The stable regions of motion of the natural satellites in the solar system.

Details The stable regions of motion of the natural satellites in the solar system. The stable regions of motion of the natural satellites in the solar system.

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppmto..12...37l&link_type=abstract

Publ. Purple Mt. Obs., Vol. 12, No. 1, p. 37 - 44

Physics

Planetary Satellites: Orbit Stability

Scientific paper

The problem of the stable regions of motion of the natural satellites in the solar system is discussed and an explanation about the reason that there exists a larger stable region for the motion of retrograde satellites is given. Based on the model of the circular restricted three-body problem consisting of Sun-planet-satellite, it is discussed whether each of the satellites in the solar system is situated in the stable region or not.

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