Momentum transfer from the DART mission kinetic impact on asteroid Dimorphos
Author:
Cheng Andrew F.ORCID, Agrusa Harrison F.ORCID, Barbee Brent W.ORCID, Meyer Alex J., Farnham Tony L.ORCID, Raducan Sabina D.ORCID, Richardson Derek C.ORCID, Dotto Elisabetta, Zinzi Angelo, Della Corte Vincenzo, Statler Thomas S.ORCID, Chesley StevenORCID, Naidu Shantanu P.ORCID, Hirabayashi MasatoshiORCID, Li Jian-YangORCID, Eggl SiegfriedORCID, Barnouin Olivier S.ORCID, Chabot Nancy L.ORCID, Chocron SidneyORCID, Collins Gareth S.ORCID, Daly R. TerikORCID, Davison Thomas M.ORCID, DeCoster Mallory E.ORCID, Ernst Carolyn M., Ferrari FabioORCID, Graninger Dawn M.ORCID, Jacobson Seth A.ORCID, Jutzi Martin, Kumamoto Kathryn M.ORCID, Luther RobertORCID, Lyzhoft Joshua R.ORCID, Michel PatrickORCID, Murdoch Naomi, Nakano RyotaORCID, Palmer EricORCID, Rivkin Andrew S.ORCID, Scheeres Daniel J.ORCID, Stickle Angela M., Sunshine Jessica M., Trigo-Rodriguez Josep M.ORCID, Vincent Jean-Baptiste, Walker James D.ORCID, Wünnemann KaiORCID, Zhang YunORCID, Amoroso Marilena, Bertini IvanoORCID, Brucato John R.ORCID, Capannolo Andrea, Cremonese GabrieleORCID, Dall’Ora Massimo, Deshapriya Prasanna J. D., Gai Igor, Hasselmann Pedro H., Ieva SimoneORCID, Impresario GabrieleORCID, Ivanovski Stavro L., Lavagna Michèle, Lucchetti AliceORCID, Epifani Elena M., Modenini Dario, Pajola MaurizioORCID, Palumbo Pasquale, Perna DavideORCID, Pirrotta Simone, Poggiali GiovanniORCID, Rossi AlessandroORCID, Tortora PaoloORCID, Zannoni MarcoORCID, Zanotti GiovanniORCID
Abstract
AbstractThe 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 26 September 2022 as a planetary defence test1. DART was the first hypervelocity impact experiment on an asteroid at size and velocity scales relevant to planetary defence, intended to validate kinetic impact as a means of asteroid deflection. Here we report a determination of the momentum transferred to an asteroid by kinetic impact. On the basis of 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, β, 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, $${\beta =3.61}_{-0.25}^{+0.19}(1\sigma )$$
β
=
3.61
−
0.25
+
0.19
(
1
σ
)
. These β values indicate that substantially 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.
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Cited by
89 articles.
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