Energy Dissipation in Synchronous Binary Asteroids
Alex J. Meyer, Daniel J. Scheeres, Harrison F. Agrusa, Guillaume, Noiset, Jay McMahon, \"Ozg\"ur Karatekin, Masatoshi Hirabayashi, Ryota Nakano

TL;DR
This paper models energy dissipation in synchronous binary asteroids, revealing how system configurations and material properties influence libration damping and orbital evolution, which is crucial for asteroid impact assessment and deflection strategies.
Contribution
It introduces a numeric model to analyze energy dissipation in binary asteroids, highlighting the effects of libration, eccentricity, and material stiffness on their long-term dynamics.
Findings
Tumbling within the synchronous state affects short-term libration damping.
Damping rates depend on the secondary's stiffness.
Hera can potentially measure libration damping to infer tidal properties.
Abstract
Synchronous binary asteroids can experience libration about their tidally-locked equilibrium, which will result in energy dissipation. This is an important topic to the Asteroid Impact and Deflection Assessment, where excitation caused by the DART kinetic impact in the Didymos binary asteroid system may be reduced through dissipation before Hera arrives to survey the effects of the impact. We develop a numeric model for energy dissipation in binary asteroids to explore how different system configurations affect the rate of energy dissipation. We find tumbling within the synchronous state eliminates a systematic trend in libration damping on short timescales (several years), but not over long times (hundreds of years) depending on the material conditions. Furthermore, damping of libration, eccentricity, and fluctuations in the semimajor axis are primarily dependent on the stiffness of…
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