Rotation-induced granular motion on the secondary component of binary asteroids: Application to the DART impact on Dimorphos
Harrison Agrusa, Ronald Ballouz, Alex J. Meyer, Elisa Tasev, Guillaume, Noiset, \"Ozgur Karatekin, Patrick Michel, Derek C. Richardson, Masatoshi, Hirabayashi

TL;DR
This study models how the DART impact on Dimorphos could induce complex spin states, leading to surface granular motion due to varying accelerations, with broader implications for binary asteroid systems.
Contribution
It introduces a comprehensive 3D simulation of post-impact dynamical evolution and surface effects on binary asteroid secondaries, highlighting potential surface refreshment mechanisms.
Findings
Excited spin states can cause significant surface slope changes.
Granular motion may be triggered by dynamical excitation.
Effect depends on shape, density, and geology of the asteroid.
Abstract
NASA's Double Asteroid Redirection Test (DART) mission will kinetically impact Dimorphos, the secondary component of the Didymos binary asteroid system, which will excite Dimorphos's dynamical state and lead to significant libration about the synchronous state and possibly chaotic non-principal axis rotation. Although this particular outcome is human caused, many other secondary components of binary systems are also prone to such exotic spin states. For a satellite in an excited spin state, the time-varying tidal and rotational environment can lead to significant surface accelerations. Depending on the circumstances, this mechanism may drive granular motion on the surface of the secondary. We modeled the dynamical evolution of a Didymos-like binary asteroid system using a fully coupled, three-dimensional simulation code. Then, we computed the time-varying gravitational and rotational…
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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Geology and Paleoclimatology Research
