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NASA's ambitious Double Asteroid Redirection Test (DART) mission continues to unravel the enigmatic past of its celestial targets long after the spacecraft's impactful end. Groundbreaking research gleaned from the mission's aftermath has significantly advanced our understanding of the formation and evolution of near-Earth asteroids, yielding invaluable knowledge not only for planetary defense but for our greater comprehension of Solar System history.
In a series of five scholarly papers published in Nature Communications, scientists have dissected the geological fabric of a distant binary asteroid system, consisting of Dimorphos—a moonlet, and Didymos—the primary asteroid. This binary pair, intriguingly mismatched in both size and surface characteristics, has become a richer source of Solar System insights following DART's deliberate collision with Dimorphos.
As revealed by these post-mission studies, the moonlet Dimorphos flaunts an assorted topography replete with boulders of diverse dimensions. By contrast, Didymos exhibits a smoother landscape at lower altitudes but a more rugged, cratered air at higher ones. Researchers, led by Olivier Barnouin and Ronald-Louis Ballouz of the Johns Hopkins Applied Physics Laboratory, suggest that Dimorphos emerged from Didymos during a colossal shedding event, a cosmic phenomenon where rotational forces result in material segregation from a parent body.
The assessment of the asteroid pair infers a stark age difference between the two; Didymos's surface is hypothesized to be 40–130 times older than that of its companion, with respective age estimations of 12.5 million years and a youthful sub-300,000 years for Dimorphos. Such a low-strength surface almost certainly contributed to DART's significant impact effectiveness in altering the moonlet's trajectory.
Digging deeper into the asteroids' makeup, another paper helmed by Maurizio Pajola of the National Institute for Astrophysics involved a meticulous comparison of the boulders across both celestial bodies. Results point to a stepwise formation of Dimorphos, from debris that once belonged to Didymos. This supports a model where binary asteroids, such as Didymos-Dimorphos, are born from the accumulation of matter cast off by a larger parent.
Scoping the surface for patterns of thermal distress, Alice Lucchetti and her team recognized rapid boulder decomposition triggered by thermal fatigue—a process expedited beyond prior estimations. This discovery underscores the unique relevance of the DART mission, which likely marked the first observational evidence of such a dynamic on this asteroid class.
Shedding light on the asteroid's bearing capacity, essential for predicting surface response to applied pressures—useful for both exploration and potential asteroid redirection attempts—Jeanne Bigot and Pauline Lombardo, guided by researcher Naomi Murdoch, disclosed Didymos's surface supports substantially less weight compared to Earth's dry sand or lunar soil.
Finally, Colas Robin and co-authors analyzed the surface boulders' structure and formation, tying their characteristics to those found on other known rubble pile asteroids. The similarities suggest a unified pattern of asteroidal formation and response to cataclysmic impacts across the cosmos.
The trove of data procured by DART acts as a precursor to ESA's upcoming Hera mission that is set to revisit and study the aftereffects of humanity's inaugural test of planetary defense. By integrating these new revelations into Hera's expectations, scientists can refine their hypotheses and technical preparedness for future exploratory ventures and protective measures.
Johns Hopkins APL's management of the DART mission, under NASA's Planetary Defense Coordination Office, showcases the collaborative network encompassing JPL, Goddard Space Flight Center, Johnson Space Center, Glenn Research Center, and Langley Research Center in a collective effort to guard our home, Earth, from celestial threats.