Special Features of the Structure of Secular Resonances in the Dynamics of Near-Earth Space Objects


Citar

Texto integral

Acesso aberto Acesso aberto
Acesso é fechado Acesso está concedido
Acesso é fechado Somente assinantes

Resumo

The special features of the structure of secular resonances in the near-earth orbital space bounded by the following range of orbital parameters: semimajor axis from 8000 to 55 000 km, inclination from 0 to 90°, and eccentricity equal to 0.01, 0.6, and 0.8 are analyzed. The influence of stable and unstable secular resonances on the long-term orbital evolution of near-earth space objects is also considered. It is demonstrated that the joint effect of the stable secular resonances of different spectral classes does not violate the regularity of motion. The chaoticity arises when stable secular resonances of one spectral class are imposed.

Sobre autores

T. Bordovitsyna

National Research Tomsk State University

Autor responsável pela correspondência
Email: tvbord@sibmail.com
Rússia, Tomsk

I. Tomilova

National Research Tomsk State University

Email: tvbord@sibmail.com
Rússia, Tomsk

Arquivos suplementares

Arquivos suplementares
Ação
1. JATS XML

Declaração de direitos autorais © Springer Science+Business Media New York, 2016