BYORP and Dissipation in Binary Asteroids: Lessons from DART
Matija \'Cuk, Harrison Agrusa, Rachel H. Cueva, Fabio Ferrari,, Masatoshi Hirabayashi, Seth A. Jacobson, Jay McMahon, Patrick Michel, Paul, S\'anchez, Daniel J. Scheeres, Stephen Schwartz, Kevin J. Walsh, and Yun, Zhang

TL;DR
This paper analyzes data from the DART mission to understand the BYORP effect and dissipation processes in binary asteroids, proposing new models for their evolution and response to impacts.
Contribution
It introduces revised paradigms for BYORP and dissipation in small binary asteroids based on recent observational data from DART.
Findings
Dimorphos has a prolate shape post-impact.
Spheroidal bodies may experience weaker, size-dependent BYORP effects.
Energy dissipation occurs in brief episodes of material movement.
Abstract
The Near-Earth binary asteroid Didymos was the target of a planetary defense demonstration mission DART in September 2022. The smaller binary component, Dimorphos, was impacted by the spacecraft in order to measure momentum transfer in kinetic impacts into rubble piles. DART and associated Earth-based observation campaigns have provided a wealth of scientific data on the Didymos-Dimorphos binary. DART revealed a largely oblate and ellipsoidal shape of Dimorphos before the impact, while the post-impact observations suggest that Dimorphos now has a prolate shape. Here we add those data points to the known properties of small binary asteroids and propose new paradigms of the radiative binary YORP (BYORP) effect as well as tidal dissipation in small binaries. We find that relatively spheroidal bodies like Dimorphos made of small debris may experience a weaker and more size-dependent BYORP…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
