NASA DART Changed Binary Asteroid's Solar Orbit in Historic First

On September 26, 2022, a refrigerator-sized spacecraft traveling at 6.6 kilometers per second slammed into a 160-meter asteroid moonlet named Dimorphos. The $324.5 million gamble — NASA's Double Asteroid Redirection Test — was designed to answer a question as old as civilization itself: can humanity defend itself against an asteroid on a collision course with Earth?

The answer, confirmed over three and a half years of painstaking observation, is more resounding than anyone anticipated. Not only did DART shorten Dimorphos's orbit around its companion asteroid Didymos by 33 minutes — far exceeding the predicted 4.2 minutes — but new research published in Science Advances in March 2026 reveals that the impact altered the entire binary system's orbit around the Sun [1]. It is the first time a human-made object has measurably changed the heliocentric path of a celestial body [2].

The Discovery That Changed Everything

The latest revelation emerged from an unlikely source: volunteer astronomers scattered across the globe. Between October 2022 and March 2025, these citizen scientists recorded 22 stellar occultations — precise moments when the Didymos system passed in front of distant stars, briefly dimming their light. Combined with ground-based radar measurements and years of pre-impact orbital data, these observations allowed a research team led by Rahil Makadia at NASA's Jet Propulsion Laboratory to calculate the heliocentric deflection with extraordinary precision [3].

The numbers are staggering in their subtlety. The Didymos system experienced an along-track velocity change of −11.7 ± 1.3 micrometers per second — roughly 42 millimeters per hour, comparable to the width of an Apple Watch [4]. The binary's orbital period around the Sun, previously about 770 days, shifted by 0.15 seconds [1].

These figures may sound trivially small. They are not.

"This is a tiny change to the orbit, but given enough time, even a tiny change can grow to a significant deflection," stated Thomas Statler, lead scientist for solar system small bodies at NASA Headquarters [1]. Over a decade, that microscopic velocity change accumulates to approximately 3.69 kilometers of positional displacement in the asteroid's solar orbit [4] — enough, with years of advance warning, to redirect a threatening asteroid past Earth entirely.

How a Moonlet Became a Watermelon

The physical consequences of DART's impact were dramatic. Dimorphos, once shaped like a "squashed ball," was hammered into a triaxial ellipsoid — something scientists have compared to an oblong watermelon [5]. Its mean orbital distance from Didymos shrank by about 37 meters, from a roughly circular orbit to an elongated one [6].

The transformation confirmed what researchers had suspected: Dimorphos is a loosely packed "rubble pile," a gravitationally bound aggregate of rocky debris rather than a solid monolith [5]. This matters enormously for planetary defense planning, because the composition and internal structure of a threatening asteroid would determine how effectively a kinetic impactor could deflect it.

Perhaps the most consequential finding was the momentum enhancement factor. DART's impact registered a factor of approximately 2.0 ± 0.3, meaning the debris ejected from Dimorphos's surface effectively doubled the punch delivered by the spacecraft alone [3]. The recoil from tons of excavated rock and dust fleeing into space pushed the asteroid system harder than the collision itself — a cosmic billiards trick that dramatically improved the deflection efficiency.

"By demonstrating that asteroid deflection missions such as DART can effect change in the heliocentric orbit of a celestial body, this study marks a notable step forward in our ability to prevent future asteroid impacts on Earth," Makadia and co-author Steven Chesley wrote in the paper [2].

The Scale of the Threat

The need for such capabilities is not theoretical. As of early 2025, astronomers have identified approximately 37,500 near-Earth objects, of which roughly 2,500 are classified as potentially hazardous asteroids (PHAs) — objects larger than 140 meters whose orbits bring them within 0.05 astronomical units of Earth's path [7]. Among those, 153 are estimated to exceed one kilometer in diameter — large enough to cause global catastrophe upon impact [7].

The reassuring news is that more than 99% of known PHAs pose no impact threat over the next century. As of February 2025, only 21 objects on the Sentry Risk Table could not be excluded as potential threats within the next hundred years [7]. But the operative word is "known." An estimated 60% of near-Earth asteroids larger than 140 meters remain undiscovered, lurking in orbital blind spots or simply too faint for current survey telescopes to detect [8].

This detection gap is precisely why NASA's planetary defense program has experienced explosive budget growth over the past 15 years.

Source: The Planetary Society

Data as of Mar 9, 2026CSV

From Millions to Hundreds of Millions: The Rise of Planetary Defense

In 2008, NASA spent just $3.3 million on planetary defense — barely enough to fund a handful of researchers tracking near-Earth objects. By 2019, that figure had ballooned to $157 million, a 40-fold increase driven largely by DART's development costs and expanding survey operations [9].

