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Gravitational Vortices And Clump Formation In Saturn's F ring During An Encounter With Prometheus

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 en...

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Autores principales: Sutton, Phil J., Kusmartsev, Feodor V.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group 2013
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3572473/
https://www.ncbi.nlm.nih.gov/pubmed/23429480
http://dx.doi.org/10.1038/srep01276
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author Sutton, Phil J.
Kusmartsev, Feodor V.
author_facet Sutton, Phil J.
Kusmartsev, Feodor V.
author_sort Sutton, Phil J.
collection PubMed
description 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.
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spelling pubmed-35724732013-02-14 Gravitational Vortices And Clump Formation In Saturn's F ring During An Encounter With Prometheus Sutton, Phil J. Kusmartsev, Feodor V. Sci Rep Article 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. Nature Publishing Group 2013-02-14 /pmc/articles/PMC3572473/ /pubmed/23429480 http://dx.doi.org/10.1038/srep01276 Text en Copyright © 2013, Macmillan Publishers Limited. All rights reserved http://creativecommons.org/licenses/by-nc-sa/3.0/ This work is licensed under a Creative Commons Attribution-NonCommercial-ShareALike 3.0 Unported License. To view a copy of this license, visit http://creativecommons.org/licenses/by-nc-sa/3.0/
spellingShingle Article
Sutton, Phil J.
Kusmartsev, Feodor V.
Gravitational Vortices And Clump Formation In Saturn's F ring During An Encounter With Prometheus
title Gravitational Vortices And Clump Formation In Saturn's F ring During An Encounter With Prometheus
title_full Gravitational Vortices And Clump Formation In Saturn's F ring During An Encounter With Prometheus
title_fullStr Gravitational Vortices And Clump Formation In Saturn's F ring During An Encounter With Prometheus
title_full_unstemmed Gravitational Vortices And Clump Formation In Saturn's F ring During An Encounter With Prometheus
title_short Gravitational Vortices And Clump Formation In Saturn's F ring During An Encounter With Prometheus
title_sort gravitational vortices and clump formation in saturn's f ring during an encounter with prometheus
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3572473/
https://www.ncbi.nlm.nih.gov/pubmed/23429480
http://dx.doi.org/10.1038/srep01276
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