Resonant Structure of the THEMIS Asteroid Family

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The existence of resonant structure associated with low-order Jovian mean-motion commensurabilities within the main asteroid belt is already well established. However, previous studies have also suggested evidence for gaps within individual asteroid families. Whereas the Kirkwood gaps in the main asteroid belt are known to result from the actual removal of asteroids from resonant locations, it is not clear if this is also the case for the gaps evident within asteroid families. Indeed, the fact that asteroid families are identified by clustering in proper element space prompted Dermott & Murray (1981) to suggest that some of these gaps might only result from a failure to identify asteroids undergoing resonant perturbations as family members. We have investigated this hypothesis for the particular case of the Themis family of asteroids by numerically integrating the orbits of a carefully created artificial asteroid family. The orbital elements for this artificial family were constructed with proper element distributions closely resembling those of the actual Themis family but with any resonant structure removed. These orbits were then evolved to determine whether asteroids were indeed being removed from resonant locations and to monitor the mechanisms by which this occurred. We present evidence which indicates that the 2:1 Jovian mean-motion resonance may have played an important role in depleting the original Themis asteroid family of some of its members.

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