{"id":23990,"date":"2024-08-04T23:27:31","date_gmt":"2024-08-04T15:27:31","guid":{"rendered":"https:\/\/wp-productionenv-bjg9h2g2bgg5b8aa.southeastasia-01.azurewebsites.net\/news\/using-data-from-darts-impact-scientists-investigate-characteristics-of-dimorphos-and-didymos\/"},"modified":"2024-08-04T23:27:31","modified_gmt":"2024-08-04T15:27:31","slug":"using-data-from-darts-impact-scientists-investigate-characteristics-of-dimorphos-and-didymos","status":"publish","type":"post","link":"https:\/\/starpath.global\/news\/using-data-from-darts-impact-scientists-investigate-characteristics-of-dimorphos-and-didymos\/","title":{"rendered":"Using data from DART\u2019s impact, scientists investigate characteristics of Dimorphos and Didymos"},"content":{"rendered":"<p>In September 2022, NASA\u2019s Double Asteroid Redirection Test (DART) mission successfully slammed into the side of asteroid moonlet Dimorphos. Initial data from the event indicated that DART had successfully altered the orbit of Dimorphos and achieved its primary mission goal \u2014 to assess how much a spacecraft could deflect an asteroid through a transfer of momentum.<\/p>\n<p>However, data analysis didn\u2019t stop, and DART\u2019s science team has released new results and information on why DART was so effective in changing Dimorphos\u2019 orbit and the origins of Dimorphos and its binary asteroid system.<\/p>\n<\/p>\n<p>The new results and information were released via five new papers published in&nbsp;<em>Nature Communications<\/em>. In the papers, DART\u2019s science team explored the geology of Dimorphos and its parent asteroid, Didymos, to characterize the origins of the asteroids and their binary system. Additionally, the team\u2019s research allowed them to learn more about how the binary system evolved and constrain the physical characteristics of the asteroids.<\/p>\n<p>\u201cThese findings give us new insights into the ways that asteroids can change over time. This is important not just for understanding the near-Earth objects that are the focus of planetary defense, but also for our ability to read the history of our Solar System from these remnants of planet formation. This is just part of the wealth of new knowledge we\u2019ve gained from DART,\u201d said Thomas Statler, who serves as the lead scientist for Solar System Small Bodies at NASA Headquarters in Washington D.C.<\/p>\n<\/p>\n<p><iframe title=\"DART Impact\" src=\"https:\/\/www.youtube.com\/embed\/N-OvnVdZP_8?feature=oembed\" frameborder=\"0\" allow=\"accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share\" referrerpolicy=\"strict-origin-when-cross-origin\" allowfullscreen=\"\" name=\"fitvid0\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\"><\/iframe><\/p>\n<p>Using images taken by DART and the LICIACube cubesat, one team \u2014 led by Olivier Barnouin and Ronald-Louis Ballouz of the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland \u2014 investigated the topography of Dimorphos and found small boulders of varying sizes all across the surface of the moonlet. Interestingly, the larger Didymos featured a smoother surface at lower elevations and a rocky surface at higher elevations. Additionally, Didymos was found to have more craters across its surface than Dimorphos.<\/p>\n<h4 class=\"widget-title penci-border-arrow\">See Also<\/h4>\n<ul>\n<li>DART Updates<\/li>\n<li>Space Science Section<\/li>\n<li>NSF Store<\/li>\n<li>Click here to Join L2<\/li>\n<\/ul>\n<p>These surface characteristics led the team to conclude that Dimorphos likely spun off from Didymos during a large mass-shedding event. The spins of small asteroids can rapidly accelerate through natural processes, and there is growing evidence that these processes may be responsible for re-shaping asteroids and\/or forcing material off of their surfaces.&nbsp; If enough material is thrown from the surface, it can reshape itself into a smaller asteroid, much like that of Dimorphos.