Long-term evolution of space debris under the \(J_2\) effect, the solar radiation pressure and the solar and lunar perturbations

DOI10.1007/S10569-015-9644-1zbMath1428.70025OpenAlexW1943385431MaRDI QIDQ748295

Daniel Casanova, Alexis Petit, Anne Lemaitre

Publication date: 20 October 2015

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10569-015-9644-1

zbMATH Keywords

Hamiltonian formulationsolar radiation pressurethird body perturbationspace debrislong-term evolution\(J_2\) effectPoincaré's variables

Mathematics Subject Classification ID

Celestial mechanics (70F15)

Related Items (8)

Proper elements for space debris ⋮ Dynamics of highly eccentric and highly inclined space debris ⋮ Old perturbative methods for a new problem in celestial mechanics: the space debris dynamics ⋮ Nekhoroshev estimates for the orbital stability of Earth's satellites ⋮ Secular dynamics around small bodies with solar radiation pressure ⋮ Observing Mercury by a quasi-propellantless mission ⋮ Phase space description of the dynamics due to the coupled effect of the planetary oblateness and the solar radiation pressure perturbations ⋮ Geostationary secular dynamics revisited: application to high area-to-mass ratio objects

Cites Work

• Collision risk against space debris in Earth orbits
• A web of secondary resonances for large \(A/m\) geostationary debris
• Fundamentals of astrodynamics and applications. With technical contributions by Wayne D. McClain.

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