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  3. Successful Kinetic Impact into an Asteroid for Planetary Defense.
 

Successful Kinetic Impact into an Asteroid for Planetary Defense.

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BORIS DOI
10.48350/179411
Date of Publication
April 2023
Publication Type
Article
Division/Institute

Physikalisches Instit...

Contributor
Daly, R Terik
Ernst, Carolyn M
Barnouin, Olivier S
Chabot, Nancy L
Rivkin, Andrew S
Cheng, Andrew F
Adams, Elena Y
Agrusa, Harrison F
Abel, Elisabeth D
Alford, Amy L
Asphaug, Erik I
Atchison, Justin A
Badger, Andrew R
Baki, Paul
Ballouz, Ronald-L
Bekker, Dmitriy L
Bellerose, Julie
Bhaskaran, Shyam
Buratti, Bonnie J
Cambioni, Saverio
Chen, Michelle H
Chesley, Steven R
Chiu, George
Collins, Gareth S
Cox, Matthew W
DeCoster, Mallory E
Ericksen, Peter S
Espiritu, Raymond C
Faber, Alan S
Farnham, Tony L
Ferrari, Fabioorcid-logo
Physikalisches Institut - Space Research and Planetology Physics
Physikalisches Institut der Universität Bern
Fletcher, Zachary J
Gaskell, Robert W
Graninger, Dawn M
Haque, Musad A
Harrington-Duff, Patricia A
Hefter, Sarah
Herreros, Isabel
Hirabayashi, Masatoshi
Huang, Philip M
Hsieh, Syau-Yun W
Jacobson, Seth A
Jenkins, Stephen N
Jensenius, Mark A
John, Jeremy W
Jutzi, Martinorcid-logo
Physikalisches Institut - Space Research and Planetology Physics
Space Research and Planetology Physics - Impacts
Physikalisches Institut der Universität Bern
Kohout, Tomas
Krueger, Timothy O
Laipert, Frank E
Lopez, Norberto R
Luther, Robert
Lucchetti, Alice
Mages, Declan M
Marchi, Simone
Martin, Anna C
McQuaide, Maria E
Michel, Patrick
Moskovitz, Nicholas A
Murphy, Ian W
Murdoch, Naomi
Naidu, Shantanu P
Nair, Hari
Nolan, Michael C
Ormö, Jens
Pajola, Maurizio
Palmer, Eric E
Peachey, James M
Pravec, Petr
Raducan, Sabina-Denisa
Physikalisches Institut - Space Research and Planetology Physics
Space Research and Planetology Physics - Impacts
Physikalisches Institut der Universität Bern
Ramesh, K T
Ramirez, Joshua R
Reynolds, Edward L
Richman, Joshua E
Robin, Colas Q
Rodriguez, Luis M
Roufberg, Lew M
Rush, Brian P
Sawyer, Carolyn A
Scheeres, Daniel J
Scheirich, Petr
Schwartz, Stephen R
Shannon, Matthew P
Shapiro, Brett N
Shearer, Caitlin E
Smith, Evan J
Steele, R Joshua
Steckloff, Jordan K
Stickle, Angela M
Sunshine, Jessica M
Superfin, Emil A
Tarzi, Zahi B
Thomas, Cristina A
Thomas, Justin R
Trigo-Rodríguez, Josep M
Tropf, B Teresa
Vaughan, Andrew T
Velez, Dianna
Waller, C Dany
Wilson, Daniel S
Wortman, Kristin A
Zhang, Yun
Subject(s)

500 - Science::530 - ...

500 - Science::520 - ...

600 - Technology::620...

Series
Nature
ISSN or ISBN (if monograph)
1476-4687
Publisher
Springer Nature
Language
English
Publisher DOI
10.1038/s41586-023-05810-5
PubMed ID
36858073
Description
While no known asteroid poses a threat to Earth for at least the next century, the catalog 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 the first 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 DART's impact4. While 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 Dimorphos's orbit7 demonstrates that kinetic impactor technology is a viable technique to potentially defend Earth if necessary.
Handle
https://boris-portal.unibe.ch/handle/20.500.12422/164626
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File(s)
FileFile TypeFormatSizeLicensePublisher/Copright statementContent
s41586-023-05810-5_reference.pdftextAdobe PDF12.71 MBacceptedOpen
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