<\/p>\n<p>SpaceX launch tickets<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>NASA mission patches<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>Space Technology<path d=\"M7.59009 18.59L9.00009 20L17.0001 12L9.00009 4L7.59009 5.41L14.1701 12\" style=\"animation: initial !important; background: initial !important; border: 0px !important; box-shadow: none !important; color: inherit !important; cursor: inherit !important; direction: inherit !important; display: inline !important; fill: currentcolor !important; filter: initial !important; float: none !important; margin: 0px !important; opacity: initial !important; outline: 0px !important; overflow: initial !important; padding: 0px !important; stroke: initial !important; transform: initial !important; vertical-align: initial !important; visibility: inherit !important;\"><\/path>\n<p>     (adsbygoogle = window.adsbygoogle || []).push({});<\/p>\n<p>The team estimates that Didymos has a surface that is 40 to 130 times older than Dimorphos, with Didymos\u2019 surface being around 12.5 million years old and Dimorphos\u2019 surface being less than 300,000 years old. With Dimorphos\u2019 surface being so young, it is not nearly as strong as Didymos\u2019 surface, which is why DART\u2019s impact likely impacted the moonlet\u2019s orbit so significantly.<\/p>\n<p>\u201cThe images and data that DART collected at the Didymos system provided a unique opportunity for a close-up geological look of a near-Earth asteroid binary system. From these images alone, we were able to infer a great deal of information on the geophysical properties of both Didymos and Dimorphos and expand our understanding on the formation of these two asteroids. We also better understand why DART was so effective in moving Dimorphos,\u201d Barnouin explained.<\/p>\n<p><img fetchpriority=\"high\" decoding=\"async\" aria-describedby=\"caption-attachment-101275\" class=\"size-full wp-image-101275\" src=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/08\/didymos-ridgeformation-press-release-fig1-scaled.webp\" alt=\"\" width=\"2560\" height=\"532\" srcset=\"https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/08\/didymos-ridgeformation-press-release-fig1-scaled.webp 2560w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/08\/didymos-ridgeformation-press-release-fig1-350x73.webp 350w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/08\/didymos-ridgeformation-press-release-fig1-630x131.webp 630w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/08\/didymos-ridgeformation-press-release-fig1-768x160.webp 768w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/08\/didymos-ridgeformation-press-release-fig1-1920x399.webp 1920w, https:\/\/www.nasaspaceflight.com\/wp-content\/uploads\/2024\/08\/didymos-ridgeformation-press-release-fig1-1170x243.webp 1170w\" sizes=\"(max-width: 2560px) 100vw, 2560px\"><\/p>\n<p id=\"caption-attachment-101275\" class=\"wp-caption-text\">Figures from Barnouin et al.\u2019s paper. The first three panels (from the left) all highlight the sloping of Dimorphos\u2019 surface. The final panel shows the effects of spin-up disruption on Didymos. (Credit: Johns Hopkins APL\/Olivier Barnouin)<\/p>\n<p>In another paper, a team led by Maurizio Pajola of the National Institute for Astrophysics (INAF) in Rome compared the shapes and sizes of various boulders and their distribution patterns across both Dimorphos and Didymos\u2019s surfaces. Pajola et al.\u2019s results showed that the physical characteristics of Dimorphos indicate that the moonlet formed in stages, likely from material inherited from Didymos. These results reinforce the longstanding theory that binary asteroid systems form from the shedding of material from the larger parent asteroid.<\/p>\n<p>The third paper, led by Alice Lucchetti of INAF, revealed that thermal fatigue, or the gradual weakening and cracking of a material due to heat, could rapidly break up boulders on the surface of Dimorphos. The breaking of these boulders could generate surface lines and alter the physical characteristics of asteroids similar to Dimorphos more rapidly than previously thought. Lucchetti et. al. believe that DART\u2019s observations were likely the first time this phenomenon has ever been observed on this type of asteroid.<\/p>\n<p>Led by students Jeanne Bigot and Pauline Lombardo, the fourth paper explored and determined Didymos\u2019 bearing capacity, or an asteroid\u2019s surface\u2019s ability to support applied loads. The students found Didymos\u2019 bearing capacity to be 1,000 times lower than that of dry sand on Earth or lunar soil on the Moon. Information on an asteroid\u2019s bearing capacity can prove to be very useful for understanding and predicting the response of a surface to different events, including displacing and removing an asteroid from its orbit.