Colliding NASA's DART probe with asteroid Dimorphos in September 2022 appears to have altered the tiny asteroid's shape significantly. The impact provides insights into Dimorphos' formation and hints that the next mission may discover a reshaped pile of space rock instead of an impact crater.
A television at NASA's Kennedy Space Center in Cape Canaveral, Florida, captures the final images from the Double Asteroid Redirection Test (DART) just before it smashes into the asteroid Dimorphos on September 26, 2022.
Insights from the DART Mission's Impact on the Asteroid's Structure and Origins
The Double Asteroid Redirection Test (DART) mission focused on planetary safety, exploring the possibility of altering an asteroid's trajectory by colliding with it using a spacecraft. Dimorphos, a smaller asteroid in mutual orbit with Didymos, served as the targeted object.
The mission's success, impacting Dimorphos and changing its orbital period more than anticipated, raised questions about ongoing effects, asteroid redirection implications, and insights into Dimorphos.
Scientists, led by planetary scientist Sabina Raducan of the University of Bern, pursued an alternative approach to monitor the space rock. They employed simulated models of Dimorphos and the DART spacecraft, aiming to replicate observed impact effects, including momentum transfer, erupted material quantity, and the formation of an ejecta cone. To achieve this, they adjusted unknown variables such as Dimorphos' composition and density.
Asteroids exhibit diverse structures, ranging from dense fragments to loose aggregates known as "rubble piles." Both Didymos and Dimorphos fall into the latter category. The simulations based on DART observations suggested that Dimorphos is a very weak rubble pile, lacking surface scarring but undergoing global deformation and resurfacing due to the impact.
The simulations indicated a cohesive strength for Dimorphos of less than a few pascals, similar to asteroids Ryugu and Bennu previously explored by human spacecraft. Dimorphos' low density, around 2.4 grams per cubic centimeter, aligns with its rubble pile classification, differing slightly from the densities of Ryugu and Bennu.
These findings imply that Dimorphos may have originated from Didymos, with rubble pile debris shedding and coalescing over time into the loosely structured asteroid targeted by the DART mission.
Guiding Future Exploration Efforts for Asteroid Deflection
Scheduled for later this year, the European Space Agency's Hera mission is poised to examine Didymos and Dimorphos, potentially confirming the accuracy of the team's simulations and advancing our comprehension of Dimorphos. The mission's outcomes could furnish crucial insights into safeguarding Earth from potential asteroid impacts.
Despite the non-extinction nature of recent impactful incidents, such as the Chelyabinsk meteor and the Tunguska impact, they underscore the substantial potential for damage and loss of life with smaller celestial bodies. The critical factor lies in the ability to predict an object's trajectory well in advance, facilitating proactive alterations to divert the asteroid's path.
Anticipating a surge in such missions, private enterprises may explore the prospect of asteroid mining for valuable metals. The straightforward extraction of material from asteroids intensifies interest in studying their evolutionary processes and the implications for impending asteroid redirection endeavors.
The DART spacecraft's impact on Dimorphos implies that moons formed similarly to asteroids are easily reshaped, providing valuable insights into the formation and characteristics of binary asteroids. This knowledge is poised to guide future exploration efforts and strategies for asteroid deflection.
RELATED ARTICLE: NASA's DART Spacecraft Worked! Asteroid Killer Changed the Harmless Space Rock's Orbit More Than Expected
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