Hubble Spots Possible Venting Activity On Europa

These composite images show a suspected plume of material erupting two years apart from the same location on Jupiter’s icy moon Europa. The images bolster evidence that the plumes are a real phenomenon, flaring up intermittently in the same region on the satellite. Both plumes, photographed in ultraviolet light by NASA’s Hubble’s Space Telescope Imaging Spectrograph, were seen in silhouette as the moon passed in front of Jupiter. Image Credit: NASA, ESA, W. Sparks (STScI), and the USGS Astrogeology Science Center

April 13, 2017 – Recent observations of Jupiter’s icy moon Europa by NASA’s Hubble Space Telescope have uncovered a probable plume of material erupting from the moon’s surface at precisely the same location as a similar apparent plume seen two years earlier by Hubble. These images bolster evidence that the plumes are a real phenomenon, flaring up intermittently in the same region on the satellite.

In the most recent observation — February 22, 2016 — Hubble’s Space Telescope Imaging Spectrograph (STIS) uncovered a dark patch, silhouetted against Jupiter and protruding slightly off the surface at Europa’s equatorial region. The dark feature is not only in the same location but is also similar in appearance to the one seen in a previous STIS study of Europa, taken March 17, 2014.

For both the 2016 and 2014 observations, Sparks and his team used the same transit technique to uncover the plumes in ultraviolet light. As Europa passes in front of Jupiter, any atmospheric features around the edge of the moon block some of Jupiter’s light, allowing STIS to see those features in silhouette.

The plumes correspond to the location of an unusually warm spot on the moon’s icy crust, seen in the late 1990s by NASA’s Galileo spacecraft. Researchers speculate that this might be circumstantial evidence for water erupting from the moon’s subsurface. Such a “location of interest” may be a site where material dredged up from beneath Europa’s surface could be analyzed for habitability by a future visiting spacecraft.

“If there is a causal link between the plumes and the thermal anomaly, there could be geologic activity on Europa’s surface that is producing the plumes, or the plume activity may be influencing the surface thermal properties,” said lead researcher William Sparks of the Space Telescope Science Institute (STScI) in Baltimore, Maryland.

Added team member Britney Schmidt of the Georgia Institute of Technology in Atlanta: “This latest observation adds to the growing evidence that Europa’s complex geology belies an active, maybe habitable, ice shell and ocean. Understanding Europa’s plumbing through studies like this gives us a chance to better understand that picture.”

The newly imaged plume rises about 62 miles above Europa’s surface. The plume observed by Hubble in 2014 in the same location was estimated to be about 30 miles high.

Sparks’ team matched the plumes’ position with their corresponding location on the thermal map taken of the moon’s night side by Galileo. The absence of sunlight at night allows Europa’s surface to cool down. But the researchers spotted a region that was warmer than the surrounding area. This region, roughly 200 miles across, is in the same location as the observed plumes. The area was previously identified as a “thermal anomaly,” because it was a few degrees warmer than the surrounding terrain. Such an apparently minor temperature variation is significant, considering that Europa’s icy surface is so cold.

One possibility for the temperature variation is that an infusion of energy warmed up the frigid surface. Another idea is that the surface retains an abnormal amount of heat. Both possibilities suggest that unusual activity is taking place.

“After Hubble imaged the second plume-like feature, we looked at its corresponding location on the thermal map, because studies of the plumes on Saturn’s moon Enceladus have shown that they are associated with hotter regions,” Sparks explained. “We discovered that Europa’s plume candidate is sitting right on the thermal anomaly.”

The plumes and the warm spot could be generated by a variety of geological activity. The team has proposed two possible scenarios for a link between the two features.

The warmer area could be caused by the heat from liquid water, located more than one mile beneath Europa’s thick, icy crust. The water is pushed upward and cracks the surface, venting as a plume.

Another idea is that water ejected by the plume falls onto the surface as a fine mist. This process could change the structure of the surface grains, allowing them to retain heat longer than the surrounding landscape.

Sparks and his team are continuing to use Hubble to search for additional examples of plume candidates on Europa, hoping to determine the frequency with which they appear.

The results will appear on April 13, 2017, in The Astrophysical Journal Letters.

The Space Telescope Imaging Spectrograph (STIS) is one of several instruments built for Hubble Space Telescope by Ball Aerospace in Boulder, Colorado.

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