Long-term evolution of Galileo operational orbits by canonical perturbation theory

  1. Lara, M. 1
  2. San-Juan, J.F. 2
  3. Cefola, P. 3
  1. 1 Real Observatorio de la Armada, San Fernando, Spain
  2. 2 Universidad de La Rioja
    info

    Universidad de La Rioja

    Logroño, España

    ROR https://ror.org/0553yr311

  3. 3 University at Buffalo, State University of New York
    info

    University at Buffalo, State University of New York

    Búfalo, Estados Unidos

    ROR https://ror.org/01y64my43

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Libro:
62nd International Astronautical Congress 2011, IAC 2011

ISBN: 978-161839805-5

Año de publicación: 2011

Volumen: 6

Páginas: 4815-4825

Tipo: Capítulo de Libro

SCOPUS: 2-s2.0-84864098488 GOOGLE SCHOLAR

Resumen

Galileo operational orbits are slightly affected by the 3 to 5 tesseral resonance, an effect that can be much more important in the case of disposal orbits. Proceeding by canonical perturbation theory we show that the part of the long-term Hamiltonian corresponding to the non-centralities of the Earth's gravitational potential can be replaced by an intermediary that shows the pendulum dynamics of the 3 to 5 tesseral resonance problem. Inclusion of lunisolar perturbations requires a semi-analytical integration, which is compared with corresponding results of the well established Draper Semi-analytical Satellite Theory. Copyright ©2011 by the International Astronautical Federation. All rights reserved.