Gravitational vortices and clump formation in Saturn's F ring during an encounter with Prometheus.

Sci Rep

Astronomy Unit, Physics Department, Loughborough University, Loughborough, Leicestershire LE11 3TU, UK.

Published: August 2013

Saturn rings are most beautiful and dynamic places in the solar system, consisting of ice particles in a constant battle between the gravitational forces of Saturn and its many moons. Fan, spiral, propellers, moonlets and streamer-channels observed by CASSINI in the F-ring have been attributed to encounters by Prometheus on the F ring, with investigations of optical thickness revealing large populations of transient moonlets. Taking into account gravitational interaction between particles and a multi-stranded F-ring structure we show that Prometheus' encounters create rotational flows, like atmospheric vortices and the self-gravity enhances the accelerated growth and size of moonlets. Vortex patches form caustics, which is a primary cause of the transient particle density clumps of 20 km width and 100 km length, and they are elongated to cover an area of 1600 km by 150 km, which may eventually combine into a vortex sheet.

Download full-text PDF

Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC3572473PMC
http://dx.doi.org/10.1038/srep01276DOI Listing

Publication Analysis

Top Keywords

gravitational vortices
4
vortices clump
4
clump formation
4
formation saturn's
4
saturn's ring
4
ring encounter
4
encounter prometheus
4
prometheus saturn
4
saturn rings
4
rings beautiful
4

Similar Publications

Want AI Summaries of new PubMed Abstracts delivered to your In-box?

Enter search terms and have AI summaries delivered each week - change queries or unsubscribe any time!