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Imagery of Early Results from NASA’s DART Mission

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. 

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. 

motion of the Didymos system across the sky
This video is constructed of images taken on November 30, 2022 by astronomers at Magdalena Ridge Observatory in New Mexico, USA. 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.
Magdalena Ridge Observatory/NM Tech
Didymos still in the frame, and thus the background stars are seen as linear trails of dots.
This image is constructed from several images taken on November 30, 2022 by astronomers at Magdalena Ridge Observatory in New Mexico, USA. 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.
Magdalena Ridge Observatory/NM Tech
average over an entire night of observing, with the telescope holding the Didymos system in the center and the stars appearing as streaks
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—129,000 kilometers across the field of view at the distance of Didymos as Didymos recedes from the Earth.
University of Canterbury Ōtehīwai Mt. John Observatory/UCNZ
two spectra shown were taken on the NASA Infrared Telescope Facility on Mauna Kea, Hawaii
The two spectra shown were taken on the NASA Infrared Telescope Facility on Mauna Kea, Hawaii. The data were obtained before and after impact (September 26 u0026amp; 27, 3:00 a.m. Hawaii Standard Time). The pre-impact spectrum is dominated by light from Didymos (~96% of the total brightness). Due to 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.
NASA Infrared Telescope Facility/Weizmann Institute of Science/Massachusetts Institute of Technology
the Didymos system were created by combining images taken in the red, green, and blue wavelengths by LUKE
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.
ASI/NASA