Using a recently introduced synthetic method to compute the asteroid secular
frequencies (Knezevic and Milani 2019), in this paper we survey the
locations of secular resonances in the 9 dynamically distinct zones of the
asteroid belt. Positions of all resonances up to order four, of a significant
fraction of the order six resonances, and of a several order eight ones were
determined, plotted in the space of proper elements, and discussed in
relation to the local dynamics and to the structure and shape of the nearby
asteroid collisional families. Only the resonant combinations with
fundamental frequencies of Jupiter and Saturn were considered, with a few
special cases involving other planets and largest asteroids. Accuracy of the
polynomial fit to determine the frequencies was found to be satisfactory for
the purpose of determination of secular resonance positions. This enabled a
precise identification of dynamical mechanisms affecting the computation of
frequencies (close vicinity of the mean motion resonances and libration in
secular resonances), and of the \cycle slips" as a primary technical
drawback causing deterioration of the results. For each zone we also
presented and discussed a fairly complete sample of recent works dealing
with interaction of the secular resonances with asteroid families present in
that zone. Finally, a few words were devoted to possibilities for future
work.
The Distribution of Asteroidal Dust in the Inner Solar System
