University of Maryland astronomers released this news on June 7, 2025. Edits by EarthSky.<\/p>\n
When NASA\u2019s DART spacecraft slammed into the asteroid moon Dimorphos in September 2022 \u2013 with the aim of testing whether we could deflect an asteroid \u2013 the craft didn\u2019t just change the asteroid\u2019s orbit as intended. It also unleashed a massive barrage of boulders that carried more than three times the momentum of the spacecraft itself. <\/p>\n
A University of Maryland-led team of astronomers found that, while the mission successfully proved that kinetic impactors like the DART spacecraft can alter an asteroid\u2019s path, the resulting ejected boulders created forces in unexpected directions that could complicate future deflection efforts. According to the team\u2019s new paper published in the Planetary Science Journal<\/em> on July 4, 2025, using asteroid deflection for planetary defense is likely far more complex than researchers initially understood. Tony Farnham, lead author of the paper and a research scientist at UMD\u2019s Department of Astronomy, said:<\/p>\n We succeeded in deflecting an asteroid, moving it from its orbit. Our research shows that while the direct impact of the DART spacecraft caused this change, the boulders ejected gave an additional kick that was almost as big. That additional factor changes the physics we need to consider when planning these types of missions.<\/p>\n<\/blockquote>\n The team used images taken by LICIACube, a small Italian spacecraft that followed along with DART in space and observed its aftermath. They tracked 104 boulders ranging from 0.2 to 3.6 meters (.7 to 12 feet) in radius as they shot away from Dimorphos at speeds up to 52 meters per second (116 miles per hour). From those images, the team determined 3-dimensional locations and velocities of the ejected rocks. Farnham said:<\/p>\n We saw that the boulders weren\u2019t scattered randomly in space. Instead, they were clustered in two pretty distinct groups, with an absence of material elsewhere, which means that something unknown is at work here.<\/p>\n<\/blockquote>\n The largest debris cluster, containing about 70% of the measured objects, was ejected toward the south at high velocities and shallow angles to the surface. The team believes that the ejected boulders likely came from specific sources, perhaps from larger boulders on Dimorphos that were shattered by DART\u2019s solar panels just before the main body of the spacecraft hit the surface. Jessica Sunshine, a professor of astronomy and geology at UMD, and the paper\u2019s 2nd author, said:<\/p>\n DART\u2019s solar panels likely hit two big boulders, called Atabaque and Bodhran, on the asteroid. Evidence suggests that the southern cluster of ejected material is probably made up of fragments from Atabaque, a 3.3-meter-radius (11-foot-radius) boulder.<\/p>\n<\/blockquote>\n Sunshine also served as deputy principal investigator for the UMD-led NASA Deep Impact mission, which involved intentionally crashing a spacecraft into comet Tempel 1 to study its interior composition. She said compared DART\u2019s results with Deep Impact\u2019s, noting how surface features and target composition fundamentally shape impact outcomes. She explained:<\/p>\n Deep Impact hit a surface that was essentially very small, uniform particles, so its ejecta was relatively smooth and continuous.<\/p>\n And here, we see that DART hit a surface that was rocky and full of large boulders, resulting in chaotic and filamentary structures in its ejecta patterns. Comparing these two missions side-by-side gives us this insight into how different types of celestial bodies respond to impacts, which is crucial to ensuring that a planetary defense mission is successful. <\/p>\n<\/blockquote>\n The momentum from the DART impact\u2019s ejected boulders was primarily perpendicular to the spacecraft\u2019s trajectory, meaning that it could have tilted Dimorphos\u2019 orbital plane by up to 1 degree and potentially sent the asteroid tumbling erratically in space. <\/p>\n The team\u2019s work on understanding the effect of the boulder debris will be key to the European Space Agency\u2019s Hera mission, which will arrive at the Didymos-Dimorphos system in 2026. Farnham said:<\/p>\n Data gathered from LICIACube provides additional perspectives on impact events, especially as DART was originally designed to solely rely on Earth-based observations. Hera will do the same by giving us another direct view of the impact\u2019s aftermath, relying on the predictions we\u2019ve made using data gathered from DART.<\/p>\n<\/blockquote>\n Farnham noted that these multiple perspectives and closeup images from LICIACube gave the DART team information that would have been impossible to detect from Earth, including data on the asteroid boulders. This new study suggests the importance of considering those variables in planning future asteroid deflection missions. Sunshine added:<\/p>\n If an asteroid was tumbling toward us, and we knew we had to move it a specific amount to prevent it from hitting Earth, then all these subtleties become very, very important. You can think of it as a cosmic pool game. We might miss the pocket if we don\u2019t consider all the variables.<\/p>\n<\/blockquote>\n Bottom line: Space rocks ejected during NASA\u2019s DART mission \u2013 to test whether we could deflect an asteroid from its path \u2013 carried three times more momentum than the spacecraft itself.<\/p>\n Source: High-speed Boulders and the Debris Field in DART Ejecta <\/p>\n Via University of Maryland<\/p>\n <\/div>\n\n
![\"Two](\"https:\/\/earthsky.org\/upl\/2025\/07\/DART-mission-ejecta-composite-e1752061969770.png\")
Not scattered randomly<\/h3>\n
\n
\n
Dart mission vs. Deep Impact<\/h3>\n
\n
\n
\n