Ontology type: schema:ScholarlyArticle
2006-03
AUTHORSMatthew S. Tiscareno, Joseph A. Burns, Matthew M. Hedman, Carolyn C. Porco, John W. Weiss, Luke Dones, Derek C. Richardson, Carl D. Murray
ABSTRACTPropelled into the limelightSaturn's ring system consists in the main of countless icy particles a few centimetres to 10 metres or so in radius. Between these and the kilometre-size moonlets Pan and Daphnis, theorists predict a population of moonlets 40–120 metres in diameter. This is too small for Cassini's cameras to see. But 100-metre-diameter moonlets have now been observed indirectly, through the ‘wake’ they leave: propeller-shaped perturbations in the ring. These features are brighter than the surrounding region of the ring: so far four have been observed but the total moonlet population could run into millions. More... »
PAGES648-650
http://scigraph.springernature.com/pub.10.1038/nature04581
DOIhttp://dx.doi.org/10.1038/nature04581
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PUBMEDhttps://www.ncbi.nlm.nih.gov/pubmed/16572165
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