The DART mission itself cost $324.5 million: $308 million for spacecraft development, $68.8 million for launch services aboard a SpaceX Falcon 9, and $16.5 million for operations and data analysis [10]. By the standards of planetary science, this was remarkably affordable — the lowest-cost NASA planetary mission in decades, yet one that delivered what may prove to be the most consequential scientific result of the century [10].

Even with DART completed, the Planetary Defense Coordination Office continues to receive robust funding, with approximately $142.7 million per year allocated for ongoing survey work and mission planning [9]. The investment reflects a bipartisan consensus, rare in Washington, that asteroid defense is worth the expenditure. A 2025 survey found that a majority of Americans support increased spending on asteroid detection and deflection [11].

The Complications No One Expected

The DART results were not uniformly reassuring. Researchers at the University of Maryland discovered that the impact ejected massive boulders from Dimorphos's surface — some measuring several meters across — that created forces in unexpected directions [12]. These wayward projectiles could complicate future deflection efforts, particularly for rubble-pile asteroids where the response to a kinetic impact may be less predictable than for solid bodies.

The finding underscores a critical lesson: while DART proved that kinetic impact works in principle, the physics of asteroid deflection are more complex than simplified models suggest. Binary asteroid systems introduce additional variables — the gravitational interplay between two bodies, the redistribution of debris, and the potential for secondary impacts between the asteroids themselves.

"We must continue to test other deflection techniques to have a varied planetary defense arsenal of response options that would best address the type of object we might have to deflect," NASA officials have stated [8].

Hera: The Follow-Up Investigation

The European Space Agency is already en route to fill in the gaps DART left behind. The Hera spacecraft, launched on October 7, 2024, aboard a SpaceX Falcon 9, is expected to reach the Didymos system by late 2026 — approximately four years after the DART impact [13].

Hera represents the second half of what is effectively a joint international experiment. Where DART was the hammer, Hera is the microscope. The spacecraft will map the entire surface of Dimorphos at a resolution of just a few meters, with the impact vicinity mapped at 10-centimeter resolution [14]. It will deploy two CubeSat companions: Milani, which will study dust and surface composition through spectral imaging, and Juventas, which will probe Dimorphos's interior structure using radar — the first time the internal properties of any binary asteroid have been directly measured [13].

These measurements will be critical for refining the momentum enhancement factor and understanding how different asteroid compositions respond to kinetic impacts. They will also provide ground truth for the heliocentric deflection measurements reported by Makadia's team — either confirming or refining the 0.15-second orbital period change that has made headlines worldwide.

As of March 2026, Hera had already completed a Mars flyby and was traversing the asteroid belt, testing its instruments on faint asteroids encountered along its trajectory [14]. ESA has indicated the spacecraft may arrive a month ahead of its original December 2026 schedule [14].

Source: NASA / Science Advances (Makadia et al. 2026)

Data as of Mar 9, 2026CSV

What Comes Next

DART answered the foundational question — yes, humanity can move an asteroid. But it also revealed how much remains unknown. The next generation of planetary defense missions will need to address several unresolved challenges:

Detection: The Vera C. Rubin Observatory, expected to begin full science operations in the coming years, will dramatically expand the catalog of known near-Earth objects. NASA's NEO Surveyor mission, an infrared space telescope designed specifically to find dark, hard-to-detect asteroids, remains a priority for the Planetary Defense Coordination Office [8].

Diverse deflection methods: Kinetic impact is only one tool. For larger asteroids or those discovered with less lead time, gravity tractors (spacecraft that use gravitational attraction to slowly tug an asteroid off course), ion beam deflection, and even nuclear standoff detonation may be required. Each method requires testing and validation [8].

International coordination: Asteroid impacts are a global threat requiring a global response. The DART-Hera partnership between NASA and ESA represents a model for future cooperation, but scaling that coordination to handle an actual emergency — with compressed timelines and geopolitical pressures — remains a challenge that has barely been explored [13].

Binary asteroid dynamics: The discovery that impacting one member of a binary pair can deflect the entire system opens new strategic possibilities. But it also demands a deeper understanding of how binary asteroids transfer momentum internally — knowledge that Hera's close-up observations should begin to provide [3].

A Species-Level Achievement

The significance of DART extends beyond planetary defense into something more fundamental. For the first time in 4.5 billion years of solar system history, a species evolved on one of its planets, built a machine, launched it into deep space, and measurably altered the orbital mechanics of another world.

The change was small — 0.15 seconds shaved from a 770-day orbit, 11.7 micrometers per second of velocity lost from a system traveling at roughly 23 kilometers per second around the Sun. But the principle it demonstrated is without precedent: the laws of celestial mechanics, which have governed the motion of every asteroid, comet, and planet since the formation of the solar system, are now subject to human intervention.

Whether that capability will ever be needed in earnest — whether an asteroid bearing down on Earth will one day be nudged aside by a descendant of DART — remains unknown. What is no longer in question is whether it can be done.

The solar system just became a slightly safer place.