JPL
Careers
Education
Science & Technology
JPL Logo
JPL Logo
Solar System
.4 min read

Cassini Finds an Active, Watery World at Saturn's Enceladus

Jet Propulsion Laboratory https://www.jpl.nasa.gov/ July 29, 2005
Map showing observed temperatures at Enceladus.+ Comparison of predicted and observed temperatures at Enceladus

Saturn's tiny icy moon Enceladus, which ought to be cold and dead, instead displays evidence for active ice volcanism.

Saturn's tiny icy moon Enceladus, which ought to be cold and dead, instead displays evidence for active ice volcanism.

NASA's Cassini spacecraft has found a huge cloud of water vapor over the moon's south pole, and warm fractures where evaporating ice probably supplies the vapor cloud. Cassini has also confirmed Enceladus is the major source of Saturn's largest ring, the E-ring.

"Enceladus is the smallest body so far found that seems to have active volcanism," said Dr. Torrence Johnson, Cassini imaging-team member at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "Enceladus' localized water vapor atmosphere is reminiscent of comets. 'Warm spots' in its icy and cracked surface are probably the result of heat from tidal energy like the volcanoes on Jupiter's moon Io. And its geologically young surface of water ice, softened by heat from below, resembles areas on Jupiter's moons, Europa and Ganymede."

Cassini flew within 175 kilometers (109 miles) of Enceladus on July 14. Data collected during that flyby confirm an extended and dynamic atmosphere. This atmosphere was first detected by the magnetometer during a distant flyby earlier this year.

The ion and neutral mass spectrometer and the ultraviolet imaging spectrograph found the atmosphere contains water vapor. The mass spectrometer found the water vapor comprises about 65 percent of the atmosphere, with molecular hydrogen at about 20 percent. The rest is mostly carbon dioxide and some combination of molecular nitrogen and carbon monoxide. The variation of water vapor density with altitude suggests the water vapor may come from a localized source comparable to a geothermal hot spot. The ultraviolet results strongly suggest a local vapor cloud.

The fact that the atmosphere persists on this low-gravity world, instead of instantly escaping into space, suggests the moon is geologically active enough to replenish the water vapor at a slow, continuous rate.

"For the first time we have a major clue not only to the role of water at the icy moons themselves, but also to its role in the evolution and dynamics of the Saturn system as a whole," said Dr. Ralph L. McNutt, ion and neutral mass spectrometer-team member, Johns Hopkins University Applied Physics Laboratory, Laurel, Md.

Images show the south pole has an even younger and more fractured appearance than the rest of Enceladus, complete with icy boulders the size of large houses and long, bluish cracks or faults dubbed "tiger stripes."

Another Cassini instrument, the composite infrared spectrometer, shows the south pole is warmer than anticipated. Temperatures near the equator were found to reach a frigid 80 degrees Kelvin (minus 316 Fahrenheit), as expected. The poles should be even colder because the Sun shines so obliquely there. However, south polar average temperatures reached 85 Kelvin (minus 307 Fahrenheit), much warmer than expected. Small areas of the pole, concentrated near the "tiger stripe" fractures, are even warmer: well over 110 Kelvin (minus 261 Fahrenheit) in some places.

"This is as astonishing as if we'd flown past Earth and found that Antarctica was warmer than the Sahara," said Dr. John Spencer, team member of the composite infrared spectrometer, Southwest Research Institute, Boulder, Colo.

Scientists find the temperatures difficult to explain if sunlight is the only heat source. More likely, a portion of the polar region, including the "tiger stripe" fractures, is warmed by heat escaping from the interior. Evaporation of this warm ice at several locations within the region could explain the density of the water vapor cloud detected by other instruments. How a 500-kilometer (310-mile) diameter moon can generate this much internal heat and why it is concentrated at the south pole is still a mystery.

Cassini's cosmic dust analyzer detected a large increase in the number of particles near Enceladus. This observation confirms Enceladus is a source of Saturn's E-ring. Scientists think micrometeoroids blast the particles off, forming a steady, icy, dust cloud around Enceladus. Other particles escape, forming the bulk of the E ring.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL.

Additional information and graphics on these results are available at: http://www.nasa.gov/cassini and hhttp://saturn.jpl.nasa.gov .

  • + Cassini news and images
  • + Cassini home page

Media Contacts

Carolina Martinez

(212) 460-4111

Erica Hupp/Dolores Beasley

(202) 358-1237/1753

2005-124

Related News

Solar System.

NASA Testing Advanced Capabilities for Moon, Mars Rovers

Solar System.

NASA’s Psyche Mission Aces Mars Flyby, Targets Metal-Rich Asteroid

Mars.

NASA’s Perseverance Rover Snaps Selfie in Mars’ Western Frontier

Mars.

NASA’s Perseverance, Curiosity Panoramas Capture Two Sides of Mars

Mars.

NASA’s Curiosity Finds Organic Molecules Never Seen Before on Mars

Solar System.

NASA Shuts Off Instrument on Voyager 1 to Keep Spacecraft Operating

Asteroids and Comets.

NASA’s DART Mission Changed Orbit of Asteroid Didymos Around Sun

Mars.

NASA’s Curiosity Rover Sees Martian ‘Spiderwebs’ Up Close

Mars.

NASA’s Perseverance Now Autonomously Pinpoints Its Location on Mars

Mars.

NASA’s Perseverance Rover Completes First AI-Planned Drive on Mars

About JPL
Who We Are
Directors
Careers
Internships
The JPL Story
JPL Achievements
Documentary Series
JPL Annual Report
Executive Council
Missions
Current
Past
Future
All
News
All
Earth
Solar System
Stars and Galaxies
Eyes on the News
Subscribe to JPL News
Galleries
Images
Videos
Audio
Podcasts
Apps
Visions of the Future
Slice of History
Robotics at JPL
Events
Lecture Series
Speakers Bureau
Calendar
Visit
Public Tours
Virtual Tour
Directions and Maps
Topics
JPL Life
Solar System
Mars
Earth
Climate Change
Exoplanets
Stars and Galaxies
Robotics
More
Asteroid Watch
NASA's Eyes Visualizations
Universe - Internal Newsletter
Social Media
Accessibility at NASA
Contact Us
Get the Latest from JPL
Follow Us

JPL is a federally funded research and development center managed for NASA by Caltech.

More from JPL
Careers
Education
Science & Technology
Acquisition
JPL Store
Careers
Education
Science & Technology
Acquisition
JPL Store
Related NASA Sites
Basics of Spaceflight
NASA Kids Science - Earth
Earth / Global Climate Change
Exoplanet Exploration
Mars Exploration
Solar System Exploration
Space Place
NASA's Eyes Visualization Project
Voyager Interstellar Mission
NASA
Caltech
Privacy
Image Policy
FAQ
Feedback
Version: v3.1.3 - 5e83a9a
Site Managers:Emilee Richardson, Alicia Cermak
Site Editors:Naomi Hartono, Steve Carney
CL#:21-0018