Your browser doesn't support javascript.
loading
Saturn's F ring is intermittently shepherded by Prometheus.
Cuzzi, Jeffrey N; Marouf, Essam A; French, Richard G; Murray, Carl D; Cooper, Nicholas J.
Afiliação
  • Cuzzi JN; Ames Research Center, NASA, Moffett Field CA 94035, USA.
  • Marouf EA; San Jose State University, San Jose, CA, USA.
  • French RG; Wellesley College, Wellesley, MA, USA.
  • Murray CD; Queen Mary University of London, London, UK.
  • Cooper NJ; Queen Mary University of London, London, UK.
Sci Adv ; 10(19): eadl6601, 2024 May 10.
Article em En | MEDLINE | ID: mdl-38728405
ABSTRACT
One of the stranger planetary rings is Saturn's narrow, clumpy F ring, lying just outside the main rings, in a region disturbed by chaotic orbital dynamics. We show that the F ring has a stable "true core" that dominates its mass and is confined into discontinuous short arcs of particles larger than a few millimeters in radius. The more obvious micron-size particles seen in images, outlining and obscuring the true core, contribute only a small fraction of its mass. We found that these arcs of large particles orbit Saturn in a specific corotational resonance with the nearby 100-kilometer diameter ringmoon Prometheus, which stabilizes the F ring material and allows it to persist within the disturbed region for decades or longer. Toward the end of the observing period, a small chaotic glitch in the orbit of Prometheus temporarily disrupted the confinement, but the arcs seem to be able to adapt.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article