The dynamics of the Saturnian satellites 1980S1 and 1980S3

Details The dynamics of the Saturnian satellites 1980S1 and 1980S3 The dynamics of the Saturnian satellites 1980S1 and 1980S3

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981icar...47...97h&link_type=abstract

Icarus, vol. 47, July 1981, p. 97-99.

Physics

15

Librational Motion, Motion Stability, Planetary Orbits, Saturn Satellites, Axes Of Rotation, Dynamic Models, Saturn Rings, Saturn, Satellites, Dynamics, 1980S1, 1980S3, Orbits, Longitude, Motion, Libration, S11, S10, Perturbations, Models

Scientific paper

The orbits of the Saturnian satellites 1980S1 and 1980S3 have
approximately the same semimajor axes, but the difference in longitude
librates between values of approximately +6 deg and -6 deg in 3000 days.
Thus the satellites never approach extreme proximity and the orbits
appear to be stable for extended periods of time.

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