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

Hubble: Possible Water Plumes on Jupiter's Moon Europa

Jet Propulsion Laboratory https://www.jpl.nasa.gov/ Sept. 26, 2016
This composite image shows suspected plumes of water vapor erupting at the 7 o'clock position off the limb of Jupiter's moon Europa. The plumes, photographed by NASA's Hubble's Space Telescope Imaging Spectrograph, were seen in silhouette as the moon passed in front of Jupiter. Credits: NASA/ESA/W. Sparks (STScI)/USGS Astrogeology Science Center

Astronomers using NASA's Hubble Space Telescope have imaged what may be water vapor plumes erupting off the surface of Jupiter's moon Europa.

Astronomers using NASA's Hubble Space Telescope have imaged what may be water vapor plumes erupting off the surface of Jupiter's moon Europa. This finding bolsters other Hubble observations suggesting the icy moon erupts with high altitude water vapor plumes.

The observation increases the possibility that missions to Europa may be able to sample Europa's ocean without having to drill through miles of ice.

"Europa's ocean is considered to be one of the most promising places that could potentially harbor life in the solar system," said Geoff Yoder, acting associate administrator for NASA's Science Mission Directorate in Washington. "These plumes, if they do indeed exist, may provide another way to sample Europa's subsurface."

The plumes are estimated to rise about 125 miles (200 kilometers) before, presumably, raining material back down onto Europa's surface. Europa has a huge global ocean containing twice as much water as Earth's oceans, but it is protected by a layer of extremely cold and hard ice of unknown thickness. The plumes provide a tantalizing opportunity to gather samples originating from under the surface without having to land or drill through the ice.

The team, led by William Sparks of the Space Telescope Science Institute in Baltimore observed these finger-like projections while viewing Europa's limb as the moon passed in front of Jupiter.

The original goal of the team's observing proposal was to determine whether Europa has a thin, extended atmosphere, or exosphere. Using the same observing method that detects atmospheres around planets orbiting other stars, the team realized if there was water vapor venting from Europa's surface, this observation would be an excellent way to see it.

"The atmosphere of an extrasolar planet blocks some of the starlight that is behind it," Sparks explained. "If there is a thin atmosphere around Europa, it has the potential to block some of the light of Jupiter, and we could see it as a silhouette. And so we were looking for absorption features around the limb of Europa as it transited the smooth face of Jupiter."

In 10 separate occurrences spanning 15 months, the team observed Europa passing in front of Jupiter. They saw what could be plumes erupting on three of these occasions.

This work provides supporting evidence for water plumes on Europa. In 2012, a team led by Lorenz Roth of Southwest Research Institute in San Antonio detected evidence of water vapor erupting from the frigid south polar region of Europa and reaching more than100 miles (160 kilometers) into space. Although both teams used Hubble's Space Telescope Imaging Spectrograph instrument, each used a totally independent method to arrive at the same conclusion.

"When we calculate in a completely different way the amount of material that would be needed to create these absorption features, it's pretty similar to what Roth and his team found," Sparks said. "The estimates for the mass are similar, the estimates for the height of the plumes are similar. The latitude of two of the plume candidates we see corresponds to their earlier work."

But as of yet, the two teams have not simultaneously detected the plumes using their independent techniques. Observations thus far have suggested the plumes could be highly variable, meaning that they may sporadically erupt for some time and then die down. For example, observations by Roth's team within a week of one of the detections by Sparks' team failed to detect any plumes.

If confirmed, Europa would be the second moon in the solar system known to have water vapor plumes. In 2005, NASA's Cassini orbiter detected jets of water vapor and dust spewing off the surface of Saturn's moon Enceladus.

Scientists may use the infrared vision of NASA's James Webb Space Telescope, which is scheduled to launch in 2018, to confirm venting or plume activity on Europa. NASA also is formulating a mission to Europa with a payload that could confirm the presence of plumes and study them from close range during multiple flybys.

"Hubble's unique capabilities enabled it to capture these plumes, once again demonstrating Hubble's ability to make observations it was never designed to make," said Paul Hertz, director of the Astrophysics Division at NASA Headquarters in Washington. "This observation opens up a world of possibilities, and we look forward to future missions -- such as the James Webb Space Telescope -- to follow-up on this exciting discovery."

The work by Sparks and his colleagues is published in the Sept. 29 issue of the Astrophysical Journal.

Planetary scientist Kevin Hand of NASA's Jet Propulsion Laboratory, Pasadena, California, co-authored the new paper.

The Hubble Space Telescope is a project of international cooperation between NASA and ESA (the European Space Agency.) NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute, which is operated for NASA by the Association of Universities for Research in Astronomy in Washington, conducts Hubble science operations.

For images and more information about Europa and Hubble, visit:

http://www.nasa.gov/hubble

http://hubblesite.org/news/2016/33

Media Contacts

Preston Dyches

818-354-7013

preston.dyches@jpl.nasa.gov

Sean Potter / Laurie Cantillo

202-358-1536 / 202-358-1077

sean.potter@nasa.gov / laura.l.cantillo@nasa.gov

Ann Jenkins / Ray Villard

410-338-4488 / 410-338-4514

jenkins@stsci.edu / villard@stsci.edu

2016-246

Related News

Mars.

NASA’s Perseverance Rover Watches Earth Vanish Behind Martian Moon

Solar System.

NASA Engineers Help Prolong Voyager 2’s Science Mission

Solar System.

NASA’s Juno Takes Temperature of Jupiter’s Fiery Moon Io

Solar System.

NASA’s Psyche Mission Delivers Mars Flyby Data, Time-lapse Video

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

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
Explore JPL
Visit
Public Tours
Virtual Tour
Directions and Maps
Explore JPL
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: v3.2.0 - 54b6266
Site Managers:Emilee Richardson, Alicia Cermak
Site Editors:Steve Carney
CL#:21-0018