New research reveals that when NASA’s
DART (Double Asteroid Redirection Test) spacecraft intentionally impacted the
asteroid moonlet Dimorphos in September 2022, it didn’t just change the motion
of Dimorphos around its larger companion, Didymos; the crash also shifted the
orbit of both asteroids around the Sun. Linked together by gravity, Didymos and
Dimorphos orbit each other around a shared center of mass in a configuration
known as a binary system, so changes to one asteroid affect the other.
As detailed in a study published on Friday in the journal Science Advances, observations of the pair’s motion revealed that the 770-day orbital period around the Sun changed by a fraction of a second after the DART spacecraft’s impact on Dimorphos. That change marks the first time a human-made object has measurably altered the path of a celestial body around the Sun.
The Hubble Space Telescope observed two tails of dust
ejected from the Didymos-Dimorphos asteroid system several days after NASA’s
DART spacecraft impacted the smaller asteroid.
NASA, ESA, Jian-Yang Li (PSI), Joe Depasquale (STScI)
“This is a tiny change to the orbit, but given enough time, even a tiny
change can grow to a significant deflection,” said Thomas Statler, lead
scientist for solar system small bodies at NASA Headquarters in Washington.
“The team’s amazingly precise measurement again validates kinetic impact as a
technique for defending Earth against asteroid hazards and shows how a binary
asteroid might be deflected by impacting just one member of the pair.”
High impact
When DART struck Dimorphos, the
impact blasted a huge cloud of rocky debris into space, altering the shape of the asteroid, which measures 560
feet (170 meters) wide. Because the debris carried its own momentum away from
the asteroid, it gave Dimorphos an explosive thrust — what scientists call the
momentum enhancement factor. More debris being kicked out means more oomph.
According to the new research, the momentum enhancement factor for DART’s
impact was about two, meaning that the debris loss doubled the punch created by
the spacecraft alone.
Earlier research showed that the
smaller asteroid’s 12-hour orbital period around the nearly half-mile-wide
(805-meter-wide) Didymos shortened by 33 minutes. The new study shows the impact ejected so much
material from the binary system that it also changed the binary’s orbital
period around the Sun by 0.15 seconds.
“The change in the binary system’s
orbital speed was about 11.7 microns per second, or 1.7 inches per hour,” said
Rahil Makadia, the study’s lead author at the University of Illinois
Urbana-Champaign. “Over time, such a small change in an asteroid’s motion can
make the difference between a hazardous object hitting or missing our planet.”
Although Didymos was not on an
impact trajectory with Earth and it was impossible for the DART mission to put
it on one, that change in orbital speed underscores the role spacecraft — aka
kinetic impactors in this context — could play if a potentially hazardous
asteroid is found to be on a collision course in the future. The key is
detecting near-Earth objects far enough in advance to send a kinetic impactor.
To that end, NASA is building
the Near-Earth
Object (NEO) Surveyor mission. Managed by NASA’s Jet Propulsion Laboratory in Southern
California, this next-generation space survey telescope is the first to be
built for planetary defense. The mission will seek out some of the
hardest-to-find near-Earth objects, such as dark asteroids and comets that
don’t reflect much visible light.
How they did it
To prove DART had a detectable
influence on both asteroids — not just on the smaller Dimorphos — the
researchers needed to measure Didymos’ orbit around the Sun to exquisite
precision. So, in addition to making radar and other ground-based observations
of the asteroid, they tracked stellar occultations, which occur when the
asteroid passes exactly in front of a star, causing the pinpoint of light to
blink out for a fraction of a second. This technique provides extremely precise
measurements of the asteroid’s speed, shape, and position.
Measuring stellar occultations is
challenging: Astronomers have to be in the right place at the right time with
several observing stations, sometimes miles apart, to track the predicted path
of the asteroid in front of a specific star. The team relied on volunteer
astronomers around the globe who recorded 22 stellar occultations between
October 2022 and March 2025.
“When combined with years of
existing ground-based observations, these stellar occultation observations
became key in helping us calculate how DART had changed Didymos’ orbit,” said
study co-lead Steve Chesley, a senior research scientist at JPL. “This work is
highly weather dependent and often requires travel to remote regions with no
guarantee of success. This result would not have been possible without the
dedication of dozens of volunteer occultation observers around the world.”
Studying changes in Didymos’ motion
also helped the researchers calculate the densities of both asteroids.
Dimorphos is slightly less dense than previously thought, supporting the theory
that it formed from rocky debris shed by a rapidly spinning Didymos. This loose
material eventually clumped together to form Dimorphos, a “rubble pile”
asteroid.
More about DART
The DART spacecraft was designed,
built, and operated by the Johns Hopkins Applied Physics Laboratory in Laurel,
Maryland, for NASA’s Planetary Defense Coordination Office, which oversees the
agency’s ongoing efforts in planetary defense. It was humanity’s first mission
to intentionally move a celestial object.
For more information about the DART mission visit: https://science.nasa.gov/mission/dart/
Source: NASA’s DART Mission Changed Orbit of Asteroid Didymos Around Sun - NASA




