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The strong rebound effect amplified NASA’s asteroid deflection experiments

A composite image of the Didymos-Dimorphos system taken on Nov. 30 shows the new projectile tail.

Scientists continue to observe remarkable results from NASA’s DART test that successfully deflected a harmless asteroid. As recent results show, the recoil from the blast of debris emitted by Dimorphos after the impact was significant, increasing the spacecraft’s impact on the asteroid.

NASA’s spacecraft is about the size of a refrigerator to destroy At 535 feet (163 meters) Dimorphus on September 26, Shortening its orbit around its larger partnerDidymus, with an impressive time of 33 minutes. This equates to tens of feet, which indicates feasibility using kinetic punches as a means of deflecting menacing asteroids.

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A notable side effect of this test is… Giant and complex column emitted by the asteroid after the collision. The Didymus-Dimorphos system, located 7 million miles (11 million km) from Earth, even developed a long tail after the experiment. DART, short for Double Asteroid Redirection Test, had a profound effect on Dimorphos, releasing an incredible amount of debris, or “projectiles” in the parlance of planetary scientists.

Dimorphos, as we’ve learned, is a debris-filled asteroid, as opposed to a solid, rocky body. This undoubtedly contributed to an increase in the amount of debris ejected, but scientists aren’t sure how much debris was ejected from the asteroid following the impact. preliminary hits A presentation Thursday at the American Geophysical Union’s fall meeting in Chicago sheds light on this and other aspects of the DART mission.

Not only does the DART fire tons of projectiles, but it also creates a ricochet effect that pushes the asteroid in the desired direction, Andy Rifkin, head of the DART’s investigative team, explained at the meeting. “We get a lot of benefits,” he said Inform BBC News.

In fact, had the Dimorphos had a more compact body, the same level of recoil might not have occurred. “If you bomb off-target material, you have a kickback force,” explained DART mission scientist Andy Cheng of the Johns Hopkins University Applied Physics Laboratory, who also spoke at the meeting. The resulting bounce is similar to releasing a balloon. As the air escapes, it pushes the balloon in the opposite direction. In the case of Dimorphos, the ejecta stream is air leaving the balloon, which also pushes the asteroid in the opposite direction.

Planetary scientists are starting to understand how much debris has been moved. The DART, traveling at 14,000 mph (22,500 km/h), struck hard enough to topple more than two million pounds of material into the void. NASA says it’s enough to fill about six or seven railroad cars declaration. The estimate may actually be low, Rifkin said at the meeting, with the real number perhaps ten times that.

The scientists set DART’s momentum factor, known as “beta”, to a value of 3.6, meaning that the momentum imparted to Dimorphos was 3.6 times greater than in a collision event that did not result in the ejection of a plume. “The result of that recoil is that you give the target more momentum and end up with a bigger deflection,” Cheng told reporters. “If you’re trying to save the Earth, it makes a big difference.”

That’s a good point, because those values ​​will set the criteria for a real mission to legally deflect a dangerous asteroid. Cheng and his colleagues will now use these results to infer beta values ​​for other asteroids, a task that requires a deeper understanding of the objects’ density, composition, porosity and other parameters. Scientists also hope to find out how far the DART’s first impact moved the asteroid and how far it moved as a result of the reflection.

Amplifiers also produce another character: the long tail, or output shaft, that forms after impact. According to Rifkin, Dimorphos developed a tail 18,600 miles (30,000 km) long.

“The asteroid impact was just the beginning,” Tom Statler, scientist and DART program presenter at the meeting, said in a statement. “We are now using the observations to understand what these objects are made of and how they formed – and how to defend our planet if an asteroid heads our way.”

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