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December 15, 2022

Scientists Following a Dusty Tail to Shape the Story of DART’s Impact

This video is constructed of images taken on Nov. 30, 2022, by astronomers at Magdalena Ridge Observatory in New Mexico.

Video of Didymos System on Nov. 30, 2022
This video is constructed of images taken on Nov. 30, 2022, by astronomers at Magdalena Ridge Observatory in New Mexico. It shows the motion of the Didymos system across the sky over the course of roughly 80 minutes, and features a long, linear tail stretching to the right from the asteroid system to the edge of the frame. The animation is roughly 32,000 kilometers across the field of view at the distance of Didymos.

Credit: Magdalena Ridge Observatory/New Mexico Tech


This image is constructed from several images taken on Nov. 30, 2022, by astronomers at Magdalena Ridge Observatory in New Mexico.

Image of Didymos System on Nov. 30, 2022
This image is constructed from several images taken on Nov. 30, 2022, by astronomers at Magdalena Ridge Observatory in New Mexico. It holds Didymos still in the frame, and thus the background stars are seen as linear trails of dots. Average images like this can provide additional details to astronomers studying faint structures in the ejecta tail. This image is roughly 32,000 kilometers across the field of view at the distance of Didymos.

Credit: Magdalena Ridge Observatory/New Mexico Tech


This video is constructed of images taken in the first month after the DART impact by astronomers at the Ōtehīwai Mt. John Observatory in New Zealand.

Video of Didymos System from Sept. 27 to Oct. 21, 2022
This video is constructed of images taken in the first month after the DART impact by astronomers at the Ōtehīwai Mt. John Observatory in New Zealand. Each frame of this video is the average over an entire night of observing, with the telescope holding the Didymos system in the center and the stars appearing as streaks. The length across the animation changes from roughly 110,000 to 129,000 kilometers across the field of view at the distance of Didymos as Didymos recedes from the Earth.

Credit: University of Canterbury Ōtehīwai Mt. John Observatory/UCNZ


Comparison of Pre- and Post-Impact Near-Infrared Spectra of the Didymos-Dimorphos System

Comparison of Pre- and Post-Impact Near-Infrared Spectra of the Didymos-Dimorphos System
The two spectra shown were taken by the NASA Infrared Telescope Facility on Mauna Kea, Hawaii. The data were obtained before and after impact (Sept. 26 and 27, 3 a.m. Hawaii Standard Time). The pre-impact spectrum is dominated by light from Didymos (approximately 96% of the total brightness). Because of the large amount of ejected material, the post-impact spectrum contains approximately two-thirds flux from Dimorphos material. Both spectra show similar characteristics, including the two large absorption features at 1 and 2 microns. These spectra are classified as S-complex and are similar to the spectra of ordinary chondrite meteorites.

Credit: NASA Infrared Telescope Facility/Weizmann Institute of Science/Massachusetts Institute of Technology


LICIACube Enhanced Color Images of the Didymos System

LICIACube Enhanced Color Images of the Didymos System
These images were acquired by the LUKE camera on LICIACube about 3 minutes after DART’s impact into Dimorphos. These enhanced color representations of the Didymos system were created by combining images taken in the red, green and blue wavelengths by LUKE; these enhanced color views do not represent how the asteroids would look to the human eye but serve to highlight color differences in the scene, which can provide information about the characteristics of the ejecta and the asteroids.

Credit: ASI/NASA

Since NASA’s Double Asteroid Redirection Test (DART) spacecraft intentionally slammed into the asteroid moonlet Dimorphos on Sept. 26 — altering its orbit by 33 minutes — the investigation team has been digging into the implications of how this planetary defense technique could be used in the future, if such a need should ever arise. This has included further analysis of the “ejecta” — the many tons of asteroidal rock displaced and launched into space by the impact — the recoil from which substantially enhanced DART’s push against Dimorphos.

Continued observations of that evolving ejecta have given the investigation team better understanding of what the DART spacecraft achieved at the impact site. DART team members provided a preliminary interpretation of their findings during the American Geophysical Union’s Fall Meeting on Thursday, Dec. 15, in Chicago.

“What we can learn from the DART mission is all part of a NASA’s overarching work to understand asteroids and other small bodies in our Solar System,” said Tom Statler, the program scientist for DART at NASA headquarters in Washington, and one of the presenters at the briefing. “Impacting the asteroid was just the start. Now we use the observations to study what these bodies are made of and how they were formed — as well as how to defend our planet should there ever be an asteroid headed our way.”

Central to this effort are detailed, post-impact science and engineering analyses of data from the world’s first planetary defense technology demonstration. In the weeks after impact, scientists turned their focus toward measuring the momentum transfer from DART’s roughly 14,000-mile-per-hour (22,530-kilometer-per-hour) collision with its target asteroid.

Scientists estimate DART’s impact displaced over two million pounds (one million kilograms) of the dusty rock into space — enough to fill six or seven rail cars. The team is using that data — as well as new information on the composition of the asteroid moonlet and the characteristics of the ejecta, gained from telescope observations and images from DART’s ride-along Light Italian CubeSat for Imaging of Asteroids (LICIACube) contributed by the Italian Space Agency (ASI) — to learn just how much DART’s initial hit moved the asteroid, and how much came from the recoil.

“We know the initial experiment worked. Now we can start to apply this knowledge,” said Andy Rivkin, DART investigation team co-lead at the Johns Hopkins Applied Physics Laboratory (APL). “Studying the ejecta made in the kinetic impact — all of it derived from Dimorphos — is a key way of gaining further insights into the nature of its surface.”

Observations before and after impact reveal that Dimorphos and its larger parent asteroid, Didymos, have similar makeup and are composed of the same material — material that has been linked to ordinary chondrites, similar to the most common type of meteorite to impact the Earth. These measurements also took advantage of the ejecta from Dimorphos, which dominated the reflected light from the system in the days after impact. Even now, telescope images of the Didymos system show how solar radiation pressure has stretched the ejecta stream into a comet-like tail tens of thousands of miles in length.

Putting those pieces together, and assuming that Didymos and Dimorphos have the same densities, the team calculates that the momentum transferred when DART hit Dimorphos was roughly 3.6 times greater than if the asteroid had simply absorbed the spacecraft and produced no ejecta at all — indicating the ejecta contributed to moving the asteroid more than the spacecraft did.

Accurately predicting momentum transfer is central to planning a future kinetic impact mission if one is ever needed, including determining the size of the impactor spacecraft and estimating the amount of lead time necessary to ensure that a small deflection would move a potentially dangerous asteroid off its path.

“Momentum transfer is one of the most important things we can measure, because it is information we would need to develop an impactor mission to divert a threating asteroid,” said Andy Cheng, DART investigation team lead from APL. “Understanding how a spacecraft impact will change an asteroid’s momentum is key to designing a mitigation strategy for a planetary defense scenario.”

Neither Dimorphos nor Didymos poses any hazard to Earth before or after DART’s controlled collision with Dimorphos.

APL built and operated the DART spacecraft and manages the DART mission for NASA’s Planetary Defense Coordination Office as a project of the agency’s Planetary Missions Program Office.

For more information about the DART mission, visit https://www.nasa.gov/dart or DART.jhuapl.edu.

Media contacts:
Justyna Surowiec, 240-228-8103, Justyna.Surowiec@jhuapl.edu
Josh Handal, NASA Headquarters, Washington, 202-374-9832, joshua.a.handal@nasa.gov

The Applied Physics Laboratory, a not-for-profit division of The Johns Hopkins University, meets critical national challenges through the innovative application of science and technology. For more information, visit www.jhuapl.edu.

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