Density waves in Saturn's rings

Details Density waves in Saturn's rings Density waves in Saturn's rings

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.292..703c&link_type=abstract

Nature, vol. 292, Aug. 20, 1981, p. 703-707.

Physics

61

Density Wave Model, Planetology, Saturn Rings, Iapetus, Spaceborne Photography, Voyager 1 Spacecraft, Saturn, Rings, Density, Waves, Brightness, Cassini Division, Amplitude, Iapetus, Surface, Kinematics, Viscosity, Theoretical Studies, Mimas, Observations, Wavelengths, Physical Properties, Photometry, Satellites, Optical Properties, Titan, Resonance, Gravity Effects, Scattering

Scientific paper

Certain radial brightness variations in the outer Cassini division of Saturn's rings may be spiral density waves driven by Saturn's large moon Iapetus, in which case a value of approximately 16 g/sq cm for the surface density is calculated in the region where the waves are seen. The kinematic viscosity in the same region is approximately 170 sq cm/s and the vertical scale height of the ring is estimated to be a maximum of approximately 40 m.

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