Dynamical investigation of minor resonances for space debris
Alessandra Celletti, Catalin Gales

TL;DR
This paper analyzes the dynamics of space debris near minor resonances using Hamiltonian models, identifying resonance structures, bifurcations, and validating results with numerical simulations including external perturbations.
Contribution
It introduces a Hamiltonian-based method to identify dominant resonant terms and predict resonance overlap and bifurcations in space debris dynamics.
Findings
Resonance islands and their amplitudes are characterized mathematically.
Conditions for resonance splitting and overlapping are established.
Numerical simulations confirm the analytical predictions with additional perturbations.
Abstract
We study the dynamics of the space debris in regions corresponding to minor resonances; precisely, we consider the resonances 3:1, 3:2, 4:1, 4:3, 5:1, 5:2, 5:3, 5:4, where a j:l resonance (with j, l integers) means that the periods of revolution of the debris and of rotation of the Earth are in the ratio j/l. We consider a Hamiltonian function describing the effect of the geopotential and we use suitable finite expansions of the Hamiltonian for the description of the different resonances. In particular, we determine the leading terms which dominate in a specific orbital region, thus limiting our computation to very few harmonics. Taking advantage from the pendulum-like structure associated to each term of the expansion, we are able to determine the amplitude of the islands corresponding to the different harmonics. By means of simple mathematical formulae, we can predict the occurrence…
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