The 1966 observations of the coorbiting satellites of Saturn, S10 and S11

Details The 1966 observations of the coorbiting satellites of Saturn, S10 and S11 The 1966 observations of the coorbiting satellites of Saturn, S10 and S11

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981icar...46..175l&link_type=abstract

Icarus, vol. 46, May 1981, p. 175-180.

Physics

13

Orbit Calculation, Planetary Orbits, Saturn Rings, Saturn Satellites, Gravitational Effects, Mimas, Saturn, Satellites, Coorbitals, Observations, S10, S11, Orbits, Data, Motion, Position (Location), Photographic Observations, Nomenclature

Scientific paper

Most of the positions of faint satellite images obtained during the 1966 Saturn ring plane crossing fit the period of the coorbital satellites 1980 S1 and 1980 S3. In 1966 the satellites were separated by 137 deg in orbital longitude. Until the mutual interaction of the satellites is understood and applied to derive the precise orbital motion, the 1966 and 1980 observations cannot be linked.

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