Saturn's ring and nearby faint satellites

Details Saturn's ring and nearby faint satellites Saturn's ring and nearby faint satellites

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978icar...36...92f&link_type=abstract

Icarus, vol. 36, Oct. 1978, p. 92-106.

Other

14

Depth Measurement, Light Scattering, Natural Satellites, Optical Thickness, Saturn Rings, Albedo, Astronomical Photography, Data Reduction, Orbit Calculation, Solar System, Saturn, Rings, Satellites, Photometry, Thickness, Scattering, Optical Properties, Depths, Imagery, Data Reduction, Photography, Orbits, Earth, Calibrations, Earth-Based Observations

Scientific paper

Observations of Saturn's rings during passage of the Earth through the ring plane, coupled with those of others, suggest a ring thickness of 1.3 plus or minus 0.3 km. The wide disparity in the optical depth of Cassini's division found by other investigators is resolved, and for conservative isotropic single scattering, a normal optical depth for Cassini's division of 0.060 plus or minus 0.006 is obtained. We find the mean normal optical depth of ring C to be 0.074 plus or minus 0.007. Analysis of all available observations of faint objects near Saturn indicates the presence of at least one previously undiscovered satellite of Saturn. The orbit for Janus determined by Dollfus is supported. These satellites may be major members of an extended ring.

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