Icy Saturn Moon May Be Covering a Salty Sea

Saturn Moon Riddled with Gushing Geysers, New Images Reveal
Dramatic plumes, both large and small, spray water ice out from many locations along the famed "tiger stripes" near the south pole of Saturn's moon Enceladus in this image taken by NASA’s Cassini probe on Nov. 21, 2009. (Image credit: NASA/JPL/Space Science Institute)

Saturn's icy moon Enceladus conceals a salty ocean beneath its frozen surface, scientists now suspect.

Using NASA's Cassini spacecraft orbiting Saturn, scientists have discovered that the water geysers erupting from Enceladus contain a significant amount of salt — enough to suggest the presence of a subterranean sea.

A team of scientists led by Frank Postberg of the University of Heidelberg used Cassini's Cosmic Dust Analyzer to directly examine the plumes during three flybys by the Cassini spacecraft. Individual particles were analyzed as they hit a metal target, and the ones closer to the moon's surface were found to have a high salt content. [Photos: The Rings and Moons of Saturn]

"The salt-rich ice grains are, on average, heavier than the salt-poor ice grains," Postberg told SPACE.com in an email. "Only a relatively small fraction of the salty particles escape into the E ring." The E ring is the outermost of Saturn's seven ring groupings, and it is made up of particles ejected by Enceladus' geyser plumes.

The idea of a salty sea beneath the icy crust of Saturn's sixth largest moon has been entertained since sodium was first detected in the planet's E ring. [Video:Enceladus: Saturn's Refreshing Secret]

Cassini discovered plumes of water vapor shooting from the southern hemisphere of Enceladus in 2005. The geysers erupt from four parallel trenches known as the "tiger stripes."

While previous studies found a relatively low amount of salt in the Enceladus geyser particles that make up Saturn's outer ring, the percentage is different when studying the geysers themselves.

"The lower you get to the surface, the more salt-rich grains you see," Postberg said.

"This makes a much stronger case for liquid water," Postberg said.

Earth's oceans get their salt from the rocks that enclose them. The same is true of any other body with an ocean. On Enceladus, pressure would push bubbles of ocean spray into space, where they would quickly freeze before they could break apart. These bubbles would become samples of the ocean they escaped.

Based on the scientists' study, these reservoirs connect to a larger ocean about 50 miles (80 km) underground. Calculations limit it to the southern hemisphere, but how wide it extends is unknown.

Scientists searching for extraterrestrial life have long considered liquid water a primary requirement for its existence, so an ocean under Enceladus' surface provides another potential target.

Postberg pointed out that, unlike other unseen oceans in the solar system, the water on Enceladus is fairly easy to reach. Jupiter's moon Europa, for instance, could have an ocean under a layer of ice, but retrieving it would require significant effort. By contrast, the geysers on Enceladus pull material — and potentially life, should it exist there — from its ocean and shoot it into space.

"The water samples are thrown in front of your spacecraft by the plumes," he said. "You don't have to drill deep to analyze ocean material."

"The fact that water is on such a remote and unlikely place surely has implications for the general likelihood of life in the universe," Postberg said.

Nola Taylor Tillman
Contributing Writer

Nola Taylor Tillman is a contributing writer for Space.com. She loves all things space and astronomy-related, and always wants to learn more. She has a Bachelor's degree in English and Astrophysics from Agnes Scott College and served as an intern at Sky & Telescope magazine. She loves to speak to groups on astronomy-related subjects. She lives with her husband in Atlanta, Georgia. Follow her on Bluesky at @astrowriter.social.bluesky