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Multiple mass shedding events explain diverse binary asteroid systems, including unusual configurations like Selam. This multi-generation satellite formation model reveals a richer history for many asteroid binaries.

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Area of Science:

  • * Planetary Science
  • * Astronomy
  • * Solar System Dynamics

Background:

  • * Binary asteroid systems are common, often forming from rotational breakup.
  • * Expected satellite configurations (prolate, compact orbits) differ from observed diversity.
  • * The contact-binary satellite Selam around (152830) Dinkinesh presents a unique case.

Purpose of the Study:

  • * To propose a unified framework explaining diverse binary asteroid configurations.
  • * To investigate the influence of multi-generation satellites on formation pathways.
  • * To analyze the dynamical histories of specific systems like Dinkinesh.

Main Methods:

  • * Theoretical modeling of mass shedding and satellite formation.
  • * Simulation of disk-satellite and inter-satellite interactions.
  • * Analysis of existing binary asteroid system configurations.

Main Results:

  • * Multiple mass shedding episodes and multi-generation satellites offer a unified explanation.
  • * Pre-existing satellites significantly alter subsequent satellite formation.
  • * The model successfully explains the Dinkinesh system and some triple systems.
  • * Approximately 44% of known binaries show evidence of multi-satellite histories.

Conclusions:

  • * Multi-generation satellite formation is a key mechanism for diverse binary asteroid systems.
  • * This mechanism reconciles expected and observed configurations.
  • * Further discoveries of diverse binary asteroid configurations are anticipated.