Are the analytical proper elements of asteroids still needed?

DOI10.1007/S10569-019-9906-4zbMath1451.70045OpenAlexW2948701637MaRDI QIDQ2005626

Andrea Milani, Zoran Knežević

Publication date: 8 October 2020

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

Full work available at URL: https://doi.org/10.1007/s10569-019-9906-4

zbMATH Keywords

dynamicsasteroidsproper elementssecular resonances

Mathematics Subject Classification ID

Orbital mechanics (70M20)

Related Items (3)

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

Cites Work

• Unnamed Item
• Secular perturbation theory and computation of asteroid proper elements
• Secular resonances in the asteroid belt: Theoretical perturbation approach and the problem of their location
• The main secular resonances \(\nu{}_ 6,\nu{}_ 5\) and \(\nu{}_{16}\) in the asteroid belt
• Proper elements for highly inclined asteroidal orbits
• The convergence domain of the Laplacian expansion of the disturbing function
• Theory of Orbit Determination
• Synthetic proper elements for outer main belt asteroids

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