dc.contributor.author
Stickle, Angela M.
dc.contributor.author
DeCoster, Mallory E.
dc.contributor.author
Burger, Christoph
dc.contributor.author
Caldwell, Wendy K.
dc.contributor.author
Graninger, Dawn
dc.contributor.author
Kumamoto, Kathryn M.
dc.contributor.author
Luther, Robert
dc.contributor.author
Ormö, Jens
dc.contributor.author
Raducan, Sabina
dc.contributor.author
Rainey, Emma
dc.contributor.author
Schäfer, Christoph M.
dc.contributor.author
Walker, James D.
dc.contributor.author
Zhang, Yun
dc.contributor.author
Michel, Patrick
dc.contributor.author
Michael Owen, J.
dc.contributor.author
Barnouin, Olivier
dc.contributor.author
Cheng, Andy F.
dc.contributor.author
Cochron, Sidney
dc.contributor.author
Collins, Gareth S.
dc.contributor.author
Davison, Thomas M.
dc.contributor.author
Dotto, Elisabetta
dc.contributor.author
Ferrari, Fabio
dc.contributor.author
Isabel Herreros, M.
dc.contributor.author
Ivanovski, Stavro L.
dc.contributor.author
Jutzi, Martin
dc.contributor.author
Lucchetti, Alice
dc.contributor.author
Martellato, Elena
dc.contributor.author
Pajola, Maurizio
dc.contributor.author
Plesko, Cathy S.
dc.contributor.author
Bruck Syal, Megan
dc.contributor.author
Schwartz, Stephen R.
dc.contributor.author
Sunshine, Jessica M.
dc.contributor.author
Wünnemann, Kai
dc.date.accessioned
2022-11-18T11:00:15Z
dc.date.available
2022-11-18T11:00:15Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/36910
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-36623
dc.description.abstract
The Double Asteroid Redirection Test (DART) spacecraft will impact into the asteroid Dimorphos on 2022 September 26 as a test of the kinetic impactor technique for planetary defense. The efficiency of the deflection following a kinetic impactor can be represented using the momentum enhancement factor, β, which is dependent on factors such as impact geometry and the specific target material properties. Currently, very little is known about Dimorphos and its material properties, which introduces uncertainty in the results of the deflection efficiency observables, including crater formation, ejecta distribution, and β. The DART Impact Modeling Working Group (IWG) is responsible for using impact simulations to better understand the results of the DART impact. Pre-impact simulation studies also provide considerable insight into how different properties and impact scenarios affect momentum enhancement following a kinetic impact. This insight provides a basis for predicting the effects of the DART impact and the first understanding of how to interpret results following the encounter. Following the DART impact, the knowledge gained from these studies will inform the initial simulations that will recreate the impact conditions, including providing estimates for potential material properties of Dimorphos and β resulting from DART’s impact. This paper summarizes, at a high level, what has been learned from the IWG simulations and experiments in preparation for the DART impact. While unknown, estimates for reasonable potential material properties of Dimorphos provide predictions for β of 1–5, depending on end-member cases in the strength regime.
en
dc.format.extent
29 Seiten
dc.rights.uri
https://creativecommons.org/licenses/by/4.0/
dc.subject
Double Asteroid Redirection Test (DART) Mission
en
dc.subject
Kinetic Impactor
en
dc.subject.ddc
500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften
dc.title
Effects of Impact and Target Parameters on the Results of a Kinetic Impactor: Predictions for the Double Asteroid Redirection Test (DART) Mission
dc.type
Wissenschaftlicher Artikel
dcterms.bibliographicCitation.doi
10.3847/PSJ/ac91cc
dcterms.bibliographicCitation.journaltitle
The Planetary Science Journal
dcterms.bibliographicCitation.number
11
dcterms.bibliographicCitation.originalpublishername
The American Astronomical Society
dcterms.bibliographicCitation.volume
3
dcterms.bibliographicCitation.url
https://doi.org/10.3847/PSJ/ac91cc
refubium.affiliation
Geowissenschaften
refubium.affiliation.other
Institut für Geologische Wissenschaften / Fachrichtung Planetologie und Fernerkundung

refubium.resourceType.isindependentpub
no
dcterms.accessRights.openaire
open access
dcterms.isPartOf.eissn
2632-3338
refubium.resourceType.provider
DeepGreen