Scientists have theorized on the origin of the water plumes possibly erupting from Jupiter’s moon Europa. Recent research adds a new potential source to the mix.
Plumes of water vapor that may be venting into space from Jupiter’s moon Europa could come from within the icy crust itself, according to new research. A model outlines a process for brine, or salt-enriched water, moving around within the moon’s shell and eventually forming pockets of water — even more concentrated with salt — that could erupt.
Europa scientists have considered the possible plumes on Europa a promising way to investigate the habitability of Jupiter’s icy moon, especially since they offer the opportunity to be directly sampled by spacecraft flying through them. The insights into the activity and composition of the ice shell covering Europa’s global, interior ocean can help determine if the ocean contains the ingredients needed to support life.
This new work that offers an additional scenario for some plumes proposes that they may originate from pockets of water embedded in the icy shell rather than water forced upward from the ocean below. The source of the plumes is important: Water originating from the icy crust is considered less hospitable to life than the global interior ocean because it likely lacks the energy that is a necessary ingredient for life. In Europa’s ocean, that energy could come from hydrothermal vents on the sea floor.
“Understanding where these water plumes are coming from is very important for knowing whether future Europa explorers could have a chance to actually detect life from space without probing Europa’s ocean,” said lead author Gregor Steinbrügge, a postdoctoral researcher at Stanford’s School of Earth, Energy & Environmental Sciences.
Using images collected by NASA’s Galileo spacecraft, the researchers developed a model to propose how a combination of freezing and pressurization could lead to a cryovolcanic eruption, or a burst of frigid water. The results, published November 10 in Geophysical Research Letters, may shed light on eruptions on other icy bodies in the solar system.
The researchers focused their analyses on Manannán, an 18-mile-wide (29-kilometer-wide) crater on Europa that resulted from an impact with another celestial object tens of millions of years ago. Reasoning that such a collision would have generated tremendous heat, they modeled how the melted ice and subsequent freezing of the water pocket within the icy shell could have pressurized it and caused the water to erupt.
“The comet or asteroid hitting the ice shell was basically a big experiment which we’re using to construct hypotheses to test,” said co-author Don Blankenship, senior research scientist at the University of Texas Institute for Geophysics (UTIG) and principal investigator of the radar instrument, REASON (Radar for Europa Assessment and Sounding: Ocean to Near-surface), that will fly aboard NASA’s upcoming Europa Clipper spacecraft. “Our model makes specific predictions we can test using data from the radar and other instruments on Europa Clipper.”
The model indicates that as Europa’s water partially froze into ice following the impact, leftover pockets of water could have been created in the moon’s surface. These salty water pockets can move sideways through Europa’s ice shell by melting adjacent regions of ice and consequently become even saltier in the process.
A Salty Driving Force
The model proposes that when a migrating brine pocket reached the center of Manannán Crater, it became stuck and began freezing, generating pressure that eventually resulted in a plume, estimated to have been over a mile high (1.6 kilometers). The eruption of this plume left a distinguishing mark: a spider-shaped feature on Europa’s surface that was observed by Galileo imaging and incorporated into the researchers’ model.
“Even though plumes generated by brine pocket migration would not provide direct insight into Europa’s ocean, our findings suggest that Europa’s ice shell itself is very dynamic,” said co-lead author Joana Voigt, a graduate research assistant at the University of Arizona, in Tucson.
The relatively small size of the plume that would form at Manannán indicates that impact craters probably can’t explain the source of other, larger plumes on Europa that have been hypothesized based on data from Galileo and NASA’s Hubble Space Telescope, researchers said. But the process modeled for the Manannán eruption could happen on other icy bodies — even without an impact event.
“The work is exciting, because it supports the growing body of research showing there could be multiple kinds of plumes on Europa,” said Robert Pappalardo of NASA’s Jet Propulsion Laboratory in Southern California and project scientist of the Europa Clipper mission. “Understanding plumes and their possible sources strongly contributes to Europa Clipper’s goal to investigate Europa’s habitability.”
Missions such as Europa Clipper help contribute to the field of astrobiology, the interdisciplinary research on the variables and conditions of distant worlds that could harbor life as we know it. While Europa Clipper is not a life-detection mission, it will conduct detailed reconnaissance of Europa and investigate whether the icy moon, with its subsurface ocean, has the capability to support life. Understanding Europa’s habitability will help scientists better understand how life developed on Earth and the potential for finding life beyond our planet.
Read Harbinger of Extraterrestrial Life? Explaining Cryovolcanic Eruptions on Jupiter’s Moon Europa for more on this research.
Reference: “Brine Migration and Impact‐Induced Cryovolcanism on Europa” by G. Steinbrügge, J. R. C. Voigt, N. S. Wolfenbarger, C. W. Hamilton, K. M. Soderlund, D. A. Young, D. D. Blankenship, S. D. Vance and D. M. Schroeder, 5 November 2020, Geophysical Research Letters.