DART Mission Determination of Momentum Transfer: Model of Ejecta Plume Observations
Andrew F. Cheng, Angela M. Stickle, Eugene G. Fahnestock, Elisabetta, Dotto, Vincenzo Della Corte, Nancy L. Chabot, Andrew S. Rivkin

TL;DR
This paper models the ejecta plume from the DART asteroid impact to help determine momentum transfer, using imaging data to infer physical properties and improve planetary defense strategies.
Contribution
It develops a model for impact ejecta plume optical depth and demonstrates how plume images can infer ejecta mass, velocity distribution, and target properties.
Findings
Plume images can distinguish impact strength and gravity-controlled regimes.
Model helps infer ejecta mass and velocity distribution from optical depth profiles.
Plume evolution analysis informs target physical properties and momentum transfer.
Abstract
The NASA Double Asteroid Redirection Test (DART) spacecraft will impact the secondary member of the [65803] Didymos binary in order to perform the first demonstration of asteroid deflection by kinetic impact. Determination of the momentum transfer to the target body from the kinetic impact is a primary planetary defense objective, using ground-based telescopic observations of the orbital period change of Didymos and imaging of the DART impact ejecta plume by the LICIACube cubesat, along with modeling and simulation of the DART impact. LICIACube, contributed by the Italian Space Agency, will perform a flyby of Didymos a few minutes after the DART impact, to resolve the ejecta plume spatial structure and to study the temporal evolution. LICIACube ejecta plume images will help determine the vector momentum transfer from the DART impact, by determining or constraining the direction and the…
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