and vapor, some of which escape the moon’s gravity, replenishing Saturn’s outermost ring, the E-ring.

“We believe that the salty material deep inside Enceladus washed out from rock at the bottom of a liquid layer,” said Frank Postberg, Cassini scientist. Postberg is lead author of a study that appears in the 25 June issue of the journal Nature.

Scientists working on the Cosmic Dust Analyzer conclude that liquid water must be present because it is the only way to dissolve significant amounts of minerals to account for the levels of salt detected. The process of sublimation — the mechanism by which vapor is released directly from solid ice in the crust — cannot account for the presence of salt.

The makeup of the E-ring grains, determined through the chemical analysis of thousands of high-speed particle hits registered by Cassini, provides indirect information about the composition of the plumes and about what lies inside Enceladus. The E-ring particles are almost pure water-ice, but nearly every time the dust analyzer checked for composition, it found at least some sodium within the particles.

“If the liquid source is an ocean, then that, coupled with heat measured at the surface near the moon’s South Pole and the organic compounds found within the plumes, could provide a suitable environment on Enceladus for the formation of life precursors”

“Our measurements imply that besides table salt, the grains also contain carbonates like soda; both components in concentrations that match the predicted composition of an Enceladus ocean,” said Postberg. “The carbonates also provide a slightly alkaline pH value. If the liquid source is an ocean, then that, coupled with the heat measured at the surface near the moon’s South Pole and the organic compounds found within the plumes, could provide a suitable environment on Enceladus for the formation of life precursors.”

In another study published in Nature, researchers doing ground-based observations did not see sodium, an important component of salt. That team notes that the amount of sodium being expelled from Enceladus is actually less than what is observed around many other planetary bodies. These scientists were looking for sodium in the plume vapor and couldn’t see it in the expelled ice grains. They argue that, if the plume vapor does come from ocean water, then the evaporation must happen slowly deep underground, rather than as a violent geyser erupting into space.

Finding salt in the plume gives evidence for liquid water below the surface. The lack of detection of sodium vapor in the plume gives hints about what the water reservoir might look like,” said Sascha Kempf, Cassini scientist.

Postberg added, "The original picture of the plumes as violently erupting Yellowstone-like geysers is changing. They seem more like steady jets of vapor and ice fed by a large water reservoir. However, we can’t decide yet if the water is currently ’trapped’ within huge pockets in Enceladus’s thick ice crust or is still connected to a large ocean in contact with the rocky core."

"Potential plume sources on Enceladus are an active area of research with evidence continuing to converge on a possible salt-water ocean," said Linda Spilker, Cassini deputy project scientist. "Our next opportunity to gather data on Enceladus will come during two flybys in November."

“The discovery of the Enceladus plume is one of the top scientific achievements of the Cassini-Huygens mission so far. These new results are inviting Cassini to making further in situ analysis of their composition; they are also whetting our appetite to further investigate whether Enceladus is habitable.” said Jean-Pierre Lebreton, ESA’s Huygens Project Scientist.

ESA

Cassini discovered the water-ice plumes on Enceladus in 2005. These plumes, emitted from fractures near its south pole, expel tiny ice grains and vapor, some of which escape the moon’s gravity, replenishing Saturn’s outermost ring, the E-ring.

“We believe that the salty material deep inside Enceladus washed out from rock at the bottom of a liquid layer,” said Frank Postberg, Cassini scientist. Postberg is lead author of a study that appears in the 25 June issue of the journal Nature.

Scientists working on the Cosmic Dust Analyzer conclude that liquid water must be present because it is the only way to dissolve significant amounts of minerals to account for the levels of salt detected. The process of sublimation — the mechanism by which vapor is released directly from solid ice in the crust — cannot account for the presence of salt.

The makeup of the E-ring grains, determined through the chemical analysis of thousands of high-speed particle hits registered by Cassini, provides indirect information about the composition of the plumes and about what lies inside Enceladus. The E-ring particles are almost pure water-ice, but nearly every time the dust analyzer checked for composition, it found at least some sodium within the particles.

“If the liquid source is an ocean, then that, coupled with heat measured at the surface near the moon’s South Pole and the organic compounds found within the plumes, could provide a suitable environment on Enceladus for the formation of life precursors”

“Our measurements imply that besides table salt, the grains also contain carbonates like soda; both components in concentrations that match the predicted composition of an Enceladus ocean,” said Postberg. “The carbonates also provide a slightly alkaline pH value. If the liquid source is an ocean, then that, coupled with the heat measured at the surface near the moon’s South Pole and the organic compounds found within the plumes, could provide a suitable environment on Enceladus for the formation of life precursors.”

In another study published in Nature, researchers doing ground-based observations did not see sodium, an important component of salt. That team notes that the amount of sodium being expelled from Enceladus is actually less than what is observed around many other planetary bodies. These scientists were looking for sodium in the plume vapor and couldn’t see it in the expelled ice grains. They argue that, if the plume vapor does come from ocean water, then the evaporation must happen slowly deep underground, rather than as a violent geyser erupting into space.

Finding salt in the plume gives evidence for liquid water below the surface. The lack of detection of sodium vapor in the plume gives hints about what the water reservoir might look like,” said Sascha Kempf, Cassini scientist.

Postberg added, "The original picture of the plumes as violently erupting Yellowstone-like geysers is changing. They seem more like steady jets of vapor and ice fed by a large water reservoir. However, we can’t decide yet if the water is currently ’trapped’ within huge pockets in Enceladus’s thick ice crust or is still connected to a large ocean in contact with the rocky core."

"Potential plume sources on Enceladus are an active area of research with evidence continuing to converge on a possible salt-water ocean," said Linda Spilker, Cassini deputy project scientist. "Our next opportunity to gather data on Enceladus will come during two flybys in November."

“The discovery of the Enceladus plume is one of the top scientific achievements of the Cassini-Huygens mission so far. These new results are inviting Cassini to making further in situ analysis of their composition; they are also whetting our appetite to further investigate whether Enceladus is habitable.” said Jean-Pierre Lebreton, ESA’s Huygens Project Scientist.

ESA