12 May 2015
WASHINGTON, D.C. – New laboratory experiments suggest the dark material coating some geological features of Jupiter’s moon Europa is likely sea salt from a subsurface ocean, discolored by exposure to radiation. The presence of sea salt on Europa’s surface suggests the ocean is interacting with its rocky seafloor — an important consideration in determining whether the icy moon could support life.
The new study has been accepted for publication in Geophysical Research Letters, a journal of the American Geophysical Union, and is available online.
“We have many questions about Europa, the most important and most difficult to answer being is there life? Research like this is important because it focuses on questions we can definitively answer, like whether or not Europa is inhabitable,” said Curt Niebur, Outer Planets Program scientist at NASA Headquarters in Washington. “Once we have those answers, we can tackle the bigger question about life in the ocean beneath Europa’s ice shell.”
For more than a decade, scientists have wondered about the nature of the dark material that coats long, linear fractures, and other relatively young geological features on Europa’s surface. Its association with young terrains suggests the material has erupted from within Europa, but with limited data available, the material’s chemical composition has remained elusive.
“If it’s just salt from the ocean below, that would be a simple and elegant solution for what the dark, mysterious material is,” said research lead Kevin Hand, a planetary scientist at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California.
One certainty is that Europa is bathed in radiation created by Jupiter’s powerful magnetic field. Electrons and ions slam into the moon’s surface with the intensity of a particle accelerator. Theories proposed to explain the nature of the dark material include this radiation as a likely part of the process that creates it.
Previous studies using data from NASA’s Galileo spacecraft, and various telescopes, attributed the discolorations on Europa’s surface to compounds containing sulfur and magnesium. While radiation-processed sulfur accounts for some of the colors on Europa, the new experiments reveal that irradiated salts could explain the color within the youngest regions of the moon’s surface.
To identify the dark material, Hand and his co-author Robert Carlson, also at JPL, created a simulated patch of Europa’s surface in a laboratory test apparatus for testing possible candidate substances. For each material, they collected spectra — which are like chemical fingerprints — encoded in the light reflected by the compounds.
“We call it our ‘Europa in a can,'” Hand said. “The lab setup mimics conditions on Europa’s surface in terms of temperature, pressure and radiation exposure. The spectra of these materials can then be compared to those collected by spacecraft and telescopes.”
For this particular research, the scientists tested samples of common salt — sodium chloride — along with mixtures of salt and water, in their vacuum chamber at Europa’s chilly surface temperature of minus 173 Celsius (minus 280 degrees Fahrenheit). They then bombarded the salty samples with an electron beam to simulate the intense radiation on the moon’s surface.
After a few tens of hours of exposure to this harsh environment, which corresponds to as long as a century on Europa, the salt samples, which were initially white just like table salt, turned a yellowish-brown color similar to features on the icy moon. The researchers found the color of these samples, as measured in their spectra, showed a strong resemblance to the color within fractures on Europa that were imaged by NASA’s Galileo mission.
“This work tells us the chemical signature of radiation-baked sodium chloride is a compelling match to spacecraft data for Europa’s mystery material,” Hand said.
Additionally, the longer the samples were exposed to radiation, the darker the resulting color. Hand thinks scientists could use this type of color variation to help determine the ages of geologic features and material ejected from any plumes that might exist on Europa.
Previous telescope observations have shown tantalizing hints of the spectral features seen by the researchers in their irradiated salts. But no telescope on or near Earth can observe Europa with sufficiently high resolving power to identify them with certainty. The researchers suggest this could be accomplished by future observations with a spacecraft visiting Europa.
JPL built and managed NASA’s Galileo mission for the agency’s Science Mission Directorate in Washington, and is developing a concept for a future mission to Europa. The California Institute of Technology in Pasadena, manages JPL for NASA.
For more information about Europa, visit: http://europa.jpl.nasa.gov
The American Geophysical Union is dedicated to advancing the Earth and space sciences for the benefit of humanity through its scholarly publications, conferences, and outreach programs. AGU is a not-for-profit, professional, scientific organization representing more than 60,000 members in 139 countries. Join the conversation onFacebook, Twitter, YouTube, and our other social media channels.
Notes for Journalists
Journalists and public information officers (PIOs) of educational and scientific institutions who have registered with AGU can download a PDF copy of the article by clicking on this link: http://onlinelibrary.wiley.com/doi/10.1002/2015GL063559/full?campaign=wlytk-41855.5282060185
Or, you may order a copy of the final paper by emailing your request to Nanci Bompey at [email protected]. Please provide your name, the name of your publication, and your phone number.
Neither the papers nor this press release is under embargo.
“Europa's surface color suggests an ocean rich with sodium chloride”
K. P. Hand and R. W. Carlson: Jet Propulsion Laboratory California Institute of Technology, Pasadena, CA, USA.
Contact Information for the Authors:
Kevin Hand: +1 (626) 487-5379, [email protected]
+1 (202) 777-7524
NASA Headquarters Contact:
+1 (202) 358-1726
NASA Jet Propulsion Laboratory Contact:
+1 (818) 354-7013