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Table 3

Properties of the secular resonances appearing in the orbital dynamics of a massless satellite at first order in the solar perturbation.

Resonance angle ξ Nominal location cos I0 Constant quantity K
ωQ + ΩQ
2ωQ + ΩQ
ωQ
2ωQ − ΩQ
ωQ − ΩQ
ΩQ 0 e

Notes. The retrograde resonances are obtained by inverting the sign of cos I0 and of ΩQ.

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