Identification of resonance features within the rings of Saturn

Details Identification of resonance features within the rings of Saturn Identification of resonance features within the rings of Saturn

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982natur.297..115h&link_type=abstract

Nature, vol. 297, May 13, 1982, p. 115-120.

Astronomy and Astrophysics

Astronomy

83

Resonance, Saturn Rings, Saturn Satellites, Stellar Occultation, Ultraviolet Astronomy, Optical Thickness, Planetary Orbits, Voyager 2 Spacecraft, Wave Propagation, Saturn, Rings, Resonance, Features, Voyager 2, Ultraviolet, Wavelengths, Spectrometer, Occultations, Optical Properties, Depth, Density Waves, Patterns, Analysis, Density, Surface, Mass, C Ring, Distance, Source, Satellites, 1980S27, 1980S26, 1980S1, Mimas, Titan, Hyperion, Iapetus, Boundaries, Origin, Morphology, Cassini Division, A Ring, B Rin

Scientific paper

The Voyager 2 UV spectrometer observed a stellar occultation by the rings of Saturn, which located ring features with an accuracy of 12 km. A high-resolution (3 km) optical depth atlas of the rings shows at least nine features, including four density wave patterns, identified with satellite resonances. Analysis of these density wave patterns yields the first surface mass densities for the A ring and, together with the optical depth atlas, a total ring mass of 6.4 x 10 to the -8th Saturn masses.

Affiliated with

Also associated with

No associations

Rating

Identification of resonance features within the rings of Saturn does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Identification of resonance features within the rings of Saturn, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Identification of resonance features within the rings of Saturn will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1101591