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dc.contributor.authorBrodie, Ian
dc.contributor.authorArion, Douglas
dc.date.accessioned2011-02-08T15:38:27Z
dc.date.available2011-02-08T15:38:27Z
dc.date.created2011-01-30
dc.date.issued2011-02-08
dc.identifier.urihttp://hdl.handle.net/123456789/117
dc.descriptionResearch Posteren_US
dc.description.abstractChanges in the rings of Saturn are difficult to detect from Earth-based telescopes because of their fine composition. Particulate bodies, like planetary rings, demonstrate strange phenomena without obvious causes and are made further puzzling by only being viewed in 2 dimensions. Spacecraft such as the Voyager and Cassini satellites, along with a few lucky snapshots during equinoxes, have resolved some of these phenomena. Figure 1 shows a new moon discovered by Cassini during an equinox. [2].en_US
dc.subjectCarthageen_US
dc.subjectPhysicsen_US
dc.subjectAstronomyen_US
dc.titleWebcam Observation of Saturn's C-Ringen_US
dc.typePresentationen_US


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