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  3. Momentum Transfer from the DART Mission Kinetic Impact on Asteroid Dimorphos.
 

Momentum Transfer from the DART Mission Kinetic Impact on Asteroid Dimorphos.

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BORIS DOI
10.48350/179409
Publisher DOI
10.1038/s41586-023-05878-z
PubMed ID
36858075
Description
The NASA Double Asteroid Redirection Test (DART) mission performed a kinetic impact on asteroid Dimorphos, the satellite of the binary asteroid (65803) Didymos, at 23:14 UTC on September 26, 2022 as a planetary defense test1. DART was the first hypervelocity impact experiment on an asteroid at size and velocity scales relevant to planetary defense, intended to validate kinetic impact as a means of asteroid deflection. Here we report the first determination of the momentum transferred to an asteroid by kinetic impact. Based on the change in the binary orbit period2, we find an instantaneous reduction in Dimorphos's along-track orbital velocity component of 2.70 ± 0.10 mm s-1, indicating enhanced momentum transfer due to recoil from ejecta streams produced by the impact3,4. For a Dimorphos bulk density range of 1,500 to 3,300 kg m-3, we find that the expected value of the momentum enhancement factor, [Formula: see text], ranges between 2.2 and 4.9, depending on the mass of Dimorphos. If Dimorphos and Didymos are assumed to have equal densities of 2,400 kg m-3, [Formula: see text]. These [Formula: see text] values indicate that significantly more momentum was transferred to Dimorphos from the escaping impact ejecta than was incident with DART. Therefore, the DART kinetic impact was highly effective in deflecting the asteroid Dimorphos.
Date of Publication
2023-04
Publication Type
Article
Subject(s)
500 Science > 520 Astronomy
600 Technology > 620 Engineering
500 Science > 530 Physics
Language(s)
en
Contributor(s)
Cheng, Andrew F
Agrusa, Harrison F
Barbee, Brent W
Meyer, Alex J
Farnham, Tony L
Raducan, Sabina-Denisa
Physikalisches Institut - Space Research and Planetology Physics
Richardson, Derek C
Dotto, Elisabetta
Zinzi, Angelo
Della Corte, Vincenzo
Statler, Thomas S
Chesley, Steven
Naidu, Shantanu P
Hirabayashi, Masatoshi
Li, Jian-Yang
Eggl, Siegfried
Barnouin, Olivier S
Chabot, Nancy L
Chocron, Sidney
Collins, Gareth S
Daly, R Terik
Davison, Thomas M
DeCoster, Mallory E
Ernst, Carolyn M
Ferrari, Fabioorcid-logo
Physikalisches Institut - Space Research and Planetology Physics
Graninger, Dawn M
Jacobson, Seth A
Jutzi, Martinorcid-logo
Physikalisches Institut - Space Research and Planetology Physics
Kumamoto, Kathryn M
Luther, Robert
Lyzhoft, Joshua R
Michel, Patrick
Murdoch, Naomi
Nakano, Ryota
Palmer, Eric
Rivkin, Andrew S
Scheeres, Daniel J
Stickle, Angela M
Sunshine, Jessica M
Trigo-Rodriguez, Josep M
Vincent, Jean-Baptiste
Walker, James D
Wünnemann, Kai
Zhang, Yun
Amoroso, Marilena
Bertini, Ivano
Brucato, John R
Capannolo, Andrea
Cremonese, Gabriele
Dall'Ora, Massimo
Deshapriya, Prasanna J D
Gai, Igor
Hasselmann, Pedro H
Ieva, Simone
Impresario, Gabriele
Ivanovski, Stavro L
Lavagna, Michèle
Lucchetti, Alice
Epifani, Elena M
Modenini, Dario
Pajola, Maurizio
Palumbo, Pasquale
Perna, Davide
Pirrotta, Simone
Poggiali, Giovanni
Rossi, Alessandro
Tortora, Paolo
Zannoni, Marco
Zanotti, Giovanni
Additional Credits
Physikalisches Institut - Space Research and Planetology Physics
Series
Nature communications
Publisher
Nature Publishing Group
ISSN
2041-1723
Access(Rights)
restricted
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