<\/p>\n<p><iframe id=\"twitter-widget-1\" scrolling=\"no\" frameborder=\"0\" allowtransparency=\"true\" allowfullscreen=\"true\" class=\"\" style=\"position: absolute; visibility: hidden; width: 0px; height: 0px; display: block; flex-grow: 1;\" title=\"X Post\" src=\"https:\/\/platform.twitter.com\/embed\/Tweet.html?creatorScreenName=haygenwarren&amp;dnt=true&amp;embedId=twitter-widget-1&amp;features=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%3D%3D&amp;frame=false&amp;hideCard=false&amp;hideThread=false&amp;id=1818364240824353191&amp;lang=en&amp;origin=https%3A%2F%2Fwww.nasaspaceflight.com%2F2024%2F08%2Fdart-impact-data%2F&amp;sessionId=f514b5546bb9c6e2426a9aff28b3bc1de332b00e&amp;siteScreenName=NASASpaceflight&amp;theme=light&amp;widgetsVersion=6a3ad42b224df%3A1778106238597&amp;width=550px\" data-gtm-yt-inspected-14=\"true\" data-gtm-yt-inspected-21=\"true\" data-tweet-id=\"1818364240824353191\"><\/iframe><\/p>\n<blockquote class=\"twitter-tweet\" data-width=\"550\" data-dnt=\"true\" data-twitter-extracted-i1783494293199412427=\"true\">\n<p lang=\"en\" dir=\"ltr\">A new spin on asteroid formation: how observations from the #DARTMission are refining our understanding of how some binary asteroid pairs come to be https:\/\/t.co\/yYyEjINqeg pic.twitter.com\/Dj9JhvrozL<\/p>\n<p>\u2014 NASA Solar System (@NASASolarSystem) July 30, 2024<\/p>\n<\/blockquote>\n<p>The fifth and final paper, led by Colas Robin of ISAE-SUPAERO, investigated and analyzed the surface boulders on Dimorphos and compared them to those on other \u201crubble pile\u201d asteroids like Ryugu, Itokawa, and Bennu. Robin et al. found that the boulders all shared similar characteristics, which suggests that all of these rubble pile asteroids formed and evolved in similar ways. The team also mentioned that the elongated nature of boulders and other surface materials around the DART impact site likely means that they were formed through impact processing.<\/p>\n<p>These papers provide a more robust overview of not only how the Didymos system formed but also how asteroids and binary systems similar to it formed in our solar system. When the European Space Agency\u2019s (ESA) Hera mission visits the DART impact site at Dimorphos in 2026, the spacecraft will further analyze the aftermath of the impact, and these five papers help provide the necessary context and information that Hera\u2019s teams will need to properly assess the impact site. Additionally, the research adds to scientists\u2019 understanding of planetary science and asteroid characteristics \u2014 vital information needed for understanding our solar system, its origins, and how it has evolved.<\/p>\n<p><em>(Lead image: Artist\u2019s rendering of DART before impacting Dimorphos. Credit: NASA)<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>In September 2022, NASA\u2019s Double Asteroid Redirection Test (DART) mission successfully slammed into the side of asteroid moonlet Dimorphos. Initial data from the event indicated that DART had successfully altered the orbit of Dimorphos and achieved its primary mission goal \u2014 to assess how much a spacecraft could deflect an asteroid through a transfer of [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"inline_featured_image":false,"footnotes":"","_links_to":"","_links_to_target":""},"categories":[2],"tags":[4365,8257,1285,1848,1849,8038,246,1286,190,1561,1563],"class_list":["post-23990","post","type-post","status-publish","format-standard","hentry","category-news","tag-asteroid","tag-asteroid-deflection","tag-dart","tag-didymos","tag-dimorphos","tag-double-asteroid-redirection-test","tag-esa","tag-hera","tag-nasa","tag-planetary-science","tag-solar-system"],"acf":[],"_links":{"self":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/23990"}],"collection":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/comments?post=23990"}],"version-history":[{"count":0,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/posts\/23990\/revisions"}],"wp:attachment":[{"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/media?parent=23990"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/categories?post=23990"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/starpath.global\/blog\/wp-json\/wp\/v2\/tags?post=23990"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}