On the nature of regularities in the radial structure of Saturnian rings

Details On the nature of regularities in the radial structure of Saturnian rings On the nature of regularities in the radial structure of Saturnian rings

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..245g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 245-247

Physics

Scientific paper

The theory [1] based on the consideration of a cosmic planetary system (PS) as a spatially limited oscillating system with many degrees of freedom predicts the formation of annular features of the type of radial standing waves (SW). The gravitating matter consisting bodies (satellites) of different sizes accumulates itself in the SW nodes and loops as in peculiar traps. The matter of Saturnian system that consists of different bodies is of undoubted interest from this point of view. The theory permits to obtain a wave length (WL) of the principal mode of SW in dependence on the central body's mass M: a = β M7/9, where β is the integrating constant. In particular for the system of Saturn ah = 74739 km.

Affiliated with

Also associated with

No associations

Rating

On the nature of regularities in the radial structure of Saturnian rings 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 On the nature of regularities in the radial structure of Saturnian rings, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the nature of regularities in the radial structure of Saturnian rings will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1386805