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The Dynamical State of the Didymos System before and after the DART Impact

Authors :
Derek C. Richardson
Harrison F. Agrusa
Brent Barbee
Rachel H. Cueva
Fabio Ferrari
Seth A. Jacobson
Rahil Makadia
Alex J. Meyer
Patrick Michel
Ryota Nakano
Yun Zhang
Paul Abell
Colby C. Merrill
Adriano Campo Bagatin
Olivier Barnouin
Nancy L. Chabot
Andrew F. Cheng
Steven R. Chesley
R. Terik Daly
Siegfried Eggl
Carolyn M. Ernst
Eugene G. Fahnestock
Tony L. Farnham
Oscar Fuentes-Muñoz
Edoardo Gramigna
Douglas P. Hamilton
Masatoshi Hirabayashi
Martin Jutzi
Josh Lyzhoft
Riccardo Lasagni Manghi
Jay McMahon
Fernando Moreno
Naomi Murdoch
Shantanu P. Naidu
Eric E. Palmer
Paolo Panicucci
Laurent Pou
Petr Pravec
Sabina D. Raducan
Andrew S. Rivkin
Alessandro Rossi
Paul Sánchez
Daniel J. Scheeres
Peter Scheirich
Stephen R. Schwartz
Damya Souami
Gonzalo Tancredi
Paolo Tanga
Paolo Tortora
Josep M. Trigo-Rodríguez
Kleomenis Tsiganis
John Wimarsson
Marco Zannoni
Source :
The Planetary Science Journal, Vol 5, Iss 8, p 182 (2024)
Publication Year :
2024
Publisher :
IOP Publishing, 2024.

Abstract

NASA’s Double Asteroid Redirection Test (DART) spacecraft impacted Dimorphos, the natural satellite of (65803) Didymos, on 2022 September 26, as a first successful test of kinetic impactor technology for deflecting a potentially hazardous object in space. The experiment resulted in a small change to the dynamical state of the Didymos system consistent with expectations and Level 1 mission requirements. In the preencounter paper, predictions were put forward regarding the pre- and postimpact dynamical state of the Didymos system. Here we assess these predictions, update preliminary findings published after the impact, report on new findings related to dynamics, and provide implications for ESA’s Hera mission to Didymos, scheduled for launch in 2024 October with arrival in 2026 December. Preencounter predictions tested to date are largely in line with observations, despite the unexpected, flattened appearance of Didymos compared to the radar model and the apparent preimpact oblate shape of Dimorphos (with implications for the origin of the system that remain under investigation). New findings include that Dimorphos likely became prolate due to the impact and may have entered a tumbling rotation state. A possible detection of a postimpact transient secular decrease in the binary orbital period suggests possible dynamical coupling with persistent ejecta. Timescales for damping of any tumbling and clearing of any debris are uncertain. The largest uncertainty in the momentum transfer enhancement factor of the DART impact remains the mass of Dimorphos, which will be resolved by the Hera mission.

Details

Language :
English
ISSN :
26323338
Volume :
5
Issue :
8
Database :
Directory of Open Access Journals
Journal :
The Planetary Science Journal
Publication Type :
Academic Journal
Accession number :
edsdoj.3fc1326af2ec4d04951b011e0b48c210
Document Type :
article
Full Text :
https://doi.org/10.3847/PSJ/ad62f5