image: This image of the Cornelia Crater on Vesta shows lobate deposits (right) and curvilinear gullies (highlighted by the short white arrows, left). According to a newly published paper in The Planetary Science Journal, ice underneath the surface of an airless world could be excavated and melted by an impact, such as from a meteoroid impact, and then flow along the walls of the impact crater as liquid brines to form these distinct surface features.
Credit: Jet Propulsion Laboratory
SAN ANTONIO — October 21, 2024—A Southwest Research Institute researcher collaborated with a team at NASA’s Jet Propulsion Laboratory to attempt to explain the presence of mysterious flow features that exist on the surfaces of airless celestial bodies, such as the asteroids Vesta and Ceres, explored recently by the NASA Dawn mission, or Jupiter’s moon Europa, which will soon be explored in detail by the NASA Europa Clipper mission that includes SwRI’s involvement.
In a new paper published in The Planetary Science Journal, its lead author, SwRI’s Dr. Michael J. Poston, and a team of researchers outline how post-impact conditions, such as from a meteoroid impact, could produce liquid brines that temporarily flow along the surface long enough to etch curved gullies and deposit fans of debris in the walls of newly formed craters.
“We wanted to investigate our previously proposed idea that ice underneath the surface of an airless world could be excavated and melted by an impact and then flow along the walls of the impact crater to form distinct surface features,” said project PI Dr. Jennifer Scully (JPL).
The team wanted to understand how long the liquid could potentially flow before refreezing, as most liquids lose stability in strong vacuum conditions.
The paper, “Experimental Examination of Brine and Water Lifetimes after Impact on Airless Worlds,” details the team’s findings after simulating the pressures that ice on Vesta, one of the largest asteroids in our solar system, experiences after a meteoroid impact and how long it takes the liquid released from the subsurface to refreeze.
The team modified a test chamber at the Jet Propulsion Laboratory to rapidly decrease pressure over a liquid sample to simulate the dramatic drop in pressure as the temporary atmosphere created after an impact on an airless body like Vesta dissipates. According to Poston, the pressure drop was so fast that test liquids immediately and dramatically expanded, ejecting material from the sample containers.
“Through our simulated impacts, we found that the pure water froze too quickly in a vacuum to effect meaningful change, but salt and water mixtures, or brines, stayed liquid and flowing for a minimum of one hour,” said Poston. “This is sufficient for the brine to destabilize slopes on crater walls on rocky bodies, cause erosion and landslides, and potentially form other unique geological features found on icy moons.”
These findings could also help to explain the origins of certain observed features on distant bodies, such as the smooth plains of Europa and the distinct “spider” feature in its Manannán crater, or the various gullies and fan-shaped debris deposits on Mars. The study could also help build a stronger case for the existence of subsurface water in seemingly inhospitable locations in the solar system.
“If the findings are consistent across these dry and airless or thin-atmosphere bodies, it demonstrates that water existed on these worlds in the recent past, indicating water might still be expelled from impacts,” said Poston. “There may still be water out there to be found.”
The study was funded through a grant from NASA’s Discovery Data Analysis Program as part of an ongoing project led by the Jet Propulsion Laboratory at the California Institute of Technology, Pasadena.
For more information, visit https://www.swri.org/technical-divisions/space-science.