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Author
Daly, R.T.Ernst, C.M.
Barnouin, O.S.
Chabot, N.L.
Rivkin, A.S.
Cheng, A.F.
Adams, E.Y.
Agrusa, H.F.
Abel, E.D.
Alford, A.L.
Asphaug, E.I.
Atchison, J.A.
Badger, A.R.
Baki, P.
Ballouz, R.-L.
Bekker, D.L.
Bellerose, J.
Bhaskaran, S.
Buratti, B.J.
Cambioni, S.
Chen, M.H.
Chesley, S.R.
Chiu, G.
Collins, G.S.
Cox, M.W.
DeCoster, M.E.
Ericksen, P.S.
Espiritu, R.C.
Faber, A.S.
Farnham, T.L.
Ferrari, F.
Fletcher, Z.J.
Gaskell, R.W.
Graninger, D.M.
Haque, M.A.
Harrington-Duff, P.A.
Hefter, S.
Herreros, I.
Hirabayashi, M.
Huang, P.M.
Hsieh, S.-Y.W.
Jacobson, S.A.
Jenkins, S.N.
Jensenius, M.A.
John, J.W.
Jutzi, M.
Kohout, T.
Krueger, T.O.
Laipert, F.E.
Lopez, N.R.
Luther, R.
Lucchetti, A.
Mages, D.M.
Marchi, S.
Martin, A.C.
McQuaide, M.E.
Michel, P.
Moskovitz, N.A.
Murphy, I.W.
Murdoch, N.
Naidu, S.P.
Nair, H.
Nolan, M.C.
Ormö, J.
Pajola, M.
Palmer, E.E.
Peachey, J.M.
Pravec, P.
Raducan, S.D.
Ramesh, K.T.
Ramirez, J.R.
Reynolds, E.L.
Richman, J.E.
Robin, C.Q.
Rodriguez, L.M.
Roufberg, L.M.
Rush, B.P.
Sawyer, C.A.
Scheeres, D.J.
Scheirich, P.
Schwartz, S.R.
Shannon, M.P.
Shapiro, B.N.
Shearer, C.E.
Smith, E.J.
Steele, R.J.
Steckloff, J.K.
Stickle, A.M.
Sunshine, J.M.
Superfin, E.A.
Tarzi, Z.B.
Thomas, C.A.
Thomas, J.R.
Trigo-Rodríguez, J.M.
Tropf, B.T.
Vaughan, A.T.
Velez, D.
Waller, C.D.
Wilson, D.S.
Wortman, K.A.
Zhang, Y.
Affiliation
University of ArizonaIssue Date
2023-03-01
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Nature ResearchCitation
Daly, R.T., Ernst, C.M., Barnouin, O.S. et al. Successful kinetic impact into an asteroid for planetary defence. Nature 616, 443–447 (2023). https://doi.org/10.1038/s41586-023-05810-5Journal
NatureRights
© The Author(s) 2023. This article is licensed under a Creative Commons Attribution 4.0 International License.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Although no known asteroid poses a threat to Earth for at least the next century, the catalogue of near-Earth asteroids is incomplete for objects whose impacts would produce regional devastation1,2. Several approaches have been proposed to potentially prevent an asteroid impact with Earth by deflecting or disrupting an asteroid1–3. A test of kinetic impact technology was identified as the highest-priority space mission related to asteroid mitigation1. NASA’s Double Asteroid Redirection Test (DART) mission is a full-scale test of kinetic impact technology. The mission’s target asteroid was Dimorphos, the secondary member of the S-type binary near-Earth asteroid (65803) Didymos. This binary asteroid system was chosen to enable ground-based telescopes to quantify the asteroid deflection caused by the impact of the DART spacecraft4. Although past missions have utilized impactors to investigate the properties of small bodies5,6, those earlier missions were not intended to deflect their targets and did not achieve measurable deflections. Here we report the DART spacecraft’s autonomous kinetic impact into Dimorphos and reconstruct the impact event, including the timeline leading to impact, the location and nature of the DART impact site, and the size and shape of Dimorphos. The successful impact of the DART spacecraft with Dimorphos and the resulting change in the orbit of Dimorphos7 demonstrates that kinetic impactor technology is a viable technique to potentially defend Earth if necessary. © 2023, The Author(s).Note
Open access articleISSN
0028-0836PubMed ID
36858073Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1038/s41586-023-05810-5
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Except where otherwise noted, this item's license is described as © The Author(s) 2023. This article is licensed under a Creative Commons Attribution 4.0 International License.
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