Ejecta cloud from the AIDA space project kinetic impact on the secondary of a binary asteroid: I. mechanical environment and dynamical model
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This paper aims at an understanding of the ejecta cloud dynamics, which is crucial to the planning of the ongoing AIDA mission.

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An informative dynamic model has been built to synthesize all relevant forces based on comprehensive analysis.

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A full-scale simulation was organized towards the response of Didymos to DART impact and the following month-long evolution of the ejecta cloud.

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Some interesting results about the post-impact physics have been uncovered according to the simulation.

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