Is the chaotic clock ticking correctly?

Astronomy and Astrophysics – Astronomy

Scientific paper

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Minor Planets: Families, Minor Planets: Ages, Minor Planets: Orbit Stability, Minor Planets: Chaos

Scientific paper

The authors performed an extensive analysis of the dynamics of all presently known members of the Veritas asteroid family, in order to check the estimate of its age given originally by Milani and Farinella (1994), who used the so-called "chaotic chronology" method for this purpose. The authors started from a much larger sample of family members and carried out many more numerical integrations of the entire family and, in particular, of the chaotic bodies. They show that the dynamics in the region of the phase space occupied by the family is more complex than previously believed, and that there are bodies with motions ranging from remarkable stability to strong chaos. Seven strongly chaotic bodies exhibit a qualitatively similar behavior, in agreement with the predictions of Milani et al. (1996), but also a number of previously unknown features. Although, in general, the authors' results do not contradict the conclusions of Milani and Farinella and fit reasonably well with their estimate of the family age, there are also some interesting results of this analysis, which open new questions and require a more thorough and dedicated investigation.

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