Laurel Kornfeld

February 21st, 2017

A dramatic plume sprays water ice and vapor from the south polar region of Saturns moon Enceladus. Cassinis first hint of this plume came during the spacecrafts first close flyby of the icy moon on February 17, 2005. Image & Caption Credit: NASA/JPL/Space Science Institute

An unexpected finding by NASAs Cassini spacecraftduring itsfirst flyby of Saturns moon Enceladushas led to the discovery of its subsurface ocean, which could, possibly, host microbial life.

After arriving at Saturn in 2004, Cassini made its first pass by Saturns sixth largest moon on February 17, 2005. The flyby was part of the spacecrafts detailed study of the planets icy moons.

Illustration showing the bending of Saturns magnetic field near Enceladus that was detected by Cassinis magnetometer. (Click to enlarge) Image & Caption Credit: NASA/JPL-Caltech

As Cassini flew by Enceladus, the spacecrafts magnetometer, which measures the magnetic field in the area, detected an anomaly, suggesting that the 157-mile (252-kilometer) moon had a thin atmosphere.

Orbiting in the middle of Saturns faint E ring, Enceladus is the Solar Systems most reflective object, but scientists attributed this brightness to the emission of ice dust from its surface and believed the small moon to be an inactive world.

However, inexplicably, Saturns magnetic field was being perturbed above Enceladuss south pole.

Because of the unusual findings, Cassini flew even closer to the small moon just several weeks later, on March 9, 2005, to obtain a better look.

According to Cassini Magnetometer Principal Investigator Michelle Dougherty, [] the atmospheric signature that we were seeing was focused at the south pole. It was almost like there was a cometary plume of water vapor coming off from the south pole.

The fact that Enceladus resembled a comet actively emitting gases led scientists to speculate its atmosphere is somehow replenishing these gases.

Some scientists excitedly speculated the south polar plume came from jets, but members of Cassinis imaging team were skeptical and wanted to make another pass at the small moon before confirming anything.

That led to a third flyby on July 14, 2005, this time coming within just 175 kilometers of Enceladuss surface, which put an end to the skepticism.

Tiger Stripes on Enceladus. Image Credit: Cassini Imaging Team / SSI / JPL / ESA / NASA

From that vantage point, the mission team was able to see geysers of water vapor and water ice particles streaming out of Enceladus south pole.

Cassinis science instruments studied the region, imaging the now-famous cracks and tiger stripes, along with heat being emitted from the stripes.

These discoveries dramatically altered mission plans. Enceladus was so exciting that, instead of just three close flybys planned for our four-year primary mission, we added 20 more, including seven that went right through the geysers at the south pole, noted Cassini project scientist Linda Spilker.

Subsequent flybys confirmed that the plumes are emitting organic material in addition to dust, water vapor, volatile gases, salts, and silica.

The surprising magnetometer reading led us to the liquid water ocean underneath Enceladus icy crust, Spilker emphasized.

From Cassinis extensive study of this small world, scientists know that an underground ocean is present and suspect Enceladuss interior is being heated by tidal forces from Saturn, meaning it could potentially support microbial life.

That has altered the way we think about where life might be found in our own Solar System, and in the worlds beyond, she added.

Microbial life has been found in underwater hydrothermal vents on Earth and could, possibly, exist in such vents on the floor of Enceladuss global salty subsurface ocean.

Enceladus joins a growing list of ocean worlds that could potentially harbor such life, including Jupiters moon Europa, fellow Saturn moon Titan, Neptunes moon Triton, and even possibly dwarf planets Ceres and Pluto.

Video Courtesy of NASA Jet Propulsion Laboratory

Tagged: Cassini Enceladus Jet Propulsion Laboratory NASA Saturn The Range

Laurel Kornfeld is an amateur astronomer and freelance writer from Highland Park, NJ, who enjoys writing about astronomy and planetary science. She studied journalism at Douglass College, Rutgers University, and earned a Graduate Certificate of Science from Swinburne Universitys Astronomy Online program. Her writings have been published online in The Atlantic, Astronomy magazines guest blog section, the UK Space Conference, the 2009 IAU General Assembly newspaper, The Space Reporter, and newsletters of various astronomy clubs. She is a member of the Cranford, NJ-based Amateur Astronomers, Inc. Especially interested in the outer solar system, Laurel gave a brief presentation at the 2008 Great Planet Debate held at the Johns Hopkins University Applied Physics Lab in Laurel, MD.

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Cassini's first flyby of Enceladus led to discovery of its subsurface ocean - SpaceFlight Insider