We study the presence of resonances in the region of space around the Earth.
We consider a massless body (e.g, a dust particle or a small space debris)
subject to different forces: the gravitational attraction of the geopotential,
the effects of Sun and Moon. We distinguish different types of resonances:
tesseral resonances are due to a commensurability involving the revolution of
the particle and the rotation of the Earth, semi-secular resonances include the
rates of variation of the mean anomalies of Moon and Sun, while secular
resonances just depend on the rates of variation of the arguments of perigee
and the longitudes of the ascending nodes of the perturbing bodies. We
characterize such resonances, giving precise statements on the regions where
the resonances can be found and provide examples of some specific
commensurability relations.Comment: 38 pages, 9 figures, submitted to Communications in Nonlinear Science
and Numerical Simulatio