About the eccentricity growth of MEO orbits

Details About the eccentricity growth of MEO orbits About the eccentricity growth of MEO orbits

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf...87d&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

Scientific paper

The main characteristic of the long term evolution of MEO objects lies in the growth of their eccentricity, which can rise up to 0.7, or even more, during the typical time scale of 200 years. This characteristic has to be accounted for mission analysis of projects such as the european navigation system Galileo. It can be precisely studied with a numerical integration of the averaged equations of motion.

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