Relative motion near the triangular libration points in the Earth-Moon system

Details Relative motion near the triangular libration points in the Earth-Moon system Relative motion near the triangular libration points in the Earth-Moon system

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.273..157s&link_type=abstract

In ESA, ESA Workshop on Optical Interferometry in Space p 157-170 (SEE N88-10613 01-74)

Physics

Earth-Moon System, Libration, Spacecraft Motion, Interferometry, Orbital Mechanics, Trajectory Analysis

Scientific paper

As the triangular libration points in the Earth-Moon system are of potential interest for optical interferometry, their dynamical property was analyzed adopting realistic models. Quasi-periodic orbits were identified, and their stability investigated. Results show that relative motion leads to baseline variation of 1 to 20 cm/sec, which may be unacceptably large for optical interferometry.

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