Resonant dynamics of medium Earth orbits: space debris issues
From MaRDI portal
Publication:1931799
DOI10.1007/s10569-008-9121-1zbMath1254.70041OpenAlexW2077583177WikidataQ114016748 ScholiaQ114016748MaRDI QIDQ1931799
Publication date: 16 January 2013
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10569-008-9121-1
Related Items (10)
Bifurcation of Lunisolar Secular Resonances for Space Debris Orbits ⋮ Analytical development of the lunisolar disturbing function and the critical inclination secular resonance ⋮ Nekhoroshev estimates for the orbital stability of Earth's satellites ⋮ To the substantiation of a numerical-analytical method for revealing secular resonances ⋮ Circular and zero-inclination solutions for optical observations of Earth-orbiting objects ⋮ On the dynamics of space debris: 1:1 and 2:1 resonances ⋮ On the predictability and robustness of Galileo disposal orbits ⋮ Dynamical investigation of minor resonances for space debris ⋮ A deep dive into the \(2g+h\) resonance: separatrices, manifolds and phase space structure of navigation satellites ⋮ Space Debris Long Term Dynamics
Cites Work
- Unnamed Item
- Long-period variations of the eccentricity vector valid also for near circular orbits around a non-spherical body
- An analytical solution of the Lagrange equations valid also for very low eccentricities: influence of a central potential
- Collision risk against space debris in Earth orbits
- Lunisolar apsidal resonances at low satellite orbits
- On the motion of a satellite in resonance with its rotating planet
- Tesseral resonance effects on satellite orbits
- The prograde C7 resonance for Earth and Mars satellite orbits
- On the coupling of luni-solar resonances for Earth satellite orbits
- Lunisolar resonances revisited
This page was built for publication: Resonant dynamics of medium Earth orbits: space debris issues