Researchers simulate defense of the Earth against asteroid impact

−3), the overburden pressure in the center of the body is about 2 Pa. The background gradient shows the transition to the gravity-dominated regime, where the target’s overburden pressure at the cratering depth exceeds the cohesion. The formation times, T, of the postimpact stable structures are shown at the top of the figure. Credit: The Planetary Science Journal (2022). DOI: 10.3847/PSJ/ac67a7″ width=”800″ height=”530″/>

Two-dimensional slices (taken at y = 0 in the x–z plane) showing possible asteroid morphologies after DART-like impacts on initially 150 m spherical bodies with varying cohesion (Y0 = 0–50 Pa) and coefficients of internal friction (f = 0.4–1.0). Impacts into targets with Y0 larger than ≈10 Pa create well-defined craters, while impacts into targets with Y0 ≲ 10 Pa create the shape deformation of the asteroid. The total strain shows the amount of deformation experienced by the target. For a 150 m spherical asteroid (ρ ≈ 1600 kg m−3), the overburden pressure in the center of the body is about 2 Pa. The background gradient shows the transition to the gravity-dominated regime, where the target’s overburden pressure at the cratering depth exceeds the cohesion. The formation times, T, of the postimpact stable structures are shown at the top of the figure. Credit: The Planetary Science Journal (2022). DOI: 10.3847/PSJ/ac67a7

NASA’s Double Asteroid Redirection Test (DART) mission is the world’s first full-scale planetary defense test against potential asteroid impacts on Earth. Researchers of the University of Bern and the National Center of Competence in Research (NCCR) PlanetS now show that instead of leaving behind a relatively small crater, the impact of the DART spacecraft on its target could leave the asteroid near unrecognizable.

Sixty-six million years ago, a giant asteroid impact on the Earth likely caused the extinction of the dinosaurs. Currently no known asteroid poses an immediate threat. But if one day a large asteroid were to be discovered on a collision course with Earth, it might have to be deflected from its trajectory to prevent catastrophic consequences.

Last November, the DART space probe of the US space agency NASA was launched as a first full-scale experiment of such a maneuver: Its mission is to collide with an asteroid and to deflect it from its orbit, in order to provide valuable information for the development of such a planetary defense system.

In a new study published in The Planetary Science Journal, researchers of the University of Bern and the National Center of Competence in Research (NCCR) PlanetS have simulated this impact with a new method. Their results indicate that it may deform its target far more severely than previously thought.

Rubble instead of solid rock

“Contrary to what one might imagine when picturing an asteroid, direct evidence from space missions like the Japanese space agency’s (JAXA) Hayabusa2 probe demonstrate that asteroid can have a very loose internal structure—similar to a pile of rubble—that is held together by gravitational interactions and small cohesive forces,” says study lead-author Sabina Raducan from the Institute of Physics and the National Center of Competence in Research PlanetS at the University of Bern.

Yet, previous simulations of the DART mission impact mostly assumed a much more solid interior of its asteroid target Dimorphos. “This could drastically change the outcome of the collision of DART and Dimorphos, which is scheduled to take place in the September,” Raducan points out. Instead of leaving a relatively small crater on the 160 meter wide asteroid, DART’s impact at a speed of 24,000 km/h could completely deform Dimorphos. The asteroid could also be deflected much more strongly and larger amounts of material could be ejected from the impact than the previous estimates predicted.

“One of the reasons that this scenario of a loose internal structure has so far not been thoroughly studied is that the necessary methods were not available,” study lead-author Sabina Raducan says. “Such impact conditions cannot be recreated in laboratory experiments and the relatively long and complex process of crater formation following such an impact—a matter of hours in the case of DART—made it impossible to realistically simulate these impact processes up to now,” according to to the researcher.

“With our novel modeling approach, which takes into account the propagation of the shock waves, the compaction and the consequent flow of material, we were for the first time able to model the entire cratering process resulting from impacts on small, asteroids like Dimorphos, Raducan reports. For this achievement, she was awarded by ESA and by the mayor of Nice at a workshop on the DART follow-up mission HERA.

Widen horizon of expectations

In 2024, the European Space Agency ESA will send a space probe to Dimorphos as part of the space mission HERA. The aim is to visually investigate the aftermath of the DART probe impact. “To get the most out of the HERA mission, we need to have a good understanding of potential outcomes of the DART impact,” says study co-author Martin Jutzi from the Institute of Physics and the National Center of Competence in Research PlanetS.

“Our work on the impact simulations adds an important potential scenario that requires us to widen our expectations in this regard. This is not only relevant in the context of planetary defense, but also adds an important piece to the puzzle of our understanding of asteroids in general,” Jutzi concludes.


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More information:
Sabina D. Raducan et al, Global-scale Reshaping and Resurfacing of Asteroids by Small-scale Impacts, with applications to the DART and Hera Missions, The Planetary Science Journal (2022). DOI: 10.3847/PSJ/ac67a7

Provided by University of Bern

Citation: Researchers simulate defense of the Earth against asteroid impact (2022, June 29) retrieved 29 June 2022 from https://phys.org/news/2022-06-simulate-defense-earth-asteroid-impact.html

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